To Mars with Mitch Schulte
Professor Carol Oliver
Peggy Whitson: First Female Space Station Commander
Valentina Tereshkova: First Woman in Space
World Space Week 2021
MethaneSAT, with the New Zealand Space Agency
Cosmic Star Safari announcement
AHiS 2021 – How to fertilise your seeds
AHiS 2021 – What to measure for your school project
AHiS 2021 – How to grow your basil

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To Mars with Mitch Schulte
NZAN Media Team, Mars, Mitch Schulte, Perseverance, 0
Learn about Mars and Perseverance with Mitch Schulte
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Professor Carol Oliver
NZAN Media Team, 0
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales Carol Oliver is an Associate Professor with...
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Peggy Whitson: First Female Space Station Commander
Caitlin MacArthur, first female space station commander, most time in space, peggy whitson, Women in Space, world space week, 0
Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight...
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Valentina Tereshkova: First Woman in Space
Caitlin MacArthur, valentina tereshkova, Women in Space, world space week, 0
In 1963, Valentina Tereshkova became the first woman in space when she launched aboard the Soviet space program’s Vostok...
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World Space Week 2021
I Haritina Mogoșanu, Maruška Strah, Women in Space, world space week, WSWA, 0
World Space Week 2021 is about women in space. We interviewed the Executive Director of the World Space Week...
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MethaneSAT, with the New Zealand Space Agency
NZAN Media Team, MethaneSAT, WSWA, 0
Learn about MethaneSAT, New Zealand's first official space mission as a country. The New Zealand Astrobiology Network interviewed Dr Peter...
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Cosmic Star Safari announcement
NZAN Media Team, astrobiology, Carterton District, Cosmic Star Safari, 0
Thanks to your support, one lucky school from the Carterton District gets a Cosmic Star Safari!
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AHiS 2021 – How to fertilise your seeds
I Haritina Mogoșanu, Fertiliser, iss, seeds in space, seeds in space 2021, 0
What to feed to your basil plants (aka fertilisers) and what has that got to do with stars.
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AHiS 2021 – What to measure for your school project
I Haritina Mogoșanu, iss, seeds in space, seeds in space 2021, 0
When you submit a report or a poster you get in the draw to win a planetarium visit to...
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AHiS 2021 – How to grow your basil
I Haritina Mogoșanu, basil, iss, seeds in space, seeds in space 2021, 0
Give your basil plenty of warmth and light. It grows well in a warm environment, with the optimum...
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.

Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
In 1963, Valentina Tereshkova became the first woman in space when she launched aboard the Soviet space program’s Vostok 6. To this day, she remains the only woman to have completed a solo space mission. The Vostok 6 mission lasted three days and orbited the Earth a total of 48 times.
Tereshkova was born in 1937 in the village of Bolshoye Maslennikovo in central Russia. Her father was killed in the Finnish Winter War, part of World War II, when she was two years old. She attended school up until age 17, after which she began working in the tyre and textile mill industries whilst completing correspondence courses at the Light Industry Technical School to continue her education. Outside of her work and studies, Tereshkova developed an interest in skydiving and completed her first jump when she was 22. It was her experience in skydiving that would lead to her selection as a cosmonaut.
The head of the Soviet cosmonaut training program, Nikolai Kamanin, decided as a part of the Space Race that the U.S.A. could not be the first to put a woman in space and begun the recruitment process for female cosmonauts. Criteria to be a female cosmonaut included being younger than 30, no taller than 170 centimetres, and having experience with parachuting. In 1962, five candidates were chosen to enter the cosmonaut training process including Valentina Tereshkova, Zhanna Yorkina, Irina Solovyeva, Valentina Ponomaryova, and Tatyana Kuznetsova. In May 1963, Valentina Tereshkova was selected to fly Vostok 6.
The Vostok 6 spacecraft was operated predominantly from the ground by the Soviet space program. During the mission, data was collected to help study the effects of spaceflight, such as the zero-gravity environment, on the female body. Photography carried out by Tereshkova during the mission was later used to study the atmosphere.
In the same year as the Vostok 6 mission, Tereshkova married the Soviet cosmonaut Andrian Nikolayev, and went on to have a daughter named Elena Andrianovna Nikolaeva-Tereshkova. Being the first child born to both a mother and father who had been exposed to space, Elena received a lot of medical interest. Following the Vostok 6 mission, Valentina Tereshkova went on to attain the rank of major general in the Air Force and to hold several political offices as a part of the Communist Party of the Soviet Union.
The New Zealand Astrobiology Network is the Country Coordinator for the World Space Week. Find out more from our page here. This year, the theme of the World Space Week is Women in Space.
Everyone can participate in the World Space Week, which is an international celebration of the advancements created by space activities.
To start the year, we interviewed Maruška Strah, Executive Director of the World Space Week who gives an overview of what World Space Week is about.
Learn about New Zealand's first official space mission as a country, MethaneSAT.
New Zealand will contribute with an Atmospheric science programme, funded from Catalyst: Strategic over 4 years and a Mission Operations Control Centre, funded from the Strategic Science Investment Fund.
In 2020, World Space Week’s theme was “Satellites Improve Life” and the New Zealand Astrobiology Network took this opportunity to interview Dr Peter Crabtree, Head of the NZ Space Agency, Dr Sara Mikaloff-Fletcher, NZ Lead Researcher for MethaneSAT and Dr. Steven Hamburg, Chief Scientist, EDF, as New Zealand joined its first official space mission to combat climate change. The interview was conducted by Haritina Mogoșanu, Executive Director of the New Zealand Astrobiology Network and held at Space Place at Carter Observatory in Wellington, during World Space Week 2020.
by it’s chemical formula CH4, methane is a powerful greenhouse gas, that contributes to global warming, as it traps heat 28 times more effectively than carbon dioxide over a 100-year timescale.
Methane is produced under conditions where little to no oxygen is available. About 30% of methane emissions are produced by wetlands, including ponds, lakes, and rivers. Another 20% is produced by agriculture, due to a combination of livestock, waste management and rice cultivation. Activities related to oil, gas, and coal extraction release an additional 30%.
Concentrations of methane have increased by more than 150% since industrial activities and intensive agriculture began. After carbon dioxide, methane was responsible for about 23% of climate change in the 20th century.
data compiled from MBIE’s MethaneSAT mission and NASA’s Video: Methane Sources
Transcript of the interview:
Haritina Mogoșanu: The World Space Week Association is the global coordinator For the World Space Week Under the guidance of the United Nations’ Committee on the Peaceful Uses of Outer Space COPUOUS and the United Nations office for Outer Space Affairs.
Every year, the World Space Week Association Board chooses a theme. In 2020, the theme was “Satellites Improve Life”. New Zealand has joined its first official space mission as a country to combat climate change. It’s called MethaneSAT, and the mission’s Control Centre will be located here in New Zealand. I’m here with Dr Peter Crabtree, the head of the New Zealand Space Agency and Dr Sara Mikaloff-Fletcher, Lead Researcher for the mission.
Kia Ora Peter and Sara, it is a real pleasure to have you here.
Kia Ora
Peter, what is MethaneSAT?
Dr. Peter Crabtree: MethaneSAT is a mission with the objective of sensing atmospheric methane concentrations. And so with the idea that we gain better information, about those concentrations, and that will enable people to make better decisions and to understand the phenomenon much better.
Why has New Zealand chosen a partnership with the Environmental Defence Fund in the US for our first official space mission?
Thank you, that’s a good question. There are two answers to that on the one hand we were thinking, prior to this, about doing something in the climate science area and that being a really good objective for New Zealand given our interest as a nation from a policy perspective and so on, and then, on the other hand, there was an opportunity that came towards us to participate and be a partner in a really cutting edge space mission that also was going to happen with what we thought was a reasonable time frame given the pace that we were moving at, which was quite quick. So the idea of working with an organisation that was going to be quite nimble in putting together a space mission, when sometimes some space missions can be put together over very long period of time, and we saw this as a real opportunity for New Zealand to step into something that was really quite a serious endeavour but something that could really assist us as a nation in quite a number of different ways.
Let’s cross over to Steven Hamburg from EDF, Steven could you please tell us a little bit more
Dr. Steven Hamburg: Hello Hari, Peter and Sara it’s great to be with you and it’s great to have an opportunity to talk about MethaneSAT a mission that I’m passionate about.
The idea of MethaneSAT started a few years ago in conversation between Steve Wofsy, a professor at Harvard University and myself about the need to be able to collect methane flux data, how much methane was being emitted from around the world, and we didn’t have that capacity and without that knowledge we really couldn’t take advantage of the opportunity to reduce methane emissions because we did not know where it was occurring.
So we determined what we would need from a satellite and then went to the technology experts and asked, could we push the envelope on the technology to build the capacity inflight in space. And while we were pushing the envelope, that technology has evolved and is now possible, and MethaneSAT is the product of that integration of new technology, innovative science and the inversion technology that Steve has pioneered, into a program that allows us to do the advocacy to bring that data to the rest of the world.
And EDF, the Environmental Defence Fund, is well situated to lead this effort. EDF was founded by a group of scientists who understood a problem but did not have the tools to implement the understanding into policy that resulted from that knowledge. And that initial problem was the impacts of DDT on birds of prey in eastern United States. So they got together and formed the Environmental Defence Fund, hired a lawyer and then, using their science, went to look at and implement the needed ban on DDT, which was implemented in the early 1970s.
So with methane emissions from oil and gas industry, we understand the impact it’s having on the climate but we didn’t have the tools to bring that data and understanding to the many oil and gas producing regions of the world so that we could reduce those emissions and greatly slow the rate of warming.
MethaneSAT is very different than many other missions in that as I mentioned we started with the problem, and then went to look at the solutions. Could the technologies provide the data necessary to address that problem? We build an amazing team led by Tom Ingersoll who comes out of the commercial space community, of people who are really committed to ensuring that you we can use space technology to help society address one of the biggest crisis we ever faced which is climate change. And so by getting the best of the space technology community together with the best of the scientific community, in partnership with New Zealand, which has been an incredible opportunity to really push this mission forward fast and implement it effectively, we are very much looking forward to the operation centre being in New Zealand and to getting the satellite launched and the data flowing so that we can start to figure out where those methane emissions are coming from and ensure that people understand how those emissions can be mitigated and in turn getting that job done.
New Zealand is a wonderful partner in that there is a real commitment to bringing good science to bear on the needs of society writ large and that is the mission of EDF and so we are really very pleased to have the partnership with the New Zealand Government and the science community.
We are partnering with New Zealand because it’s a real natural fit. The focus of the Ministry for Business, Innovation and Employment on the use of science to help improve New Zealand society and the well-being of your citizens fits wonderfully into the objectives of this mission and to the DNA of EDF as an organisation for these fifty plus years. So by taking advantage of the scientific knowledge that already exists in New Zealand and to help develop the nascent space capacity in the country we were able to accelerate progress on the mission while developing the skill sets in New Zealand. It’s a partnership that we very much value, and are confident will persist and enhance the work we are doing together over the coming years.
Thank you Steven.
I have a couple of questions for Sara
What is novel about the satellite mission?
Dr Sara Mikaloff-Fletcher: So many things.
It’s an amazing mission! I mean for me, on the technical side, there are two big things. One is that it’s the first time we’re going to have a satellite flying in the sky that’s going to be able to measure methane with the kind of precision we would expect to have of someone on my team tried to measure it with an instrument on the ground. That’s extraordinary! The other thing is the spatial resolution so this thing is going to capture a 200 x 200 km scene and within that scene is going to do a raster scan with very high precision so we will be able to pick up exactly where these emissions are happening; but then on the policy side, it’s the first satellite that’s been purposely designed to support and enable climate action.
So there are two big things happening there, one is that they are going to have inverse modelling as part of the whole framework, which is the modelling tool you used to go from what the satellite measures, which is the concentration, to what you need for policy action which is to know the emissions. So that’s going to be happening live throughout the satellite’s mission, and then in addition to that is the impact in communicating as quickly so that we can empower people to be able to reduce these emissions.
Tell me Sara,
What relevant expertise do we have here in New Zealand to contribute to MethaneSAT science?
Well we have quite a big going on in New Zealand. New Zealand has been a leader in greenhouse gas measurements, since before I was born. In fact, when I was a PhD student coming up at NOAA, which is kind of our opposite number in the US, NIWA was already famous to me for having the best methane isotopes almost anywhere in the world. And so we have this amazing rich history of these atmospheric measurements both on the ground and also in the total air column. So you can imagine that you have a satellite it’s flying around looking down trying to measure things. To make sure that you get that satellite measurement right it’s really helpful to have an instrument on the ground that looks up. It’s a similar type of instrument but it’s on the ground so there are all kinds of extra things you can do to work out what you’re seeing when you have something that’s ground based.
So New Zealand has one of the two initial ground-based instruments like this, they are called TCCON (Total Column Carbon Observing Network) instruments. They support all types of satellite activities and will be supporting MethaneSat as well. And then the third big thing is the modelling. We have already a well-developed modelling framework that’s operating at a very high resolution, where we’ll be able to be right in there with that modelling to be able to turn those concentrations that we’re seeing in the satellite into the emissions we need to take policy action.
The next question is for Peter.
What will New Zealand get out of being part of this mission?
Dr. Peter Crabtree: Quite a lot! There is a number of elements.
One element is that the mission control for this programme is going to be based in New Zealand, so we get to participate in the programme from an engineering perspective, setting up the mission control functions and all the protocols around the mission control itself. From a space capability perspective, that’s a really good opportunity for us to step into the idea of hosting a world class space mission. So, very much for the space systems people, very excited about it from that perspective.
Then on the other side of things is the science. It’s really around the fact that we get to stand alongside some international partners like Harvard University and the Smithsonian and work with them on the science programme. New Zealand is going to lead the agricultural emissions side of that, and with the United States in particular focused on oil and gas emissions, with methane emissions as well. We love the idea of international science partnerships that are operating at that level, they really help us get more impact out of our science programmes.
So those are two elements, and really, the third bit, is from a policy perspective is New Zealand being able to make better informed decisions when we come to think around our own climate policy and so on.
Sara what are your plans for working with the Harvard team working on oil and gas industry methane?
Dr Sara Mikaloff-Fletcher: Another thing about MethaneSAT that we haven’t talked about is that it was purpose designed to be able to tackle anthropogenic emissions, mostly from oil and gas. That’s because these are really the low hanging fruit of climate action. If you tell people where a leak is, because it’s usually an accidental leak, then you have a really good chance that those people are going to be excited to go fix that leak and reduce our methane. But there is tremendous opportunity to be able to use the same data that are designed to be able to detect these oil and gas leaks for agricultural problems.
So we also have agricultural emissions of methane from sheep, cows, rice patties, those types of things, and the aim of the New Zealand-based science project is to develop the capability to use these data to detect those agricultural emissions not only giving New Zealand some of the best information anywhere in the world about our agricultural emissions but also helping to design a framework for how the international team can pick other places they might want to look at and target to support climate action there.
Peter the theme of world space week this year is “satellites improve life” what other satellite activities is the New Zealand space agency involved in?
Dr. Peter Crabtree: New Zealand is a pretty young space actor. We have a space sector now which is about $1.7 billion dollars worth of activity, but we are still quite young. In terms of satellite development, a lot of our effort is going largely into educational institutions probably smaller scale satellite programmes, cubesat opportunities. Which start to, on the one hand demonstrate what you can do with small satellites, as a capability, and the things you can do with small satellites every day, like miniaturisation across all technology is that is ever expanding. We are also really interested from a government perspective as what are the government’s needs that can be better addressed through satellites.
So really, at the moment, we are spending a lot of time across government working with lots of agencies that have an interest and have had for a long time often used Earth observation, but is really about the New Zealand government being a super user of satellites. I think, over time, that will lead us to getting clearer about which area we want to invest in, in particular when it comes to the satellite capabilities. We are on a journey at the moment.
And would you like to see New Zealand making greater use of satellite data?
Absolutely! It’s quite a challenge for a lot of people who have not been exposed to the possibilities of this, and there are a lot of things we do that at the moment, we might be on Earth, and might measure in certain ways, and it’s often quite labour-intensive and resource-intensive but also the issue around frontier technologies like this is that they push the boundaries of what might be possible.
So what if, from space, you could, every day you could track, or every week, we could track if we were winning the battle against possums in our conservationist state? Suddenly on your desktop you would have AI, robots essentially, being able to tell you that those species are thriving or not thriving. And so we are interested, we are seeing those kinds of possibilities all over the place and it’s a question of getting the customer or the potential users to understand that is a real possibility, and on the other hand that we fast track our technology development so that we can actually give people these types of solutions, is really really exciting times.
Haritina Mogosanu: This is what World Space Week is all about, bringing space technology here to people on Earth, so we are on a very good path.
Thank you very much Peter and Sara for your time and for coming here and Happy World Space Week!
On the 18th of March 2021, the community gathered at KaPai soup round 4, voted Cosmic Star Safari to be the winner of the $1070 prize in cash.
Thank you to everyone for their stellar generosity and for voting for us. Special thanks to Kapai Soup for inviting us to join the bidding team.
At the end of the programme, we would like to invite everyone who was at the Kapai Soup Carterton on the 18th of March to attend the wrap-up of the Cosmic Star Safari at Stonehenge Aotearoa.
The event will be free for the attendees of Kapai Soup on the 18th of March 2021.
What is a Cosmic Star Safari?
Cosmic Star Safari is a one year space and astronomy programme for a lucky school.
Here are the space and astronomy-related projects and milestones that are part of it:
Milestone 1. Our portable planetarium visits the school.
Milestone 2. The school visits Stonehenge Aotearoa.
Throughout the year, 30 students get to access robotic telescopes in Chile and the Canary Islands.
Milestone 3. After one year, the school creates a temporary exhibition from what they learned during the online astronomy programme.
Cosmic Star Safari is provided by NZAN with support from Milky-Way.Kiwi and Stonehenge Aotearoa
What will happen now?
Schools can win a Cosmic Star Safari by doing their own pitch, telling us why they should get a Cosmic Star Safari.
Keep an eye on social media and our website to learn what you need to do. Like us on Facebook, Instagram and Twitter or subscribe to our blog to be the first to find out.
To grow for an entire month, your seeds will need water, light, an atmosphere and also food.
In the AHiS space experiments JAXA used OAT house series fertiliser as nutrient for growing sweet basil.
However, we might not find this in New Zealand. JAXA advises to use instead hydroponics fertiliser or any fertiliser for vegetables. Make sure you follow the manufacturer’s instructions on how to dilute and prepare it.

You may substitute the fertiliser with a supernatant resulted from mixing soil and water and is let to sit for a while. The soil contains various elements necessary for the plants’ growth, which dissolve into water after mixing the water and soil.
Let the solution sit a while – half a day to a day and the soil and water will be separate.
Remove the residues on top and use the aqueous solution resulted (this is the supernatant) as a fertiliser for your seeds.
If you are experimenting with soil as a medium, you do not need fertiliser. The soil contains the elements necessary for plant growth.
The OAT house series fertiliser used on the ISS contains major elements and trace amounts of metal ions necessary for plant growth and has the following chemical composition:
https://www.oat-agrio.co.jp/cgi/psearch/item/2013101716413104/index.html
In the AHiS experiment on the ISS, OAT house #1 powder and OAT house #2 powder are dissolved in water at 0.3% and 0.2%, respectively. For example, 3.0 g of OAT house #1 and 2.0 g of OAT house #2 fertilizer powder are dissolved in 1000 mL of bottled water. As a result, the following is the final concentration. This is filled in the watering syringes.
Concentrated
OAT house fertiliser
OAT house #1 | OAT house #2 |
TN (Total nitrogen) * 10.0% | TN (Total nitrogen) 11.0% |
P2O5 (phosphorus) 8.0% | Ca (calcium) 16.4% |
K2O (potassium) 27.0% | |
MgO (magnesium) 4.0% | |
MnO (manganese) 0.10% | |
B2O3 (boron) 0.10% | |
Fe (ferrum) 0.18% | |
Cu (copper) 0.002% | |
Zn (zinc) 0.006% | |
Mo (molybdenum) 0.002% |
*Total nitrogen includes ammoniacal nitrogen and nitrate nitrogen.
OAT house fertiliser’s concentration after dissolving it with water
OAT house #1 | OAT house #2 |
TN (Total nitrogen) 0.030% | TN (Total nitrogen) 0.022% |
P2O5 (phosphorus) 0.024% | Ca (calcium) 0.0328% |
K2O (potassium) 0.081% | |
MgO (magnesium) 0.012% | |
MnO (manganese) 0.0003% | |
B2O3 (boron) 0.0003% | |
Fe (ferrum) 0.00054% | |
Cu (copper) 0.000006% | |
Zn (zinc) 0.000018% | |
Mo (molybdenum) 0.000006% |
Did you know?
The fertiliser solution used on the International Space Station to grow the basil seeds comes from space. Except for hydrogen, some helium and lithium, which were formed after the Big Bang, all other chemical elements we have here on Earth have once been in a star. This means, you are made of stardust too!
The following two tables show nutritional elements (what we need to survive) and where were they formed (in which type of stars or processes)
Growing conditions
Record all information or data you have about the growing conditions of your plants, for instance you can take readings of the daily temperature, humidity and light.
The more readings you take, the better your information will be for analysing your investigation results and drawing conclusions for your research paper / poster.
Describe these conditions in detail, so we can understand what your measurements were about.
Ideally, everyone should conduct the research under the same conditions but it is difficult to maintain the same temperature, humidity or lighting levels across all the schools in New Zealand. To be able to make a comparison between all the seeds grown in schools, it is a very good idea to write down as much as you can about your particular conditions.
All collected data should be recorded regularly in a personally designed data logbook or using a data sheet.

Basic characteristics
The following are basic characteristics that you may choose to observe, measure, and record for your seeds
- Germination rate: Record the number of seeds that sprout and the date that each sprout appeared. Monitor how many of the seeds sprout within the first two weeks.
- Plant height: Measure and record this measurement daily.
- The number of leaves: Count and record daily.
- Observation of glandular hair cells on the leaves: Behind the leaves of basil plants are glandular hair cells that secrete essential oils. Let’s observe the shape of the cell. You will have to use a microscope or magnifying glass for this experiment, to observe glandular hairs.
- Aroma: describe the scent of the leaves.
#きょうのバジル 24日目。きょうはうえからもかんさつしたよ。はっぱが太陽電池パネルみたいにおおきく広がってるのがわかるね! #Spacebasil Day24 Leaves are just like #SolarArray of #ISS! pic.twitter.com/2s005Pbm5r
— NOGUCHI, Soichi 野口 聡一(のぐち そういち) (@Astro_Soichi) March 12, 2021
Comparison between the ISS and the ground data
The Japanese Space Agency (JAXA) AHiS Project team is looking for the following data:
- Observations on the growth of your lot of sweet basil plants. Think about why plants grew well and why they didn’t.
- Observations on the difference between the microgravity on the ISS and Earth’s gravity – 1G, by comparing your experiments with the one on the ISS.
The New Zealand Astrobiology Network will evaluate the participants’ reports from a scientific perspective.
You will compare growth such as stem length, leaf size, leaf color and number of leaves. At the end of the 30 days, we will also look at the glandular hair cells on the back of leaves, and count them.
Let’s find out how these are different from the sweet basil grown on the ISS.
What is the difference between under the ISS environment and your experiment conditions? These differences may significantly affect the results of growth experiment.
- Temperature
- Humidity
- Light
- Fertilizer
- Growth medium
- CO2 concentration
- Plant chamber (ventilation efficiency, water supply volume, plant density)
- Presence or absence of gravity
↓
What will change when you change these?
Furthermore, you can try different conditions on the ground to find the more suitable conditions for the growth of sweet basil, such as changing the plant box, fertiliser’s concentration, and the number of seeds sown in the plant box.
Submit your results and you will go in the draw to win a prize.
You can either write a report or produce an electronic poster of your experiment.
Here is what we require from you:
What to write in your report / poster
The structure of a general experiment report is as follows:
- Experimenter’s name(s) (Your name)
- Date started and the duration of the experiment
- Objective: What does the experiment observe?
- Experimental method: How did you make the plant box / what type of plant box did you use, what was the growing environment, what kind of work and how did you do it?
- Results: What kind of results did you get? (Please use “Plant growth records, photographs, Graph, Table, etc.” to make it easy to understand.)
- Discussion: What did you think of the obtained experimental results? (For example, what is the cause of the difference in growth between the ISS and the ground?)
Submit your results and win
How to grow your basil
Warmth
Sweet basil grows well in a warm environment, with the optimum temperature being 22 to 30 degrees Celsius and it does not like cold climates.
Plenty of light
Sweet basil also likes light in order to grow well. If it is too dark, sweet basil will not grow healthy.
When growing it indoors, keep it as close as possible to the fluorescent lights in the room or place the container closer to a desk light.
CO2
The CO2 concentration inside the ISS is higher than on the ground. However, it may be difficult for you to produce the same CO2 concentration like the one on the ISS so JAXA does not recommend anything about maintaining the same the CO2 levels.
Basil is a very popular plant and even though is mostly associated with Mediterranean cuisine, it is likely originated from India. Sweet basil is an annual herb of the mint family (Lamiaceae). Other famous plants in the same family are lavender and rosemary, thyme and even the famous catnip. (Encyclopaedia Britannica, 2021).

Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
Professor Carol Oliver
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales Carol Oliver is an Associate Professor with...
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
In 1963, Valentina Tereshkova became the first woman in space when she launched aboard the Soviet space program’s Vostok 6. To this day, she remains the only woman to have completed a solo space mission. The Vostok 6 mission lasted three days and orbited the Earth a total of 48 times.
Tereshkova was born in 1937 in the village of Bolshoye Maslennikovo in central Russia. Her father was killed in the Finnish Winter War, part of World War II, when she was two years old. She attended school up until age 17, after which she began working in the tyre and textile mill industries whilst completing correspondence courses at the Light Industry Technical School to continue her education. Outside of her work and studies, Tereshkova developed an interest in skydiving and completed her first jump when she was 22. It was her experience in skydiving that would lead to her selection as a cosmonaut.
The head of the Soviet cosmonaut training program, Nikolai Kamanin, decided as a part of the Space Race that the U.S.A. could not be the first to put a woman in space and begun the recruitment process for female cosmonauts. Criteria to be a female cosmonaut included being younger than 30, no taller than 170 centimetres, and having experience with parachuting. In 1962, five candidates were chosen to enter the cosmonaut training process including Valentina Tereshkova, Zhanna Yorkina, Irina Solovyeva, Valentina Ponomaryova, and Tatyana Kuznetsova. In May 1963, Valentina Tereshkova was selected to fly Vostok 6.
The Vostok 6 spacecraft was operated predominantly from the ground by the Soviet space program. During the mission, data was collected to help study the effects of spaceflight, such as the zero-gravity environment, on the female body. Photography carried out by Tereshkova during the mission was later used to study the atmosphere.
In the same year as the Vostok 6 mission, Tereshkova married the Soviet cosmonaut Andrian Nikolayev, and went on to have a daughter named Elena Andrianovna Nikolaeva-Tereshkova. Being the first child born to both a mother and father who had been exposed to space, Elena received a lot of medical interest. Following the Vostok 6 mission, Valentina Tereshkova went on to attain the rank of major general in the Air Force and to hold several political offices as a part of the Communist Party of the Soviet Union.
The New Zealand Astrobiology Network is the Country Coordinator for the World Space Week. Find out more from our page here. This year, the theme of the World Space Week is Women in Space.
Everyone can participate in the World Space Week, which is an international celebration of the advancements created by space activities.
To start the year, we interviewed Maruška Strah, Executive Director of the World Space Week who gives an overview of what World Space Week is about.
Learn about New Zealand's first official space mission as a country, MethaneSAT.
New Zealand will contribute with an Atmospheric science programme, funded from Catalyst: Strategic over 4 years and a Mission Operations Control Centre, funded from the Strategic Science Investment Fund.
In 2020, World Space Week’s theme was “Satellites Improve Life” and the New Zealand Astrobiology Network took this opportunity to interview Dr Peter Crabtree, Head of the NZ Space Agency, Dr Sara Mikaloff-Fletcher, NZ Lead Researcher for MethaneSAT and Dr. Steven Hamburg, Chief Scientist, EDF, as New Zealand joined its first official space mission to combat climate change. The interview was conducted by Haritina Mogoșanu, Executive Director of the New Zealand Astrobiology Network and held at Space Place at Carter Observatory in Wellington, during World Space Week 2020.
by it’s chemical formula CH4, methane is a powerful greenhouse gas, that contributes to global warming, as it traps heat 28 times more effectively than carbon dioxide over a 100-year timescale.
Methane is produced under conditions where little to no oxygen is available. About 30% of methane emissions are produced by wetlands, including ponds, lakes, and rivers. Another 20% is produced by agriculture, due to a combination of livestock, waste management and rice cultivation. Activities related to oil, gas, and coal extraction release an additional 30%.
Concentrations of methane have increased by more than 150% since industrial activities and intensive agriculture began. After carbon dioxide, methane was responsible for about 23% of climate change in the 20th century.
data compiled from MBIE’s MethaneSAT mission and NASA’s Video: Methane Sources
Transcript of the interview:
Haritina Mogoșanu: The World Space Week Association is the global coordinator For the World Space Week Under the guidance of the United Nations’ Committee on the Peaceful Uses of Outer Space COPUOUS and the United Nations office for Outer Space Affairs.
Every year, the World Space Week Association Board chooses a theme. In 2020, the theme was “Satellites Improve Life”. New Zealand has joined its first official space mission as a country to combat climate change. It’s called MethaneSAT, and the mission’s Control Centre will be located here in New Zealand. I’m here with Dr Peter Crabtree, the head of the New Zealand Space Agency and Dr Sara Mikaloff-Fletcher, Lead Researcher for the mission.
Kia Ora Peter and Sara, it is a real pleasure to have you here.
Kia Ora
Peter, what is MethaneSAT?
Dr. Peter Crabtree: MethaneSAT is a mission with the objective of sensing atmospheric methane concentrations. And so with the idea that we gain better information, about those concentrations, and that will enable people to make better decisions and to understand the phenomenon much better.
Why has New Zealand chosen a partnership with the Environmental Defence Fund in the US for our first official space mission?
Thank you, that’s a good question. There are two answers to that on the one hand we were thinking, prior to this, about doing something in the climate science area and that being a really good objective for New Zealand given our interest as a nation from a policy perspective and so on, and then, on the other hand, there was an opportunity that came towards us to participate and be a partner in a really cutting edge space mission that also was going to happen with what we thought was a reasonable time frame given the pace that we were moving at, which was quite quick. So the idea of working with an organisation that was going to be quite nimble in putting together a space mission, when sometimes some space missions can be put together over very long period of time, and we saw this as a real opportunity for New Zealand to step into something that was really quite a serious endeavour but something that could really assist us as a nation in quite a number of different ways.
Let’s cross over to Steven Hamburg from EDF, Steven could you please tell us a little bit more
Dr. Steven Hamburg: Hello Hari, Peter and Sara it’s great to be with you and it’s great to have an opportunity to talk about MethaneSAT a mission that I’m passionate about.
The idea of MethaneSAT started a few years ago in conversation between Steve Wofsy, a professor at Harvard University and myself about the need to be able to collect methane flux data, how much methane was being emitted from around the world, and we didn’t have that capacity and without that knowledge we really couldn’t take advantage of the opportunity to reduce methane emissions because we did not know where it was occurring.
So we determined what we would need from a satellite and then went to the technology experts and asked, could we push the envelope on the technology to build the capacity inflight in space. And while we were pushing the envelope, that technology has evolved and is now possible, and MethaneSAT is the product of that integration of new technology, innovative science and the inversion technology that Steve has pioneered, into a program that allows us to do the advocacy to bring that data to the rest of the world.
And EDF, the Environmental Defence Fund, is well situated to lead this effort. EDF was founded by a group of scientists who understood a problem but did not have the tools to implement the understanding into policy that resulted from that knowledge. And that initial problem was the impacts of DDT on birds of prey in eastern United States. So they got together and formed the Environmental Defence Fund, hired a lawyer and then, using their science, went to look at and implement the needed ban on DDT, which was implemented in the early 1970s.
So with methane emissions from oil and gas industry, we understand the impact it’s having on the climate but we didn’t have the tools to bring that data and understanding to the many oil and gas producing regions of the world so that we could reduce those emissions and greatly slow the rate of warming.
MethaneSAT is very different than many other missions in that as I mentioned we started with the problem, and then went to look at the solutions. Could the technologies provide the data necessary to address that problem? We build an amazing team led by Tom Ingersoll who comes out of the commercial space community, of people who are really committed to ensuring that you we can use space technology to help society address one of the biggest crisis we ever faced which is climate change. And so by getting the best of the space technology community together with the best of the scientific community, in partnership with New Zealand, which has been an incredible opportunity to really push this mission forward fast and implement it effectively, we are very much looking forward to the operation centre being in New Zealand and to getting the satellite launched and the data flowing so that we can start to figure out where those methane emissions are coming from and ensure that people understand how those emissions can be mitigated and in turn getting that job done.
New Zealand is a wonderful partner in that there is a real commitment to bringing good science to bear on the needs of society writ large and that is the mission of EDF and so we are really very pleased to have the partnership with the New Zealand Government and the science community.
We are partnering with New Zealand because it’s a real natural fit. The focus of the Ministry for Business, Innovation and Employment on the use of science to help improve New Zealand society and the well-being of your citizens fits wonderfully into the objectives of this mission and to the DNA of EDF as an organisation for these fifty plus years. So by taking advantage of the scientific knowledge that already exists in New Zealand and to help develop the nascent space capacity in the country we were able to accelerate progress on the mission while developing the skill sets in New Zealand. It’s a partnership that we very much value, and are confident will persist and enhance the work we are doing together over the coming years.
Thank you Steven.
I have a couple of questions for Sara
What is novel about the satellite mission?
Dr Sara Mikaloff-Fletcher: So many things.
It’s an amazing mission! I mean for me, on the technical side, there are two big things. One is that it’s the first time we’re going to have a satellite flying in the sky that’s going to be able to measure methane with the kind of precision we would expect to have of someone on my team tried to measure it with an instrument on the ground. That’s extraordinary! The other thing is the spatial resolution so this thing is going to capture a 200 x 200 km scene and within that scene is going to do a raster scan with very high precision so we will be able to pick up exactly where these emissions are happening; but then on the policy side, it’s the first satellite that’s been purposely designed to support and enable climate action.
So there are two big things happening there, one is that they are going to have inverse modelling as part of the whole framework, which is the modelling tool you used to go from what the satellite measures, which is the concentration, to what you need for policy action which is to know the emissions. So that’s going to be happening live throughout the satellite’s mission, and then in addition to that is the impact in communicating as quickly so that we can empower people to be able to reduce these emissions.
Tell me Sara,
What relevant expertise do we have here in New Zealand to contribute to MethaneSAT science?
Well we have quite a big going on in New Zealand. New Zealand has been a leader in greenhouse gas measurements, since before I was born. In fact, when I was a PhD student coming up at NOAA, which is kind of our opposite number in the US, NIWA was already famous to me for having the best methane isotopes almost anywhere in the world. And so we have this amazing rich history of these atmospheric measurements both on the ground and also in the total air column. So you can imagine that you have a satellite it’s flying around looking down trying to measure things. To make sure that you get that satellite measurement right it’s really helpful to have an instrument on the ground that looks up. It’s a similar type of instrument but it’s on the ground so there are all kinds of extra things you can do to work out what you’re seeing when you have something that’s ground based.
So New Zealand has one of the two initial ground-based instruments like this, they are called TCCON (Total Column Carbon Observing Network) instruments. They support all types of satellite activities and will be supporting MethaneSat as well. And then the third big thing is the modelling. We have already a well-developed modelling framework that’s operating at a very high resolution, where we’ll be able to be right in there with that modelling to be able to turn those concentrations that we’re seeing in the satellite into the emissions we need to take policy action.
The next question is for Peter.
What will New Zealand get out of being part of this mission?
Dr. Peter Crabtree: Quite a lot! There is a number of elements.
One element is that the mission control for this programme is going to be based in New Zealand, so we get to participate in the programme from an engineering perspective, setting up the mission control functions and all the protocols around the mission control itself. From a space capability perspective, that’s a really good opportunity for us to step into the idea of hosting a world class space mission. So, very much for the space systems people, very excited about it from that perspective.
Then on the other side of things is the science. It’s really around the fact that we get to stand alongside some international partners like Harvard University and the Smithsonian and work with them on the science programme. New Zealand is going to lead the agricultural emissions side of that, and with the United States in particular focused on oil and gas emissions, with methane emissions as well. We love the idea of international science partnerships that are operating at that level, they really help us get more impact out of our science programmes.
So those are two elements, and really, the third bit, is from a policy perspective is New Zealand being able to make better informed decisions when we come to think around our own climate policy and so on.
Sara what are your plans for working with the Harvard team working on oil and gas industry methane?
Dr Sara Mikaloff-Fletcher: Another thing about MethaneSAT that we haven’t talked about is that it was purpose designed to be able to tackle anthropogenic emissions, mostly from oil and gas. That’s because these are really the low hanging fruit of climate action. If you tell people where a leak is, because it’s usually an accidental leak, then you have a really good chance that those people are going to be excited to go fix that leak and reduce our methane. But there is tremendous opportunity to be able to use the same data that are designed to be able to detect these oil and gas leaks for agricultural problems.
So we also have agricultural emissions of methane from sheep, cows, rice patties, those types of things, and the aim of the New Zealand-based science project is to develop the capability to use these data to detect those agricultural emissions not only giving New Zealand some of the best information anywhere in the world about our agricultural emissions but also helping to design a framework for how the international team can pick other places they might want to look at and target to support climate action there.
Peter the theme of world space week this year is “satellites improve life” what other satellite activities is the New Zealand space agency involved in?
Dr. Peter Crabtree: New Zealand is a pretty young space actor. We have a space sector now which is about $1.7 billion dollars worth of activity, but we are still quite young. In terms of satellite development, a lot of our effort is going largely into educational institutions probably smaller scale satellite programmes, cubesat opportunities. Which start to, on the one hand demonstrate what you can do with small satellites, as a capability, and the things you can do with small satellites every day, like miniaturisation across all technology is that is ever expanding. We are also really interested from a government perspective as what are the government’s needs that can be better addressed through satellites.
So really, at the moment, we are spending a lot of time across government working with lots of agencies that have an interest and have had for a long time often used Earth observation, but is really about the New Zealand government being a super user of satellites. I think, over time, that will lead us to getting clearer about which area we want to invest in, in particular when it comes to the satellite capabilities. We are on a journey at the moment.
And would you like to see New Zealand making greater use of satellite data?
Absolutely! It’s quite a challenge for a lot of people who have not been exposed to the possibilities of this, and there are a lot of things we do that at the moment, we might be on Earth, and might measure in certain ways, and it’s often quite labour-intensive and resource-intensive but also the issue around frontier technologies like this is that they push the boundaries of what might be possible.
So what if, from space, you could, every day you could track, or every week, we could track if we were winning the battle against possums in our conservationist state? Suddenly on your desktop you would have AI, robots essentially, being able to tell you that those species are thriving or not thriving. And so we are interested, we are seeing those kinds of possibilities all over the place and it’s a question of getting the customer or the potential users to understand that is a real possibility, and on the other hand that we fast track our technology development so that we can actually give people these types of solutions, is really really exciting times.
Haritina Mogosanu: This is what World Space Week is all about, bringing space technology here to people on Earth, so we are on a very good path.
Thank you very much Peter and Sara for your time and for coming here and Happy World Space Week!
On the 18th of March 2021, the community gathered at KaPai soup round 4, voted Cosmic Star Safari to be the winner of the $1070 prize in cash.
Thank you to everyone for their stellar generosity and for voting for us. Special thanks to Kapai Soup for inviting us to join the bidding team.
At the end of the programme, we would like to invite everyone who was at the Kapai Soup Carterton on the 18th of March to attend the wrap-up of the Cosmic Star Safari at Stonehenge Aotearoa.
The event will be free for the attendees of Kapai Soup on the 18th of March 2021.
What is a Cosmic Star Safari?
Cosmic Star Safari is a one year space and astronomy programme for a lucky school.
Here are the space and astronomy-related projects and milestones that are part of it:
Milestone 1. Our portable planetarium visits the school.
Milestone 2. The school visits Stonehenge Aotearoa.
Throughout the year, 30 students get to access robotic telescopes in Chile and the Canary Islands.
Milestone 3. After one year, the school creates a temporary exhibition from what they learned during the online astronomy programme.
Cosmic Star Safari is provided by NZAN with support from Milky-Way.Kiwi and Stonehenge Aotearoa
What will happen now?
Schools can win a Cosmic Star Safari by doing their own pitch, telling us why they should get a Cosmic Star Safari.
Keep an eye on social media and our website to learn what you need to do. Like us on Facebook, Instagram and Twitter or subscribe to our blog to be the first to find out.
To grow for an entire month, your seeds will need water, light, an atmosphere and also food.
In the AHiS space experiments JAXA used OAT house series fertiliser as nutrient for growing sweet basil.
However, we might not find this in New Zealand. JAXA advises to use instead hydroponics fertiliser or any fertiliser for vegetables. Make sure you follow the manufacturer’s instructions on how to dilute and prepare it.

You may substitute the fertiliser with a supernatant resulted from mixing soil and water and is let to sit for a while. The soil contains various elements necessary for the plants’ growth, which dissolve into water after mixing the water and soil.
Let the solution sit a while – half a day to a day and the soil and water will be separate.
Remove the residues on top and use the aqueous solution resulted (this is the supernatant) as a fertiliser for your seeds.
If you are experimenting with soil as a medium, you do not need fertiliser. The soil contains the elements necessary for plant growth.
The OAT house series fertiliser used on the ISS contains major elements and trace amounts of metal ions necessary for plant growth and has the following chemical composition:
https://www.oat-agrio.co.jp/cgi/psearch/item/2013101716413104/index.html
In the AHiS experiment on the ISS, OAT house #1 powder and OAT house #2 powder are dissolved in water at 0.3% and 0.2%, respectively. For example, 3.0 g of OAT house #1 and 2.0 g of OAT house #2 fertilizer powder are dissolved in 1000 mL of bottled water. As a result, the following is the final concentration. This is filled in the watering syringes.
Concentrated
OAT house fertiliser
OAT house #1 | OAT house #2 |
TN (Total nitrogen) * 10.0% | TN (Total nitrogen) 11.0% |
P2O5 (phosphorus) 8.0% | Ca (calcium) 16.4% |
K2O (potassium) 27.0% | |
MgO (magnesium) 4.0% | |
MnO (manganese) 0.10% | |
B2O3 (boron) 0.10% | |
Fe (ferrum) 0.18% | |
Cu (copper) 0.002% | |
Zn (zinc) 0.006% | |
Mo (molybdenum) 0.002% |
*Total nitrogen includes ammoniacal nitrogen and nitrate nitrogen.
OAT house fertiliser’s concentration after dissolving it with water
OAT house #1 | OAT house #2 |
TN (Total nitrogen) 0.030% | TN (Total nitrogen) 0.022% |
P2O5 (phosphorus) 0.024% | Ca (calcium) 0.0328% |
K2O (potassium) 0.081% | |
MgO (magnesium) 0.012% | |
MnO (manganese) 0.0003% | |
B2O3 (boron) 0.0003% | |
Fe (ferrum) 0.00054% | |
Cu (copper) 0.000006% | |
Zn (zinc) 0.000018% | |
Mo (molybdenum) 0.000006% |
Did you know?
The fertiliser solution used on the International Space Station to grow the basil seeds comes from space. Except for hydrogen, some helium and lithium, which were formed after the Big Bang, all other chemical elements we have here on Earth have once been in a star. This means, you are made of stardust too!
The following two tables show nutritional elements (what we need to survive) and where were they formed (in which type of stars or processes)
Growing conditions
Record all information or data you have about the growing conditions of your plants, for instance you can take readings of the daily temperature, humidity and light.
The more readings you take, the better your information will be for analysing your investigation results and drawing conclusions for your research paper / poster.
Describe these conditions in detail, so we can understand what your measurements were about.
Ideally, everyone should conduct the research under the same conditions but it is difficult to maintain the same temperature, humidity or lighting levels across all the schools in New Zealand. To be able to make a comparison between all the seeds grown in schools, it is a very good idea to write down as much as you can about your particular conditions.
All collected data should be recorded regularly in a personally designed data logbook or using a data sheet.

Basic characteristics
The following are basic characteristics that you may choose to observe, measure, and record for your seeds
- Germination rate: Record the number of seeds that sprout and the date that each sprout appeared. Monitor how many of the seeds sprout within the first two weeks.
- Plant height: Measure and record this measurement daily.
- The number of leaves: Count and record daily.
- Observation of glandular hair cells on the leaves: Behind the leaves of basil plants are glandular hair cells that secrete essential oils. Let’s observe the shape of the cell. You will have to use a microscope or magnifying glass for this experiment, to observe glandular hairs.
- Aroma: describe the scent of the leaves.
#きょうのバジル 24日目。きょうはうえからもかんさつしたよ。はっぱが太陽電池パネルみたいにおおきく広がってるのがわかるね! #Spacebasil Day24 Leaves are just like #SolarArray of #ISS! pic.twitter.com/2s005Pbm5r
— NOGUCHI, Soichi 野口 聡一(のぐち そういち) (@Astro_Soichi) March 12, 2021
Comparison between the ISS and the ground data
The Japanese Space Agency (JAXA) AHiS Project team is looking for the following data:
- Observations on the growth of your lot of sweet basil plants. Think about why plants grew well and why they didn’t.
- Observations on the difference between the microgravity on the ISS and Earth’s gravity – 1G, by comparing your experiments with the one on the ISS.
The New Zealand Astrobiology Network will evaluate the participants’ reports from a scientific perspective.
You will compare growth such as stem length, leaf size, leaf color and number of leaves. At the end of the 30 days, we will also look at the glandular hair cells on the back of leaves, and count them.
Let’s find out how these are different from the sweet basil grown on the ISS.
What is the difference between under the ISS environment and your experiment conditions? These differences may significantly affect the results of growth experiment.
- Temperature
- Humidity
- Light
- Fertilizer
- Growth medium
- CO2 concentration
- Plant chamber (ventilation efficiency, water supply volume, plant density)
- Presence or absence of gravity
↓
What will change when you change these?
Furthermore, you can try different conditions on the ground to find the more suitable conditions for the growth of sweet basil, such as changing the plant box, fertiliser’s concentration, and the number of seeds sown in the plant box.
Submit your results and you will go in the draw to win a prize.
You can either write a report or produce an electronic poster of your experiment.
Here is what we require from you:
What to write in your report / poster
The structure of a general experiment report is as follows:
- Experimenter’s name(s) (Your name)
- Date started and the duration of the experiment
- Objective: What does the experiment observe?
- Experimental method: How did you make the plant box / what type of plant box did you use, what was the growing environment, what kind of work and how did you do it?
- Results: What kind of results did you get? (Please use “Plant growth records, photographs, Graph, Table, etc.” to make it easy to understand.)
- Discussion: What did you think of the obtained experimental results? (For example, what is the cause of the difference in growth between the ISS and the ground?)
Submit your results and win
How to grow your basil
Warmth
Sweet basil grows well in a warm environment, with the optimum temperature being 22 to 30 degrees Celsius and it does not like cold climates.
Plenty of light
Sweet basil also likes light in order to grow well. If it is too dark, sweet basil will not grow healthy.
When growing it indoors, keep it as close as possible to the fluorescent lights in the room or place the container closer to a desk light.
CO2
The CO2 concentration inside the ISS is higher than on the ground. However, it may be difficult for you to produce the same CO2 concentration like the one on the ISS so JAXA does not recommend anything about maintaining the same the CO2 levels.
Basil is a very popular plant and even though is mostly associated with Mediterranean cuisine, it is likely originated from India. Sweet basil is an annual herb of the mint family (Lamiaceae). Other famous plants in the same family are lavender and rosemary, thyme and even the famous catnip. (Encyclopaedia Britannica, 2021).
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
In 1963, Valentina Tereshkova became the first woman in space when she launched aboard the Soviet space program’s Vostok 6. To this day, she remains the only woman to have completed a solo space mission. The Vostok 6 mission lasted three days and orbited the Earth a total of 48 times.
Tereshkova was born in 1937 in the village of Bolshoye Maslennikovo in central Russia. Her father was killed in the Finnish Winter War, part of World War II, when she was two years old. She attended school up until age 17, after which she began working in the tyre and textile mill industries whilst completing correspondence courses at the Light Industry Technical School to continue her education. Outside of her work and studies, Tereshkova developed an interest in skydiving and completed her first jump when she was 22. It was her experience in skydiving that would lead to her selection as a cosmonaut.
The head of the Soviet cosmonaut training program, Nikolai Kamanin, decided as a part of the Space Race that the U.S.A. could not be the first to put a woman in space and begun the recruitment process for female cosmonauts. Criteria to be a female cosmonaut included being younger than 30, no taller than 170 centimetres, and having experience with parachuting. In 1962, five candidates were chosen to enter the cosmonaut training process including Valentina Tereshkova, Zhanna Yorkina, Irina Solovyeva, Valentina Ponomaryova, and Tatyana Kuznetsova. In May 1963, Valentina Tereshkova was selected to fly Vostok 6.
The Vostok 6 spacecraft was operated predominantly from the ground by the Soviet space program. During the mission, data was collected to help study the effects of spaceflight, such as the zero-gravity environment, on the female body. Photography carried out by Tereshkova during the mission was later used to study the atmosphere.
In the same year as the Vostok 6 mission, Tereshkova married the Soviet cosmonaut Andrian Nikolayev, and went on to have a daughter named Elena Andrianovna Nikolaeva-Tereshkova. Being the first child born to both a mother and father who had been exposed to space, Elena received a lot of medical interest. Following the Vostok 6 mission, Valentina Tereshkova went on to attain the rank of major general in the Air Force and to hold several political offices as a part of the Communist Party of the Soviet Union.
The New Zealand Astrobiology Network is the Country Coordinator for the World Space Week. Find out more from our page here. This year, the theme of the World Space Week is Women in Space.
Everyone can participate in the World Space Week, which is an international celebration of the advancements created by space activities.
To start the year, we interviewed Maruška Strah, Executive Director of the World Space Week who gives an overview of what World Space Week is about.
Learn about New Zealand's first official space mission as a country, MethaneSAT.
New Zealand will contribute with an Atmospheric science programme, funded from Catalyst: Strategic over 4 years and a Mission Operations Control Centre, funded from the Strategic Science Investment Fund.
In 2020, World Space Week’s theme was “Satellites Improve Life” and the New Zealand Astrobiology Network took this opportunity to interview Dr Peter Crabtree, Head of the NZ Space Agency, Dr Sara Mikaloff-Fletcher, NZ Lead Researcher for MethaneSAT and Dr. Steven Hamburg, Chief Scientist, EDF, as New Zealand joined its first official space mission to combat climate change. The interview was conducted by Haritina Mogoșanu, Executive Director of the New Zealand Astrobiology Network and held at Space Place at Carter Observatory in Wellington, during World Space Week 2020.
by it’s chemical formula CH4, methane is a powerful greenhouse gas, that contributes to global warming, as it traps heat 28 times more effectively than carbon dioxide over a 100-year timescale.
Methane is produced under conditions where little to no oxygen is available. About 30% of methane emissions are produced by wetlands, including ponds, lakes, and rivers. Another 20% is produced by agriculture, due to a combination of livestock, waste management and rice cultivation. Activities related to oil, gas, and coal extraction release an additional 30%.
Concentrations of methane have increased by more than 150% since industrial activities and intensive agriculture began. After carbon dioxide, methane was responsible for about 23% of climate change in the 20th century.
data compiled from MBIE’s MethaneSAT mission and NASA’s Video: Methane Sources
Transcript of the interview:
Haritina Mogoșanu: The World Space Week Association is the global coordinator For the World Space Week Under the guidance of the United Nations’ Committee on the Peaceful Uses of Outer Space COPUOUS and the United Nations office for Outer Space Affairs.
Every year, the World Space Week Association Board chooses a theme. In 2020, the theme was “Satellites Improve Life”. New Zealand has joined its first official space mission as a country to combat climate change. It’s called MethaneSAT, and the mission’s Control Centre will be located here in New Zealand. I’m here with Dr Peter Crabtree, the head of the New Zealand Space Agency and Dr Sara Mikaloff-Fletcher, Lead Researcher for the mission.
Kia Ora Peter and Sara, it is a real pleasure to have you here.
Kia Ora
Peter, what is MethaneSAT?
Dr. Peter Crabtree: MethaneSAT is a mission with the objective of sensing atmospheric methane concentrations. And so with the idea that we gain better information, about those concentrations, and that will enable people to make better decisions and to understand the phenomenon much better.
Why has New Zealand chosen a partnership with the Environmental Defence Fund in the US for our first official space mission?
Thank you, that’s a good question. There are two answers to that on the one hand we were thinking, prior to this, about doing something in the climate science area and that being a really good objective for New Zealand given our interest as a nation from a policy perspective and so on, and then, on the other hand, there was an opportunity that came towards us to participate and be a partner in a really cutting edge space mission that also was going to happen with what we thought was a reasonable time frame given the pace that we were moving at, which was quite quick. So the idea of working with an organisation that was going to be quite nimble in putting together a space mission, when sometimes some space missions can be put together over very long period of time, and we saw this as a real opportunity for New Zealand to step into something that was really quite a serious endeavour but something that could really assist us as a nation in quite a number of different ways.
Let’s cross over to Steven Hamburg from EDF, Steven could you please tell us a little bit more
Dr. Steven Hamburg: Hello Hari, Peter and Sara it’s great to be with you and it’s great to have an opportunity to talk about MethaneSAT a mission that I’m passionate about.
The idea of MethaneSAT started a few years ago in conversation between Steve Wofsy, a professor at Harvard University and myself about the need to be able to collect methane flux data, how much methane was being emitted from around the world, and we didn’t have that capacity and without that knowledge we really couldn’t take advantage of the opportunity to reduce methane emissions because we did not know where it was occurring.
So we determined what we would need from a satellite and then went to the technology experts and asked, could we push the envelope on the technology to build the capacity inflight in space. And while we were pushing the envelope, that technology has evolved and is now possible, and MethaneSAT is the product of that integration of new technology, innovative science and the inversion technology that Steve has pioneered, into a program that allows us to do the advocacy to bring that data to the rest of the world.
And EDF, the Environmental Defence Fund, is well situated to lead this effort. EDF was founded by a group of scientists who understood a problem but did not have the tools to implement the understanding into policy that resulted from that knowledge. And that initial problem was the impacts of DDT on birds of prey in eastern United States. So they got together and formed the Environmental Defence Fund, hired a lawyer and then, using their science, went to look at and implement the needed ban on DDT, which was implemented in the early 1970s.
So with methane emissions from oil and gas industry, we understand the impact it’s having on the climate but we didn’t have the tools to bring that data and understanding to the many oil and gas producing regions of the world so that we could reduce those emissions and greatly slow the rate of warming.
MethaneSAT is very different than many other missions in that as I mentioned we started with the problem, and then went to look at the solutions. Could the technologies provide the data necessary to address that problem? We build an amazing team led by Tom Ingersoll who comes out of the commercial space community, of people who are really committed to ensuring that you we can use space technology to help society address one of the biggest crisis we ever faced which is climate change. And so by getting the best of the space technology community together with the best of the scientific community, in partnership with New Zealand, which has been an incredible opportunity to really push this mission forward fast and implement it effectively, we are very much looking forward to the operation centre being in New Zealand and to getting the satellite launched and the data flowing so that we can start to figure out where those methane emissions are coming from and ensure that people understand how those emissions can be mitigated and in turn getting that job done.
New Zealand is a wonderful partner in that there is a real commitment to bringing good science to bear on the needs of society writ large and that is the mission of EDF and so we are really very pleased to have the partnership with the New Zealand Government and the science community.
We are partnering with New Zealand because it’s a real natural fit. The focus of the Ministry for Business, Innovation and Employment on the use of science to help improve New Zealand society and the well-being of your citizens fits wonderfully into the objectives of this mission and to the DNA of EDF as an organisation for these fifty plus years. So by taking advantage of the scientific knowledge that already exists in New Zealand and to help develop the nascent space capacity in the country we were able to accelerate progress on the mission while developing the skill sets in New Zealand. It’s a partnership that we very much value, and are confident will persist and enhance the work we are doing together over the coming years.
Thank you Steven.
I have a couple of questions for Sara
What is novel about the satellite mission?
Dr Sara Mikaloff-Fletcher: So many things.
It’s an amazing mission! I mean for me, on the technical side, there are two big things. One is that it’s the first time we’re going to have a satellite flying in the sky that’s going to be able to measure methane with the kind of precision we would expect to have of someone on my team tried to measure it with an instrument on the ground. That’s extraordinary! The other thing is the spatial resolution so this thing is going to capture a 200 x 200 km scene and within that scene is going to do a raster scan with very high precision so we will be able to pick up exactly where these emissions are happening; but then on the policy side, it’s the first satellite that’s been purposely designed to support and enable climate action.
So there are two big things happening there, one is that they are going to have inverse modelling as part of the whole framework, which is the modelling tool you used to go from what the satellite measures, which is the concentration, to what you need for policy action which is to know the emissions. So that’s going to be happening live throughout the satellite’s mission, and then in addition to that is the impact in communicating as quickly so that we can empower people to be able to reduce these emissions.
Tell me Sara,
What relevant expertise do we have here in New Zealand to contribute to MethaneSAT science?
Well we have quite a big going on in New Zealand. New Zealand has been a leader in greenhouse gas measurements, since before I was born. In fact, when I was a PhD student coming up at NOAA, which is kind of our opposite number in the US, NIWA was already famous to me for having the best methane isotopes almost anywhere in the world. And so we have this amazing rich history of these atmospheric measurements both on the ground and also in the total air column. So you can imagine that you have a satellite it’s flying around looking down trying to measure things. To make sure that you get that satellite measurement right it’s really helpful to have an instrument on the ground that looks up. It’s a similar type of instrument but it’s on the ground so there are all kinds of extra things you can do to work out what you’re seeing when you have something that’s ground based.
So New Zealand has one of the two initial ground-based instruments like this, they are called TCCON (Total Column Carbon Observing Network) instruments. They support all types of satellite activities and will be supporting MethaneSat as well. And then the third big thing is the modelling. We have already a well-developed modelling framework that’s operating at a very high resolution, where we’ll be able to be right in there with that modelling to be able to turn those concentrations that we’re seeing in the satellite into the emissions we need to take policy action.
The next question is for Peter.
What will New Zealand get out of being part of this mission?
Dr. Peter Crabtree: Quite a lot! There is a number of elements.
One element is that the mission control for this programme is going to be based in New Zealand, so we get to participate in the programme from an engineering perspective, setting up the mission control functions and all the protocols around the mission control itself. From a space capability perspective, that’s a really good opportunity for us to step into the idea of hosting a world class space mission. So, very much for the space systems people, very excited about it from that perspective.
Then on the other side of things is the science. It’s really around the fact that we get to stand alongside some international partners like Harvard University and the Smithsonian and work with them on the science programme. New Zealand is going to lead the agricultural emissions side of that, and with the United States in particular focused on oil and gas emissions, with methane emissions as well. We love the idea of international science partnerships that are operating at that level, they really help us get more impact out of our science programmes.
So those are two elements, and really, the third bit, is from a policy perspective is New Zealand being able to make better informed decisions when we come to think around our own climate policy and so on.
Sara what are your plans for working with the Harvard team working on oil and gas industry methane?
Dr Sara Mikaloff-Fletcher: Another thing about MethaneSAT that we haven’t talked about is that it was purpose designed to be able to tackle anthropogenic emissions, mostly from oil and gas. That’s because these are really the low hanging fruit of climate action. If you tell people where a leak is, because it’s usually an accidental leak, then you have a really good chance that those people are going to be excited to go fix that leak and reduce our methane. But there is tremendous opportunity to be able to use the same data that are designed to be able to detect these oil and gas leaks for agricultural problems.
So we also have agricultural emissions of methane from sheep, cows, rice patties, those types of things, and the aim of the New Zealand-based science project is to develop the capability to use these data to detect those agricultural emissions not only giving New Zealand some of the best information anywhere in the world about our agricultural emissions but also helping to design a framework for how the international team can pick other places they might want to look at and target to support climate action there.
Peter the theme of world space week this year is “satellites improve life” what other satellite activities is the New Zealand space agency involved in?
Dr. Peter Crabtree: New Zealand is a pretty young space actor. We have a space sector now which is about $1.7 billion dollars worth of activity, but we are still quite young. In terms of satellite development, a lot of our effort is going largely into educational institutions probably smaller scale satellite programmes, cubesat opportunities. Which start to, on the one hand demonstrate what you can do with small satellites, as a capability, and the things you can do with small satellites every day, like miniaturisation across all technology is that is ever expanding. We are also really interested from a government perspective as what are the government’s needs that can be better addressed through satellites.
So really, at the moment, we are spending a lot of time across government working with lots of agencies that have an interest and have had for a long time often used Earth observation, but is really about the New Zealand government being a super user of satellites. I think, over time, that will lead us to getting clearer about which area we want to invest in, in particular when it comes to the satellite capabilities. We are on a journey at the moment.
And would you like to see New Zealand making greater use of satellite data?
Absolutely! It’s quite a challenge for a lot of people who have not been exposed to the possibilities of this, and there are a lot of things we do that at the moment, we might be on Earth, and might measure in certain ways, and it’s often quite labour-intensive and resource-intensive but also the issue around frontier technologies like this is that they push the boundaries of what might be possible.
So what if, from space, you could, every day you could track, or every week, we could track if we were winning the battle against possums in our conservationist state? Suddenly on your desktop you would have AI, robots essentially, being able to tell you that those species are thriving or not thriving. And so we are interested, we are seeing those kinds of possibilities all over the place and it’s a question of getting the customer or the potential users to understand that is a real possibility, and on the other hand that we fast track our technology development so that we can actually give people these types of solutions, is really really exciting times.
Haritina Mogosanu: This is what World Space Week is all about, bringing space technology here to people on Earth, so we are on a very good path.
Thank you very much Peter and Sara for your time and for coming here and Happy World Space Week!
On the 18th of March 2021, the community gathered at KaPai soup round 4, voted Cosmic Star Safari to be the winner of the $1070 prize in cash.
Thank you to everyone for their stellar generosity and for voting for us. Special thanks to Kapai Soup for inviting us to join the bidding team.
At the end of the programme, we would like to invite everyone who was at the Kapai Soup Carterton on the 18th of March to attend the wrap-up of the Cosmic Star Safari at Stonehenge Aotearoa.
The event will be free for the attendees of Kapai Soup on the 18th of March 2021.
What is a Cosmic Star Safari?
Cosmic Star Safari is a one year space and astronomy programme for a lucky school.
Here are the space and astronomy-related projects and milestones that are part of it:
Milestone 1. Our portable planetarium visits the school.
Milestone 2. The school visits Stonehenge Aotearoa.
Throughout the year, 30 students get to access robotic telescopes in Chile and the Canary Islands.
Milestone 3. After one year, the school creates a temporary exhibition from what they learned during the online astronomy programme.
Cosmic Star Safari is provided by NZAN with support from Milky-Way.Kiwi and Stonehenge Aotearoa
What will happen now?
Schools can win a Cosmic Star Safari by doing their own pitch, telling us why they should get a Cosmic Star Safari.
Keep an eye on social media and our website to learn what you need to do. Like us on Facebook, Instagram and Twitter or subscribe to our blog to be the first to find out.
To grow for an entire month, your seeds will need water, light, an atmosphere and also food.
In the AHiS space experiments JAXA used OAT house series fertiliser as nutrient for growing sweet basil.
However, we might not find this in New Zealand. JAXA advises to use instead hydroponics fertiliser or any fertiliser for vegetables. Make sure you follow the manufacturer’s instructions on how to dilute and prepare it.

You may substitute the fertiliser with a supernatant resulted from mixing soil and water and is let to sit for a while. The soil contains various elements necessary for the plants’ growth, which dissolve into water after mixing the water and soil.
Let the solution sit a while – half a day to a day and the soil and water will be separate.
Remove the residues on top and use the aqueous solution resulted (this is the supernatant) as a fertiliser for your seeds.
If you are experimenting with soil as a medium, you do not need fertiliser. The soil contains the elements necessary for plant growth.
The OAT house series fertiliser used on the ISS contains major elements and trace amounts of metal ions necessary for plant growth and has the following chemical composition:
https://www.oat-agrio.co.jp/cgi/psearch/item/2013101716413104/index.html
In the AHiS experiment on the ISS, OAT house #1 powder and OAT house #2 powder are dissolved in water at 0.3% and 0.2%, respectively. For example, 3.0 g of OAT house #1 and 2.0 g of OAT house #2 fertilizer powder are dissolved in 1000 mL of bottled water. As a result, the following is the final concentration. This is filled in the watering syringes.
Concentrated
OAT house fertiliser
OAT house #1 | OAT house #2 |
TN (Total nitrogen) * 10.0% | TN (Total nitrogen) 11.0% |
P2O5 (phosphorus) 8.0% | Ca (calcium) 16.4% |
K2O (potassium) 27.0% | |
MgO (magnesium) 4.0% | |
MnO (manganese) 0.10% | |
B2O3 (boron) 0.10% | |
Fe (ferrum) 0.18% | |
Cu (copper) 0.002% | |
Zn (zinc) 0.006% | |
Mo (molybdenum) 0.002% |
*Total nitrogen includes ammoniacal nitrogen and nitrate nitrogen.
OAT house fertiliser’s concentration after dissolving it with water
OAT house #1 | OAT house #2 |
TN (Total nitrogen) 0.030% | TN (Total nitrogen) 0.022% |
P2O5 (phosphorus) 0.024% | Ca (calcium) 0.0328% |
K2O (potassium) 0.081% | |
MgO (magnesium) 0.012% | |
MnO (manganese) 0.0003% | |
B2O3 (boron) 0.0003% | |
Fe (ferrum) 0.00054% | |
Cu (copper) 0.000006% | |
Zn (zinc) 0.000018% | |
Mo (molybdenum) 0.000006% |
Did you know?
The fertiliser solution used on the International Space Station to grow the basil seeds comes from space. Except for hydrogen, some helium and lithium, which were formed after the Big Bang, all other chemical elements we have here on Earth have once been in a star. This means, you are made of stardust too!
The following two tables show nutritional elements (what we need to survive) and where were they formed (in which type of stars or processes)
Growing conditions
Record all information or data you have about the growing conditions of your plants, for instance you can take readings of the daily temperature, humidity and light.
The more readings you take, the better your information will be for analysing your investigation results and drawing conclusions for your research paper / poster.
Describe these conditions in detail, so we can understand what your measurements were about.
Ideally, everyone should conduct the research under the same conditions but it is difficult to maintain the same temperature, humidity or lighting levels across all the schools in New Zealand. To be able to make a comparison between all the seeds grown in schools, it is a very good idea to write down as much as you can about your particular conditions.
All collected data should be recorded regularly in a personally designed data logbook or using a data sheet.

Basic characteristics
The following are basic characteristics that you may choose to observe, measure, and record for your seeds
- Germination rate: Record the number of seeds that sprout and the date that each sprout appeared. Monitor how many of the seeds sprout within the first two weeks.
- Plant height: Measure and record this measurement daily.
- The number of leaves: Count and record daily.
- Observation of glandular hair cells on the leaves: Behind the leaves of basil plants are glandular hair cells that secrete essential oils. Let’s observe the shape of the cell. You will have to use a microscope or magnifying glass for this experiment, to observe glandular hairs.
- Aroma: describe the scent of the leaves.
#きょうのバジル 24日目。きょうはうえからもかんさつしたよ。はっぱが太陽電池パネルみたいにおおきく広がってるのがわかるね! #Spacebasil Day24 Leaves are just like #SolarArray of #ISS! pic.twitter.com/2s005Pbm5r
— NOGUCHI, Soichi 野口 聡一(のぐち そういち) (@Astro_Soichi) March 12, 2021
Comparison between the ISS and the ground data
The Japanese Space Agency (JAXA) AHiS Project team is looking for the following data:
- Observations on the growth of your lot of sweet basil plants. Think about why plants grew well and why they didn’t.
- Observations on the difference between the microgravity on the ISS and Earth’s gravity – 1G, by comparing your experiments with the one on the ISS.
The New Zealand Astrobiology Network will evaluate the participants’ reports from a scientific perspective.
You will compare growth such as stem length, leaf size, leaf color and number of leaves. At the end of the 30 days, we will also look at the glandular hair cells on the back of leaves, and count them.
Let’s find out how these are different from the sweet basil grown on the ISS.
What is the difference between under the ISS environment and your experiment conditions? These differences may significantly affect the results of growth experiment.
- Temperature
- Humidity
- Light
- Fertilizer
- Growth medium
- CO2 concentration
- Plant chamber (ventilation efficiency, water supply volume, plant density)
- Presence or absence of gravity
↓
What will change when you change these?
Furthermore, you can try different conditions on the ground to find the more suitable conditions for the growth of sweet basil, such as changing the plant box, fertiliser’s concentration, and the number of seeds sown in the plant box.
Submit your results and you will go in the draw to win a prize.
You can either write a report or produce an electronic poster of your experiment.
Here is what we require from you:
What to write in your report / poster
The structure of a general experiment report is as follows:
- Experimenter’s name(s) (Your name)
- Date started and the duration of the experiment
- Objective: What does the experiment observe?
- Experimental method: How did you make the plant box / what type of plant box did you use, what was the growing environment, what kind of work and how did you do it?
- Results: What kind of results did you get? (Please use “Plant growth records, photographs, Graph, Table, etc.” to make it easy to understand.)
- Discussion: What did you think of the obtained experimental results? (For example, what is the cause of the difference in growth between the ISS and the ground?)
Submit your results and win
How to grow your basil
Warmth
Sweet basil grows well in a warm environment, with the optimum temperature being 22 to 30 degrees Celsius and it does not like cold climates.
Plenty of light
Sweet basil also likes light in order to grow well. If it is too dark, sweet basil will not grow healthy.
When growing it indoors, keep it as close as possible to the fluorescent lights in the room or place the container closer to a desk light.
CO2
The CO2 concentration inside the ISS is higher than on the ground. However, it may be difficult for you to produce the same CO2 concentration like the one on the ISS so JAXA does not recommend anything about maintaining the same the CO2 levels.
Basil is a very popular plant and even though is mostly associated with Mediterranean cuisine, it is likely originated from India. Sweet basil is an annual herb of the mint family (Lamiaceae). Other famous plants in the same family are lavender and rosemary, thyme and even the famous catnip. (Encyclopaedia Britannica, 2021).
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
In 1963, Valentina Tereshkova became the first woman in space when she launched aboard the Soviet space program’s Vostok 6. To this day, she remains the only woman to have completed a solo space mission. The Vostok 6 mission lasted three days and orbited the Earth a total of 48 times.
Tereshkova was born in 1937 in the village of Bolshoye Maslennikovo in central Russia. Her father was killed in the Finnish Winter War, part of World War II, when she was two years old. She attended school up until age 17, after which she began working in the tyre and textile mill industries whilst completing correspondence courses at the Light Industry Technical School to continue her education. Outside of her work and studies, Tereshkova developed an interest in skydiving and completed her first jump when she was 22. It was her experience in skydiving that would lead to her selection as a cosmonaut.
The head of the Soviet cosmonaut training program, Nikolai Kamanin, decided as a part of the Space Race that the U.S.A. could not be the first to put a woman in space and begun the recruitment process for female cosmonauts. Criteria to be a female cosmonaut included being younger than 30, no taller than 170 centimetres, and having experience with parachuting. In 1962, five candidates were chosen to enter the cosmonaut training process including Valentina Tereshkova, Zhanna Yorkina, Irina Solovyeva, Valentina Ponomaryova, and Tatyana Kuznetsova. In May 1963, Valentina Tereshkova was selected to fly Vostok 6.
The Vostok 6 spacecraft was operated predominantly from the ground by the Soviet space program. During the mission, data was collected to help study the effects of spaceflight, such as the zero-gravity environment, on the female body. Photography carried out by Tereshkova during the mission was later used to study the atmosphere.
In the same year as the Vostok 6 mission, Tereshkova married the Soviet cosmonaut Andrian Nikolayev, and went on to have a daughter named Elena Andrianovna Nikolaeva-Tereshkova. Being the first child born to both a mother and father who had been exposed to space, Elena received a lot of medical interest. Following the Vostok 6 mission, Valentina Tereshkova went on to attain the rank of major general in the Air Force and to hold several political offices as a part of the Communist Party of the Soviet Union.
The New Zealand Astrobiology Network is the Country Coordinator for the World Space Week. Find out more from our page here. This year, the theme of the World Space Week is Women in Space.
Everyone can participate in the World Space Week, which is an international celebration of the advancements created by space activities.
To start the year, we interviewed Maruška Strah, Executive Director of the World Space Week who gives an overview of what World Space Week is about.
Learn about New Zealand's first official space mission as a country, MethaneSAT.
New Zealand will contribute with an Atmospheric science programme, funded from Catalyst: Strategic over 4 years and a Mission Operations Control Centre, funded from the Strategic Science Investment Fund.
In 2020, World Space Week’s theme was “Satellites Improve Life” and the New Zealand Astrobiology Network took this opportunity to interview Dr Peter Crabtree, Head of the NZ Space Agency, Dr Sara Mikaloff-Fletcher, NZ Lead Researcher for MethaneSAT and Dr. Steven Hamburg, Chief Scientist, EDF, as New Zealand joined its first official space mission to combat climate change. The interview was conducted by Haritina Mogoșanu, Executive Director of the New Zealand Astrobiology Network and held at Space Place at Carter Observatory in Wellington, during World Space Week 2020.
by it’s chemical formula CH4, methane is a powerful greenhouse gas, that contributes to global warming, as it traps heat 28 times more effectively than carbon dioxide over a 100-year timescale.
Methane is produced under conditions where little to no oxygen is available. About 30% of methane emissions are produced by wetlands, including ponds, lakes, and rivers. Another 20% is produced by agriculture, due to a combination of livestock, waste management and rice cultivation. Activities related to oil, gas, and coal extraction release an additional 30%.
Concentrations of methane have increased by more than 150% since industrial activities and intensive agriculture began. After carbon dioxide, methane was responsible for about 23% of climate change in the 20th century.
data compiled from MBIE’s MethaneSAT mission and NASA’s Video: Methane Sources
Transcript of the interview:
Haritina Mogoșanu: The World Space Week Association is the global coordinator For the World Space Week Under the guidance of the United Nations’ Committee on the Peaceful Uses of Outer Space COPUOUS and the United Nations office for Outer Space Affairs.
Every year, the World Space Week Association Board chooses a theme. In 2020, the theme was “Satellites Improve Life”. New Zealand has joined its first official space mission as a country to combat climate change. It’s called MethaneSAT, and the mission’s Control Centre will be located here in New Zealand. I’m here with Dr Peter Crabtree, the head of the New Zealand Space Agency and Dr Sara Mikaloff-Fletcher, Lead Researcher for the mission.
Kia Ora Peter and Sara, it is a real pleasure to have you here.
Kia Ora
Peter, what is MethaneSAT?
Dr. Peter Crabtree: MethaneSAT is a mission with the objective of sensing atmospheric methane concentrations. And so with the idea that we gain better information, about those concentrations, and that will enable people to make better decisions and to understand the phenomenon much better.
Why has New Zealand chosen a partnership with the Environmental Defence Fund in the US for our first official space mission?
Thank you, that’s a good question. There are two answers to that on the one hand we were thinking, prior to this, about doing something in the climate science area and that being a really good objective for New Zealand given our interest as a nation from a policy perspective and so on, and then, on the other hand, there was an opportunity that came towards us to participate and be a partner in a really cutting edge space mission that also was going to happen with what we thought was a reasonable time frame given the pace that we were moving at, which was quite quick. So the idea of working with an organisation that was going to be quite nimble in putting together a space mission, when sometimes some space missions can be put together over very long period of time, and we saw this as a real opportunity for New Zealand to step into something that was really quite a serious endeavour but something that could really assist us as a nation in quite a number of different ways.
Let’s cross over to Steven Hamburg from EDF, Steven could you please tell us a little bit more
Dr. Steven Hamburg: Hello Hari, Peter and Sara it’s great to be with you and it’s great to have an opportunity to talk about MethaneSAT a mission that I’m passionate about.
The idea of MethaneSAT started a few years ago in conversation between Steve Wofsy, a professor at Harvard University and myself about the need to be able to collect methane flux data, how much methane was being emitted from around the world, and we didn’t have that capacity and without that knowledge we really couldn’t take advantage of the opportunity to reduce methane emissions because we did not know where it was occurring.
So we determined what we would need from a satellite and then went to the technology experts and asked, could we push the envelope on the technology to build the capacity inflight in space. And while we were pushing the envelope, that technology has evolved and is now possible, and MethaneSAT is the product of that integration of new technology, innovative science and the inversion technology that Steve has pioneered, into a program that allows us to do the advocacy to bring that data to the rest of the world.
And EDF, the Environmental Defence Fund, is well situated to lead this effort. EDF was founded by a group of scientists who understood a problem but did not have the tools to implement the understanding into policy that resulted from that knowledge. And that initial problem was the impacts of DDT on birds of prey in eastern United States. So they got together and formed the Environmental Defence Fund, hired a lawyer and then, using their science, went to look at and implement the needed ban on DDT, which was implemented in the early 1970s.
So with methane emissions from oil and gas industry, we understand the impact it’s having on the climate but we didn’t have the tools to bring that data and understanding to the many oil and gas producing regions of the world so that we could reduce those emissions and greatly slow the rate of warming.
MethaneSAT is very different than many other missions in that as I mentioned we started with the problem, and then went to look at the solutions. Could the technologies provide the data necessary to address that problem? We build an amazing team led by Tom Ingersoll who comes out of the commercial space community, of people who are really committed to ensuring that you we can use space technology to help society address one of the biggest crisis we ever faced which is climate change. And so by getting the best of the space technology community together with the best of the scientific community, in partnership with New Zealand, which has been an incredible opportunity to really push this mission forward fast and implement it effectively, we are very much looking forward to the operation centre being in New Zealand and to getting the satellite launched and the data flowing so that we can start to figure out where those methane emissions are coming from and ensure that people understand how those emissions can be mitigated and in turn getting that job done.
New Zealand is a wonderful partner in that there is a real commitment to bringing good science to bear on the needs of society writ large and that is the mission of EDF and so we are really very pleased to have the partnership with the New Zealand Government and the science community.
We are partnering with New Zealand because it’s a real natural fit. The focus of the Ministry for Business, Innovation and Employment on the use of science to help improve New Zealand society and the well-being of your citizens fits wonderfully into the objectives of this mission and to the DNA of EDF as an organisation for these fifty plus years. So by taking advantage of the scientific knowledge that already exists in New Zealand and to help develop the nascent space capacity in the country we were able to accelerate progress on the mission while developing the skill sets in New Zealand. It’s a partnership that we very much value, and are confident will persist and enhance the work we are doing together over the coming years.
Thank you Steven.
I have a couple of questions for Sara
What is novel about the satellite mission?
Dr Sara Mikaloff-Fletcher: So many things.
It’s an amazing mission! I mean for me, on the technical side, there are two big things. One is that it’s the first time we’re going to have a satellite flying in the sky that’s going to be able to measure methane with the kind of precision we would expect to have of someone on my team tried to measure it with an instrument on the ground. That’s extraordinary! The other thing is the spatial resolution so this thing is going to capture a 200 x 200 km scene and within that scene is going to do a raster scan with very high precision so we will be able to pick up exactly where these emissions are happening; but then on the policy side, it’s the first satellite that’s been purposely designed to support and enable climate action.
So there are two big things happening there, one is that they are going to have inverse modelling as part of the whole framework, which is the modelling tool you used to go from what the satellite measures, which is the concentration, to what you need for policy action which is to know the emissions. So that’s going to be happening live throughout the satellite’s mission, and then in addition to that is the impact in communicating as quickly so that we can empower people to be able to reduce these emissions.
Tell me Sara,
What relevant expertise do we have here in New Zealand to contribute to MethaneSAT science?
Well we have quite a big going on in New Zealand. New Zealand has been a leader in greenhouse gas measurements, since before I was born. In fact, when I was a PhD student coming up at NOAA, which is kind of our opposite number in the US, NIWA was already famous to me for having the best methane isotopes almost anywhere in the world. And so we have this amazing rich history of these atmospheric measurements both on the ground and also in the total air column. So you can imagine that you have a satellite it’s flying around looking down trying to measure things. To make sure that you get that satellite measurement right it’s really helpful to have an instrument on the ground that looks up. It’s a similar type of instrument but it’s on the ground so there are all kinds of extra things you can do to work out what you’re seeing when you have something that’s ground based.
So New Zealand has one of the two initial ground-based instruments like this, they are called TCCON (Total Column Carbon Observing Network) instruments. They support all types of satellite activities and will be supporting MethaneSat as well. And then the third big thing is the modelling. We have already a well-developed modelling framework that’s operating at a very high resolution, where we’ll be able to be right in there with that modelling to be able to turn those concentrations that we’re seeing in the satellite into the emissions we need to take policy action.
The next question is for Peter.
What will New Zealand get out of being part of this mission?
Dr. Peter Crabtree: Quite a lot! There is a number of elements.
One element is that the mission control for this programme is going to be based in New Zealand, so we get to participate in the programme from an engineering perspective, setting up the mission control functions and all the protocols around the mission control itself. From a space capability perspective, that’s a really good opportunity for us to step into the idea of hosting a world class space mission. So, very much for the space systems people, very excited about it from that perspective.
Then on the other side of things is the science. It’s really around the fact that we get to stand alongside some international partners like Harvard University and the Smithsonian and work with them on the science programme. New Zealand is going to lead the agricultural emissions side of that, and with the United States in particular focused on oil and gas emissions, with methane emissions as well. We love the idea of international science partnerships that are operating at that level, they really help us get more impact out of our science programmes.
So those are two elements, and really, the third bit, is from a policy perspective is New Zealand being able to make better informed decisions when we come to think around our own climate policy and so on.
Sara what are your plans for working with the Harvard team working on oil and gas industry methane?
Dr Sara Mikaloff-Fletcher: Another thing about MethaneSAT that we haven’t talked about is that it was purpose designed to be able to tackle anthropogenic emissions, mostly from oil and gas. That’s because these are really the low hanging fruit of climate action. If you tell people where a leak is, because it’s usually an accidental leak, then you have a really good chance that those people are going to be excited to go fix that leak and reduce our methane. But there is tremendous opportunity to be able to use the same data that are designed to be able to detect these oil and gas leaks for agricultural problems.
So we also have agricultural emissions of methane from sheep, cows, rice patties, those types of things, and the aim of the New Zealand-based science project is to develop the capability to use these data to detect those agricultural emissions not only giving New Zealand some of the best information anywhere in the world about our agricultural emissions but also helping to design a framework for how the international team can pick other places they might want to look at and target to support climate action there.
Peter the theme of world space week this year is “satellites improve life” what other satellite activities is the New Zealand space agency involved in?
Dr. Peter Crabtree: New Zealand is a pretty young space actor. We have a space sector now which is about $1.7 billion dollars worth of activity, but we are still quite young. In terms of satellite development, a lot of our effort is going largely into educational institutions probably smaller scale satellite programmes, cubesat opportunities. Which start to, on the one hand demonstrate what you can do with small satellites, as a capability, and the things you can do with small satellites every day, like miniaturisation across all technology is that is ever expanding. We are also really interested from a government perspective as what are the government’s needs that can be better addressed through satellites.
So really, at the moment, we are spending a lot of time across government working with lots of agencies that have an interest and have had for a long time often used Earth observation, but is really about the New Zealand government being a super user of satellites. I think, over time, that will lead us to getting clearer about which area we want to invest in, in particular when it comes to the satellite capabilities. We are on a journey at the moment.
And would you like to see New Zealand making greater use of satellite data?
Absolutely! It’s quite a challenge for a lot of people who have not been exposed to the possibilities of this, and there are a lot of things we do that at the moment, we might be on Earth, and might measure in certain ways, and it’s often quite labour-intensive and resource-intensive but also the issue around frontier technologies like this is that they push the boundaries of what might be possible.
So what if, from space, you could, every day you could track, or every week, we could track if we were winning the battle against possums in our conservationist state? Suddenly on your desktop you would have AI, robots essentially, being able to tell you that those species are thriving or not thriving. And so we are interested, we are seeing those kinds of possibilities all over the place and it’s a question of getting the customer or the potential users to understand that is a real possibility, and on the other hand that we fast track our technology development so that we can actually give people these types of solutions, is really really exciting times.
Haritina Mogosanu: This is what World Space Week is all about, bringing space technology here to people on Earth, so we are on a very good path.
Thank you very much Peter and Sara for your time and for coming here and Happy World Space Week!
On the 18th of March 2021, the community gathered at KaPai soup round 4, voted Cosmic Star Safari to be the winner of the $1070 prize in cash.
Thank you to everyone for their stellar generosity and for voting for us. Special thanks to Kapai Soup for inviting us to join the bidding team.
At the end of the programme, we would like to invite everyone who was at the Kapai Soup Carterton on the 18th of March to attend the wrap-up of the Cosmic Star Safari at Stonehenge Aotearoa.
The event will be free for the attendees of Kapai Soup on the 18th of March 2021.
What is a Cosmic Star Safari?
Cosmic Star Safari is a one year space and astronomy programme for a lucky school.
Here are the space and astronomy-related projects and milestones that are part of it:
Milestone 1. Our portable planetarium visits the school.
Milestone 2. The school visits Stonehenge Aotearoa.
Throughout the year, 30 students get to access robotic telescopes in Chile and the Canary Islands.
Milestone 3. After one year, the school creates a temporary exhibition from what they learned during the online astronomy programme.
Cosmic Star Safari is provided by NZAN with support from Milky-Way.Kiwi and Stonehenge Aotearoa
What will happen now?
Schools can win a Cosmic Star Safari by doing their own pitch, telling us why they should get a Cosmic Star Safari.
Keep an eye on social media and our website to learn what you need to do. Like us on Facebook, Instagram and Twitter or subscribe to our blog to be the first to find out.
To grow for an entire month, your seeds will need water, light, an atmosphere and also food.
In the AHiS space experiments JAXA used OAT house series fertiliser as nutrient for growing sweet basil.
However, we might not find this in New Zealand. JAXA advises to use instead hydroponics fertiliser or any fertiliser for vegetables. Make sure you follow the manufacturer’s instructions on how to dilute and prepare it.

You may substitute the fertiliser with a supernatant resulted from mixing soil and water and is let to sit for a while. The soil contains various elements necessary for the plants’ growth, which dissolve into water after mixing the water and soil.
Let the solution sit a while – half a day to a day and the soil and water will be separate.
Remove the residues on top and use the aqueous solution resulted (this is the supernatant) as a fertiliser for your seeds.
If you are experimenting with soil as a medium, you do not need fertiliser. The soil contains the elements necessary for plant growth.
The OAT house series fertiliser used on the ISS contains major elements and trace amounts of metal ions necessary for plant growth and has the following chemical composition:
https://www.oat-agrio.co.jp/cgi/psearch/item/2013101716413104/index.html
In the AHiS experiment on the ISS, OAT house #1 powder and OAT house #2 powder are dissolved in water at 0.3% and 0.2%, respectively. For example, 3.0 g of OAT house #1 and 2.0 g of OAT house #2 fertilizer powder are dissolved in 1000 mL of bottled water. As a result, the following is the final concentration. This is filled in the watering syringes.
Concentrated
OAT house fertiliser
OAT house #1 | OAT house #2 |
TN (Total nitrogen) * 10.0% | TN (Total nitrogen) 11.0% |
P2O5 (phosphorus) 8.0% | Ca (calcium) 16.4% |
K2O (potassium) 27.0% | |
MgO (magnesium) 4.0% | |
MnO (manganese) 0.10% | |
B2O3 (boron) 0.10% | |
Fe (ferrum) 0.18% | |
Cu (copper) 0.002% | |
Zn (zinc) 0.006% | |
Mo (molybdenum) 0.002% |
*Total nitrogen includes ammoniacal nitrogen and nitrate nitrogen.
OAT house fertiliser’s concentration after dissolving it with water
OAT house #1 | OAT house #2 |
TN (Total nitrogen) 0.030% | TN (Total nitrogen) 0.022% |
P2O5 (phosphorus) 0.024% | Ca (calcium) 0.0328% |
K2O (potassium) 0.081% | |
MgO (magnesium) 0.012% | |
MnO (manganese) 0.0003% | |
B2O3 (boron) 0.0003% | |
Fe (ferrum) 0.00054% | |
Cu (copper) 0.000006% | |
Zn (zinc) 0.000018% | |
Mo (molybdenum) 0.000006% |
Did you know?
The fertiliser solution used on the International Space Station to grow the basil seeds comes from space. Except for hydrogen, some helium and lithium, which were formed after the Big Bang, all other chemical elements we have here on Earth have once been in a star. This means, you are made of stardust too!
The following two tables show nutritional elements (what we need to survive) and where were they formed (in which type of stars or processes)
Growing conditions
Record all information or data you have about the growing conditions of your plants, for instance you can take readings of the daily temperature, humidity and light.
The more readings you take, the better your information will be for analysing your investigation results and drawing conclusions for your research paper / poster.
Describe these conditions in detail, so we can understand what your measurements were about.
Ideally, everyone should conduct the research under the same conditions but it is difficult to maintain the same temperature, humidity or lighting levels across all the schools in New Zealand. To be able to make a comparison between all the seeds grown in schools, it is a very good idea to write down as much as you can about your particular conditions.
All collected data should be recorded regularly in a personally designed data logbook or using a data sheet.

Basic characteristics
The following are basic characteristics that you may choose to observe, measure, and record for your seeds
- Germination rate: Record the number of seeds that sprout and the date that each sprout appeared. Monitor how many of the seeds sprout within the first two weeks.
- Plant height: Measure and record this measurement daily.
- The number of leaves: Count and record daily.
- Observation of glandular hair cells on the leaves: Behind the leaves of basil plants are glandular hair cells that secrete essential oils. Let’s observe the shape of the cell. You will have to use a microscope or magnifying glass for this experiment, to observe glandular hairs.
- Aroma: describe the scent of the leaves.
#きょうのバジル 24日目。きょうはうえからもかんさつしたよ。はっぱが太陽電池パネルみたいにおおきく広がってるのがわかるね! #Spacebasil Day24 Leaves are just like #SolarArray of #ISS! pic.twitter.com/2s005Pbm5r
— NOGUCHI, Soichi 野口 聡一(のぐち そういち) (@Astro_Soichi) March 12, 2021
Comparison between the ISS and the ground data
The Japanese Space Agency (JAXA) AHiS Project team is looking for the following data:
- Observations on the growth of your lot of sweet basil plants. Think about why plants grew well and why they didn’t.
- Observations on the difference between the microgravity on the ISS and Earth’s gravity – 1G, by comparing your experiments with the one on the ISS.
The New Zealand Astrobiology Network will evaluate the participants’ reports from a scientific perspective.
You will compare growth such as stem length, leaf size, leaf color and number of leaves. At the end of the 30 days, we will also look at the glandular hair cells on the back of leaves, and count them.
Let’s find out how these are different from the sweet basil grown on the ISS.
What is the difference between under the ISS environment and your experiment conditions? These differences may significantly affect the results of growth experiment.
- Temperature
- Humidity
- Light
- Fertilizer
- Growth medium
- CO2 concentration
- Plant chamber (ventilation efficiency, water supply volume, plant density)
- Presence or absence of gravity
↓
What will change when you change these?
Furthermore, you can try different conditions on the ground to find the more suitable conditions for the growth of sweet basil, such as changing the plant box, fertiliser’s concentration, and the number of seeds sown in the plant box.
Submit your results and you will go in the draw to win a prize.
You can either write a report or produce an electronic poster of your experiment.
Here is what we require from you:
What to write in your report / poster
The structure of a general experiment report is as follows:
- Experimenter’s name(s) (Your name)
- Date started and the duration of the experiment
- Objective: What does the experiment observe?
- Experimental method: How did you make the plant box / what type of plant box did you use, what was the growing environment, what kind of work and how did you do it?
- Results: What kind of results did you get? (Please use “Plant growth records, photographs, Graph, Table, etc.” to make it easy to understand.)
- Discussion: What did you think of the obtained experimental results? (For example, what is the cause of the difference in growth between the ISS and the ground?)
Submit your results and win
How to grow your basil
Warmth
Sweet basil grows well in a warm environment, with the optimum temperature being 22 to 30 degrees Celsius and it does not like cold climates.
Plenty of light
Sweet basil also likes light in order to grow well. If it is too dark, sweet basil will not grow healthy.
When growing it indoors, keep it as close as possible to the fluorescent lights in the room or place the container closer to a desk light.
CO2
The CO2 concentration inside the ISS is higher than on the ground. However, it may be difficult for you to produce the same CO2 concentration like the one on the ISS so JAXA does not recommend anything about maintaining the same the CO2 levels.
Basil is a very popular plant and even though is mostly associated with Mediterranean cuisine, it is likely originated from India. Sweet basil is an annual herb of the mint family (Lamiaceae). Other famous plants in the same family are lavender and rosemary, thyme and even the famous catnip. (Encyclopaedia Britannica, 2021).
WEEK SUMMARY TITLES
Learn about Mars and Perseverance with Mitch Schulte
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales Carol Oliver is an Associate Professor with...
Peggy Whitson: First Female Space Station Commander
Caitlin MacArthur, first female space station commander, most time in space, peggy whitson, Women in Space, world space week, 0Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight...
Valentina Tereshkova: First Woman in Space
Caitlin MacArthur, valentina tereshkova, Women in Space, world space week, 0In 1963, Valentina Tereshkova became the first woman in space when she launched aboard the Soviet space program’s Vostok...
World Space Week 2021 is about women in space. We interviewed the Executive Director of the World Space Week...
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
In 1963, Valentina Tereshkova became the first woman in space when she launched aboard the Soviet space program’s Vostok 6. To this day, she remains the only woman to have completed a solo space mission. The Vostok 6 mission lasted three days and orbited the Earth a total of 48 times.
Tereshkova was born in 1937 in the village of Bolshoye Maslennikovo in central Russia. Her father was killed in the Finnish Winter War, part of World War II, when she was two years old. She attended school up until age 17, after which she began working in the tyre and textile mill industries whilst completing correspondence courses at the Light Industry Technical School to continue her education. Outside of her work and studies, Tereshkova developed an interest in skydiving and completed her first jump when she was 22. It was her experience in skydiving that would lead to her selection as a cosmonaut.
The head of the Soviet cosmonaut training program, Nikolai Kamanin, decided as a part of the Space Race that the U.S.A. could not be the first to put a woman in space and begun the recruitment process for female cosmonauts. Criteria to be a female cosmonaut included being younger than 30, no taller than 170 centimetres, and having experience with parachuting. In 1962, five candidates were chosen to enter the cosmonaut training process including Valentina Tereshkova, Zhanna Yorkina, Irina Solovyeva, Valentina Ponomaryova, and Tatyana Kuznetsova. In May 1963, Valentina Tereshkova was selected to fly Vostok 6.
The Vostok 6 spacecraft was operated predominantly from the ground by the Soviet space program. During the mission, data was collected to help study the effects of spaceflight, such as the zero-gravity environment, on the female body. Photography carried out by Tereshkova during the mission was later used to study the atmosphere.
In the same year as the Vostok 6 mission, Tereshkova married the Soviet cosmonaut Andrian Nikolayev, and went on to have a daughter named Elena Andrianovna Nikolaeva-Tereshkova. Being the first child born to both a mother and father who had been exposed to space, Elena received a lot of medical interest. Following the Vostok 6 mission, Valentina Tereshkova went on to attain the rank of major general in the Air Force and to hold several political offices as a part of the Communist Party of the Soviet Union.
The New Zealand Astrobiology Network is the Country Coordinator for the World Space Week. Find out more from our page here. This year, the theme of the World Space Week is Women in Space.
Everyone can participate in the World Space Week, which is an international celebration of the advancements created by space activities.
To start the year, we interviewed Maruška Strah, Executive Director of the World Space Week who gives an overview of what World Space Week is about.
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
In 1963, Valentina Tereshkova became the first woman in space when she launched aboard the Soviet space program’s Vostok 6. To this day, she remains the only woman to have completed a solo space mission. The Vostok 6 mission lasted three days and orbited the Earth a total of 48 times.
Tereshkova was born in 1937 in the village of Bolshoye Maslennikovo in central Russia. Her father was killed in the Finnish Winter War, part of World War II, when she was two years old. She attended school up until age 17, after which she began working in the tyre and textile mill industries whilst completing correspondence courses at the Light Industry Technical School to continue her education. Outside of her work and studies, Tereshkova developed an interest in skydiving and completed her first jump when she was 22. It was her experience in skydiving that would lead to her selection as a cosmonaut.
The head of the Soviet cosmonaut training program, Nikolai Kamanin, decided as a part of the Space Race that the U.S.A. could not be the first to put a woman in space and begun the recruitment process for female cosmonauts. Criteria to be a female cosmonaut included being younger than 30, no taller than 170 centimetres, and having experience with parachuting. In 1962, five candidates were chosen to enter the cosmonaut training process including Valentina Tereshkova, Zhanna Yorkina, Irina Solovyeva, Valentina Ponomaryova, and Tatyana Kuznetsova. In May 1963, Valentina Tereshkova was selected to fly Vostok 6.
The Vostok 6 spacecraft was operated predominantly from the ground by the Soviet space program. During the mission, data was collected to help study the effects of spaceflight, such as the zero-gravity environment, on the female body. Photography carried out by Tereshkova during the mission was later used to study the atmosphere.
In the same year as the Vostok 6 mission, Tereshkova married the Soviet cosmonaut Andrian Nikolayev, and went on to have a daughter named Elena Andrianovna Nikolaeva-Tereshkova. Being the first child born to both a mother and father who had been exposed to space, Elena received a lot of medical interest. Following the Vostok 6 mission, Valentina Tereshkova went on to attain the rank of major general in the Air Force and to hold several political offices as a part of the Communist Party of the Soviet Union.
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
In 1963, Valentina Tereshkova became the first woman in space when she launched aboard the Soviet space program’s Vostok 6. To this day, she remains the only woman to have completed a solo space mission. The Vostok 6 mission lasted three days and orbited the Earth a total of 48 times.
Tereshkova was born in 1937 in the village of Bolshoye Maslennikovo in central Russia. Her father was killed in the Finnish Winter War, part of World War II, when she was two years old. She attended school up until age 17, after which she began working in the tyre and textile mill industries whilst completing correspondence courses at the Light Industry Technical School to continue her education. Outside of her work and studies, Tereshkova developed an interest in skydiving and completed her first jump when she was 22. It was her experience in skydiving that would lead to her selection as a cosmonaut.
The head of the Soviet cosmonaut training program, Nikolai Kamanin, decided as a part of the Space Race that the U.S.A. could not be the first to put a woman in space and begun the recruitment process for female cosmonauts. Criteria to be a female cosmonaut included being younger than 30, no taller than 170 centimetres, and having experience with parachuting. In 1962, five candidates were chosen to enter the cosmonaut training process including Valentina Tereshkova, Zhanna Yorkina, Irina Solovyeva, Valentina Ponomaryova, and Tatyana Kuznetsova. In May 1963, Valentina Tereshkova was selected to fly Vostok 6.
The Vostok 6 spacecraft was operated predominantly from the ground by the Soviet space program. During the mission, data was collected to help study the effects of spaceflight, such as the zero-gravity environment, on the female body. Photography carried out by Tereshkova during the mission was later used to study the atmosphere.
In the same year as the Vostok 6 mission, Tereshkova married the Soviet cosmonaut Andrian Nikolayev, and went on to have a daughter named Elena Andrianovna Nikolaeva-Tereshkova. Being the first child born to both a mother and father who had been exposed to space, Elena received a lot of medical interest. Following the Vostok 6 mission, Valentina Tereshkova went on to attain the rank of major general in the Air Force and to hold several political offices as a part of the Communist Party of the Soviet Union.
The New Zealand Astrobiology Network is the Country Coordinator for the World Space Week. Find out more from our page here. This year, the theme of the World Space Week is Women in Space.
Everyone can participate in the World Space Week, which is an international celebration of the advancements created by space activities.
To start the year, we interviewed Maruška Strah, Executive Director of the World Space Week who gives an overview of what World Space Week is about.
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.

Peggy Whitson’s first space mission took place in 2002 aboard the International Space Station’s Expedition 5 as a flight engineer. In 2007, Whitson returned to the International Space Station aboard the Expedition 16 mission as the commander, which made her the first woman commander of the International Space Station. Whitson’s third and final trip to the International Space Station was aboard Expedition 50/51 whereby she was again the commander. This in turn made her the first woman to be commander of the International Space Station twice. During Expedition 50/51, Whitson became the oldest woman to ever travel to space at 57 years of age. Over the course of her career as an astronaut, Whitson has spent the most time in space for any woman at a total of 665 days. In addition to this, Whitson was also the first woman to be appointed to the position of Chief of the Astronaut Office at NASA in 2009.
Whitson holds a doctorate degree in biochemistry, with her thesis topic being “The lactose repressor-operator DNA interaction: chemical and physical studies of the complex (modification, equilibrium, protein, stopped-flow, kinetics).” Throughout her career, Whitson has also worked as a research scientist with NASA in the fields of biochemistry and medical sciences. She received her doctorate degree in 1986 and worked at NASA-JSC in the Biomedical Operations and Research Branch in biochemistry research from 1989 to 1993. When she was selected as an astronaut candidate in 1996, she was working at the Johnson Space Center as the deputy division chief of the Medical Sciences division.
The Expedition 5 mission consisted of the astronauts continuing scientific investigations aboard the ISS as were begun by the previous mission, as well as carrying out around 25 new investigations. These investigations included investigating the growth of soybeans in space conditions, investigating the effects of spaceflight on the human body, and making observations of Earth from the ISS viewpoint. During the re-entry to Earth from Expedition 16 on the Soyuz TMA-11 spacecraft, a malfunction led to the astronauts experiencing forces of around 10 G due to a very disorderly descent. Despite this, all astronauts were in good health upon landing. Expedition 50/51 involved investigating the growth of vegetables in the NASA Vegetable Production System, such as Chinese cabbage. It was during Expedition 50/51 that Whitson broke the record for the most time spent in space.
Learn about the Perseverance Rover with NASA scientist Mitch Schulte. Mitch is also Principal Adviser of the New Zealand Astrobiology Network.
Mitch talks to us about Perseverance, Mars regolith, asterisms, working from home and we are listening to sounds from Mars and try to find out how our voices would sound like if we were on Mars. You can do this too at mars.nasa.gov/mars2020/participate/sounds/ Simply record yourself and then play it back.
The interview was taken in July 2021 by Hari Mogoșanu and Sam Leske.
A/Prof Carol A. Oliver PhD, MSciCom, SFHEA, University of New South Wales

Carol Oliver is an Associate Professor with the University of New South Wales (UNSW) in Sydney, teaching astrobiology and science communication. She is a Fellow of UNSW’s Scientia Education Academy, a Senior Fellow of the UK Higher Education Academy, and in 2022 won the UNSW Vice Chancellor’s Award for Teaching Excellence.
Carol is Deputy Director of the iCinema Research Centre currently collaborating on a $5m Australian Research Council grant, and a member of the Australian Centre for Astrobiology, both at UNSW. She is also a founder and now international associate of the Education Through Exploration Centre at Arizona State University.
Carol’s grant record includes more than AUD$5.5 million for astrobiology-related education programs, leading national and international teams. She pioneered the first astrobiology-related immersive laptop delivered Virtual Field Trip with NASA Learning Technologies in 2007 and is internationally recognised for her VFT development of both the pedagogy and the technology.