‘Star Trek into Darkness’ & NASA Station Crews Join Forces at Live NASA Webcast

NASA and Star Trek connect on NASA TV on May 16 for the premiere of “Star Trek Into Darkness” on May 17, 2013 to celebrate the wonders of Space Exploration. Still image of the fictional star ship ‘Enterprise’. Credit: Star Trek

Science Fact and Science Fiction join forces in space today for a one of a kind meeting turning science fiction into reality – and you can participate courtesy of NASA and Hollywood!

Fictional astronauts and crews from the newest Star Trek incarnation; “Star Trek into Darkness” and real life astronauts taking part from outer space and Earth get connected today (May 16) via a live ‘space bridge’ webcast hosted by NASA. The movies premieres today – May 16.

NASA Television broadcasts the face-to-face meeting as a Google+ Hangout from noon to 12:45 p.m. EDT, May 16. Watch live below!

The webcast includes “Captain Kirk” – played by actor Chris Pine, and NASA astronaut Chris Cassidy – fresh off from his real life ‘emergency spacewalk’ this past weekend that saved the critically important cooling system aboard the International Space Station (ISS). “Into Darkness” features dramatic life and death spacewalks.

Astronaut Chris Cassidy during the May 11, 2013 emergency spacewalk at the ISS. Credit: NASA
Astronaut Chris Cassidy during the May 11, 2013 emergency spacewalk at the ISS. Credit: NASA

Also participating in the live NASA webcast are ‘Star Trek’ director J.J. Abrams, screenwriter and producer Damon Lindelof; and actors Alice Eve (Dr. Carol Marcus) and John Cho (Sulu) and astronauts Michael Fincke and Kjell Lindgren at NASA’s Johnson Space Center in Houston.

Fincke flew on the Space Shuttle and the ISS and made a guest appearance on the finale of the TV series – “Star Trek: Enterprise”. See photo below.

‘Star Trek Into Darkness’ movie still image. Credit: Star Trek
‘Star Trek Into Darkness’ movie still image. Credit: Star Trek

The ISS is a sort of early forerunner for the fictional ‘Federation’ in the ‘Star Trek’ Universe – constructed in low Earth orbit by the combined genius and talents of 5 space agencies and 16 nations of Earth to forge a united path forward for the peaceful exploration of Outer Space.

Cassidy will provide insights about everyday life aboard the real space station – like eating, sleeping, exercising and fun ( think Chris Hadfield’s guitar strumming ‘Space Oddity’ -watch the YouTube video below) – as well as the myriad of over 300 biological, chemical and astronomical science experiments performed by himself and the six person station crews during their six-month stints in zero gravity.

Astronaut Terry Virts, left, Actor Scott Bakula and Astronaut Mike Fincke, right, beam on the set of Star Trek's final Enterprise voyage. Credit: NASA
Astronaut Terry Virts, left, Actor Scott Bakula and Astronaut Mike Fincke, right, beam on the set of Star Trek’s final Enterprise voyage. Credit: NASA

The participants will ask questions of each other and take questions from the Intrepid Sea, Air & Space Museum in New York City (home of the space shuttle Enterprise), the Smithsonian’s National Air and Space Museum in Washington, and social media followers, says NASA.

Social media followers were allowed to submit 30 sec video questions until early this morning.

And you can submit questions today and during the live broadcast using the hashtag #askNASA on YouTube, Google+, Twitter and Facebook.

Captain Kirk and Mr. Spock in ‘Star Trek Into Darkness’. Credit: Star Trek
Captain Kirk and Mr. Spock in ‘Star Trek Into Darkness’. Credit: Star Trek

Watch the hangout live on NASA’s Google+ page, the NASA Television YouTube channel, or NASA TV starting at Noon EDT, May 16.

As a long time Star Trek fan (since TOS) I can’t wait to see ‘Into Darkness’

Ken Kremer

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Learn more about NASA missions, Mars, Curiosity and more at Ken’s upcoming lecture presentation:

June 12: “Send your Name to Mars” and “LADEE Lunar & Antares ISS Rocket Launches from Virginia”; Franklin Institute and Rittenhouse Astronomical Society, Philadelphia, PA, 8 PM.

NASA’s real life Space Shuttle Enterprise transits the NYC Skyline at Dusk on a barge on June 3, 2012 during a two stage seagoing  journey to her permanent  new home at the Intrepid Sea, Air and Space Museum. Enterprise is bracketed by the Empire State Building, The Freedom Tower (still under construction) and the torch lit Statue of Liberty. Credit: Ken Kremer
NASA’s real life Space Shuttle Enterprise transits the NYC Skyline at Dusk on a barge on June 3, 2012 during a two stage seagoing journey to her permanent new home at the Intrepid Sea, Air and Space Museum. Enterprise is bracketed by the Empire State Building, The Freedom Tower (still under construction) and the torch lit Statue of Liberty. Credit: Ken Kremer

More Insight on How NASA Might Revive the Kepler Space Telescope

Artst concept of the Kepler telescope in orbit. Credit: NASA

The future of NASA’s Kepler space telescope mission is in doubt, NASA announced yesterday, as it suffered a failure of a second reaction wheel, losing its ability to precisely point to look for planets orbiting other stars. Reaction wheels enable the spacecraft to aim in different directions without firing thrusters, and the spacecraft needs at least three of the four wheels working to provide the ability to point precisely enough to continue the mission.

But, as we pointed out in our article yesterday, the Kepler team said there are still possibilities of keeping the spacecraft in working order, or perhaps even finding other opportunities for different science for Kepler, something that doesn’t require such precise pointing abilities.

“We’re not ready to call the mission down and out just yet,” said John Grunsfeld, NASA’s associate administrator for the Science Mission Directorate, “but by any measure it’s been a spectacular mission.”

Space expert Scott Hubbard has provided additional insight on the possible ways that NASA could bring the spacecraft back online, and what planet hunters will do next if that’s not possible. Hubbard is a consulting professor of aeronautics and astronautics at Stanford’s School of Engineering, and served as director of NASA Ames Research Center during much of the building phase of the Kepler space telescope. He also worked on the project alongside William Borucki, the Kepler science principal investigator at Ames and the driving force behind the effort, for the decades leading up to formal approval of the mission.

Standford University provided this conversation Hubbard:

Q: How big of a loss will it be if the Kepler space telescope can’t be repaired?

Hubbard: The science returns of the Kepler mission have been staggering and have changed our view of the universe, in that we now think there are planets just about everywhere.

It will be very sad if it can’t go on any longer, but the taxpayers did get their money’s worth. Kepler has, so far, detected more than 2,700 candidate exoplanets orbiting distant stars, including many Earth-size planets that are within their star’s habitable zone, where water could exist in liquid form.

Kepler has done what the program managers said it would do, and that is to give us an inventory of extrasolar planets. It completed its primary observation phase, and had entered its extended science phase. We’re already in the gravy train period – there’s still a year and a half’s worth of data in the pipeline that scientists will analyze to identify other candidate planets, and there will continue to be Kepler science discoveries for quite some time.

Kepler space telescope's field of view. Credit: NASA
Kepler space telescope’s field of view. Credit: NASA

Q: How might NASA engineers go about getting Kepler functional again?

Hubbard: There are two possible ways to salvage the spacecraft that I’m aware of. One is that they could try turning back on the reaction wheel that they shut off a year ago. It was putting metal on metal, and the friction was interfering with its operation, so you could see if the lubricant that is in there, having sat quietly, has redistributed itself, and maybe it will work.

The other scheme, and this has never been tried, involves using thrusters and the solar pressure exerted on the solar panels to try and act as a third reaction wheel and provide additional pointing stability. I haven’t investigated it, but my impression is that it would require sending a lot more operational commands to the spacecraft.

Q: If neither of these options works, Kepler is still an amazing space instrument. Could it conduct other types of experiments?

Hubbard: People have asked about using it to find near-Earth objects, or asteroids. Kepler carries a photometer, not a camera, that looks at the brightness of stars, and so its optics deliberately defocus light from stars to create a nice spread of light on the detector, which is not ideal for spotting asteroids.

Whether or not it could function as a detector for asteroids is something that would have to be studied, but since it wasn’t built as a camera, I would say that I’m skeptical. That said, certainly between Ames Research Center and the Jet Propulsion Laboratory, they’ve got the best people in the world working on it.

Visualization of Kepler's planet candidates shown in transit with their parent stars. Credit: Jason Rowe/Kepler Mission/NASA
Visualization of Kepler’s planet candidates shown in transit with their parent stars. Credit: Jason Rowe/Kepler Mission/NASA

Q: What’s next for exoplanet hunters?

Hubbard: As I said earlier, there is still a year and a half’s worth of data in the pipeline to analyze to identify candidate planets, so there are still discoveries to be made.

It’s important to make clear, though, that in the original queue of missions aimed at finding life elsewhere, a mission like Kepler was a survey mission to establish the statistical frequency of whether these planets are rare or common. It lived the length of its prime mission, and was extremely successful during that time at achieving this goal. It has paved the way for additional missions, such as TESS – Transiting Exoplanet Survey Satellite – and TPF – Terrestrial Planet Finder – which will continue the search for Earth-like exoplanets in the near future.

Our Spoiler-Free Review of Star Trek: Into Darkness

Spock (Zachary Quinto) and Kirk (Chris Pine) as portrayed in Star Trek: Into Darkness. Credit: StarTrekMovie.com

If you’re a fan of the rebooted 2009 Star Trek film, we think you’ll love the second edition. You’ll find similar whip-cracking dialog, inside jokes and action-filled storyline in the sequel, Star Trek: Into Darkness, which opens in theaters in the United States and several other countries today.

While the first movie introduced us to the characters, this movie is all about choices… moral choices, and when it is best to help somebody, as opposed to letting things be. That’s where things can get uncomfortable, though.

The film’s start portrays a moral dilemma in the first few minutes, with choices that bring upon punishment for the players involved. The consequences are quite logical — Spock would point that out — but when more dilemmas pile up at the end of the film, many decisions go unquestioned.

Yes, this is an action film and yes, the Star Trek franchise is one that never lets itself get slowed down by plot holes and inconsistencies. (The plot isn’t that groundbreaking, either.) Still, the movie could have benefitted from an extra five or 10 minutes to show the reasoning behind the final few choices. Thinking over what happened, there could be problems with what the crew decided to do.

Nyota Uhura as seen in Star Trek: Into Darkness. Credit: StarTrekMovie.com
Nyota Uhura as seen in Star Trek: Into Darkness. Credit: StarTrekMovie.com

Enough Tribble-like quibbling, though. Star Trek: Into Darkness pulls you in with an action sequence in the first few minutes, and the pace never lets up. Spock (Zachary Quinto)’s straightforward nature gets him into trouble — as usual — with James T. Kirk (Chris Pine), leading to quotable insults that generated audience guffaws in an advance screening Universe Today saw in Ottawa, Canada.

There’s enough time and, well, space for other characters to shine as well. While Nyota Uhura (Zoë Saldana) spends ample screen time mooning about her boyfriend, she proves to be an excellent and forceful translator. Scotty (Simon Pegg) also has a wonderful back-and-forth sequence late in the movie, breaking up some intense moments with his slapstick humor.

Also: Another character comes along and — with a presence that commands attention on the big screen — threatens to steal the show from our heroes. You don’t want to like them, but as you get to know them you realize they have reasons behind their actions.

What did you think of the film? Please share your thoughts in the comments

Kepler Planet-Hunting Mission in Jeopardy

A diagram of the Kepler space telescope. Credit: NASA

NASA’s Kepler telescope has lost its ability to precisely point toward stars, putting its exoplanet search in jeopardy. One of the reaction wheels –devices which enable the spacecraft to aim in different directions without firing thrusters – has failed. This is of grave concern because last year reaction wheel #2 failed, and now #4 has failed. Kepler scientists say the spacecraft needs at least three reaction wheels to be able to point precisely enough to hunt for planets orbiting distant stars.

“We need three wheels in service to give us the pointing precision to enable us to find planets,” said Bill Borucki, Kepler principal investigator, during a press briefing today. “Without three wheels it is unclear whether we could continue to do anything on that order.”

But the Kepler team said there are still possibilities of keeping the spacecraft in working order, or perhaps even finding other opportunities for different science for Kepler, something that doesn’t require such precise pointing abilities.

“We’re not ready to call the mission down and out just yet,” said John Grunsfeld, NASA’s associate administrator for the Science Mission Directorate, “but by any measure it’s been a spectacular mission.”

Last year, NASA had approved an extended mission for Kepler through 2016, and so a lot is riding on the health of the spacecraft’s reaction wheels.

Yesterday, (May 14, 2013) Kepler went into safe mode, a pre-programmed software mode that if the observatory has trouble with pointing, it puts the spacecraft in a state where the solar panels turn towards the Sun to maintain power to its systems, as well as sending an alert to ground controllers. When engineers looked at telemetry, they saw indication that reaction wheel #4 was not moving, even after they commanded it to speed up.

“Initially, they did see some movement on the wheel,”said Charles Sobeck, Kepler deputy project manager during today’s briefing, “but it quickly went back to zero speed, indicative of internal failure on the wheel. Our next step is to see what we can do to reduce the fuel consumption, as we would like to extend the fuel reserve as long as we can.”

Sobeck said they have a few things to try yet to perhaps get wheel #4 working again, such as “jiggling” it or trying the wheel in reverse.

“We can try jiggling it, like you’d do with any wheel here on Earth, commanding it to move back and forth,” said Sobeck, “so we can try to bring the wheel back in service. Or perhaps since wheel #2 hasn’t been turned on for eight months, it may come back if we turn it on. It will take us awhile to come up with a plan.”

Sobeck explained they are currently using thrusters to stabilize the spacecraft, and in its current mode, the onboard fuel will last for several months. But they hope to soon put the spacecraft into what is called a “Point Rest State,” which would extend the fuel to last a period of several years.

“The Point Rest State is a sort of oasis where we can park the vehicle while we decide what we can do next, or see if there’s another mode we can operate the spacecraft in,” Sobeck said “Once we know how we can operate, we can know what the spacecraft can do in the future.”

The Point Rest State is a loosely-pointed, thruster-controlled state that minimizes fuels usage while providing a continuous X-band communication downlink. Sobeck described it as using the solar pressure from the Sun in conjunction with minimum thruster use to allow for a periodic slow back and forth rocking motion of the vehicle which is very fuel efficient but still keeps the solar arrays pointing towards the Sun and communications antennas pointed towards Earth.

The software to execute that state was loaded to the spacecraft last week, and last night the team completed the upload of the parameters the software will use.

Sobeck also said there is the possibility of the wheel running in the opposite direction, but running the wheel backward would mean they would need to use more thruster fuel. “The reaction wheels try to balance the forces from the solar pressure, that’s what forces a wheel to run,” he told Universe Today. “If you’re running the wheel backward, you don’t balance the forces, but add to it, and spacecraft will start to tip, so you will have to offset that with additional thruster firings.”

Reaction wheels have been a problem with several different missions, and Sobeck said NASA does have a team looking at problems of reaction wheels and trying to find ways to maximize their longevity.

Earlier this year, elevated friction was detected in reaction wheel #4, and so as a precaution for wheel safety, and as a measure to mitigate the friction, the reaction wheels were spun down to zero-speed and the spacecraft was placed in a thruster-controlled safe mode for several days. After that, the wheel was able to be used again and it operated until this week.

But the team stressed that even if the Kepler spacecraft is unable to make more observations, there are still terabytes of data to pore over yet from the mission.

“We have two years of data that has yet to be searched through,” said Borucki, “I’m optimistic that the data we have we’ll be able to accomplish Kepler’s mission of finding another Earth. We believe that in the next couple of years we will have many more exciting discoveries with respect to finding planets.”

Boricki added that while he’s delighted that they have found so many planetary candidates, on the other hand “I would have been even happier if it had continued another four years. That would have been frosting on the cake,” he said, “but we have an excellent cake right now.”

Kepler has found over 2,700 planetary candidates, with 130 confirmed planets, from the size of Earth’s moon to larger than Jupiter.

“We’ll continue to analyze the data to get the science that Kepler was designed to do,” said Paul Hertz, NASA’s astrophysics director. “Even though Kepler is in trouble, it has collected all the data necessary to answer its scientific objectives. Kepler is not the last exoplanet mission, but the first. It has been a great start to our path of exoplanet exploration.”

There’s also the chance that something else could be done with the spacecraft if it no longer can do planet hunting, such as asteroid hunting or other astronomical observations…just something that doesn’t need as precise ability for pointing. If that’s the case, Hertz said they would open up a call for science mission proposals.

Additional info here from the Kepler Mission Manager Update

Mars Gets Bombarded by 200 Small Asteroids and Comets Every Year

A relatively new cluster of impact craters on Mars as seen by the HiRISE camera on the Mars Reconnaissance Orbiter. Credit: NASA/JPL-Caltech/MSSS/Univ. of Arizona

One of the benefits of having a spacecraft in orbit around another planet for several years is the ability to make long-term observations and interpretations. The Mars Reconnaissance Orbiter has been orbiting Mars for over seven years now, and by studying before-and-after images from the High Resolution Imaging Science Experiment (HiRISE) camera, scientists have been able to estimate that the Red Planet gets womped by more than 200 small asteroids or bits of comets per year, forming craters at least 3.9 meters (12.8 feet) across.

“It’s exciting to find these new craters right after they form,” said Ingrid Daubar of the University of Arizona, Tucson, lead author of the paper published online this month by the journal Icarus. “It reminds you Mars is an active planet, and we can study processes that are happening today.”

New impact site on Mars formed between November 2005 and October 2010. Credit: NASA/JPL-Caltech/MSSS/Univ. of Arizona
New impact site on Mars formed between November 2005 and October 2010. Credit: NASA/JPL-Caltech/MSSS/Univ. of Arizona

Over the last decade, researchers have identified 248 new impact sites on parts of the Martian surface in the past decade from spacecraft images, determining when the craters appeared. The 200-per-year planetwide estimate is a calculation based on the number found in a systematic survey of a portion of the planet.

The orbiters took pictures of the fresh craters at sites where before-and-after images by other cameras helped figure out when the impacts occurred. This combination provided a new way to make direct measurements of the impact rate on Mars. This will lead to better age estimates of recent features on Mars.

Daubar and co-authors calculated a rate for how frequently new craters at least 3.9 meters in diameter are excavated. The rate is equivalent to an average of one each year on each area of the Martian surface roughly the size of the U.S. state of Texas. Earlier estimates pegged the cratering rate at three to 10 times more craters per year. They were based on studies of craters on the moon and the ages of lunar rocks collected during NASA’s Apollo missions in the late 1960s and early 1970s.

“Mars now has the best-known current rate of cratering in the solar system,” said HiRISE Principal Investigator Alfred McEwen of the University of Arizona, a co-author on the paper.

Examples of craters listed in the paper 'The Current Martian Cratering Rate.' Credit: NASA/JPL/Univ. of Arizona.
Examples of craters listed in the paper ‘The Current Martian Cratering Rate.’ Credit: NASA/JPL/Univ. of Arizona.

These asteroids, or comet fragments, typically are no more than 3 to 6 feet (1 to 2 meters) in diameter. Space rocks too small to reach the ground on Earth cause craters on Mars because the Red Planet has a much thinner atmosphere.

For comparison, the meteor over Chelyabinsk, Russia, in February was about 10 times bigger than the objects that dug the fresh Martian craters.

HiRISE targeted places where dark spots had appeared during the time between images taken by the spacecraft’s Context Camera (CTX) or cameras on other orbiters. The new estimate of cratering rate is based on a portion of the 248 new craters detected. It comes from a systematic check of a dusty fraction of the planet with CTX since late 2006. The impacts disturb the dust, creating noticeable blast zones. In this part of the research, 44 fresh impact sites were identified.

Estimates of the rate at which new craters appear serve as scientists’ best yardstick for estimating the ages of exposed landscape surfaces on Mars and other worlds.

One of many fresh impact craters spotted by the UA-led HiRISE camera, orbiting the Red Planet on board NASA's Mars Reconnaissance Orbiter since 2006. (Photo: NASA/JPL-Caltech/MSSS/UA).
One of many fresh impact craters spotted by the UA-led HiRISE camera, orbiting the Red Planet on board NASA’s Mars Reconnaissance Orbiter since 2006. (Photo: NASA/JPL-Caltech/MSSS/UA).

See the abstract and other information here.
Source: JPL

Timelapse Shows the Blazing Beauty of a ‘Ring of Fire’ Eclipse

Images and videos are still coming in from last week’s spectacular annular eclipse of the Sun, seen across Australia and the southern Pacific region on May 10, 2013. This gorgeous timelapse by Colin Legg captures the eclipse from 3 locations in the Pilbara, Western Australia where the Sun was rising at the time of the event. “If you ever get to see an annular eclipse, I recommend going to the path limits (sunset or sunrise),” Legg said on Vimeo. “All sorts of weird things happen to the Sun, right on the horizon.”

Wow.

See more at our previous gallery of images and video from the eclipse.

Continue reading “Timelapse Shows the Blazing Beauty of a ‘Ring of Fire’ Eclipse”

Astrophoto: Stonehenge, the Milky Way and an Eta Aquarids Meteor

A meteor from the Eta Aquarids flashes over the iconic Stonehenge. Credit and copyright: Peter Greig.

Astrophotographer Peter Greig (St1nkyPete on Flickr) had always wanted to go to Stonehenge in Wiltshire, England, and chose to go there this year for his birthday. It turns out the Universe gave him a little birthday present, with a fabulous clear evening to see the Milky Way shining overhead, along with a few Eta Aquarid meteors flashing in the sky. He captured this amazing shot on May 12. Happy birthday, Peter!

Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

Orion’s Secret Fire Dance

In this image, the submillimetre-wavelength glow of dust clouds in the Orion A nebula is overlaid on a view of the region in the more familiar visible light, from the Digitized Sky Survey 2. The large bright cloud in the upper right of the image is the well-known Orion Nebula, also called Messier 42. Credit: ESO/Digitized Sky Survey 2

The Great Orion Nebula has captivated observers for at least four hundred years, but the ancient Mayans may have known about its secrets long before then. According to legend, the nebula might have been the smoke situated between the “Three Hearthstones” and the light of the emerging stars seen as the very embers of creation itself. Now the ESO-operated Atacama Pathfinder Experiment (APEX) in Chile has revealed what we cannot see. At wavelengths too long for human vision, this new image shows us an ancient fire dance painted in colors of cold interstellar dust.

As we know, deposits of gas and interstellar dust are virtual star factories. However, the very material which creates stars also masks them. So how do we peer behind the veil? The answer is to observe at alternative wavelengths of light. In this case, the submillimetre wavelength reveals what our eyes cannot see… dust grains igniting the view, even though they are just a few tens of degrees above absolute zero. This makes the APEX telescope with its submillimetre-wavelength camera LABOCA, located at an altitude of 5000 metres above sea level on the Chajnantor Plateau in the Chilean Andes, the perfect instrument to play the tune for this cold fire dance.

Take a look around the picture. It’s just a small portion of a vast complex known as the Orion Molecular Cloud. Wafting across hundreds of light years space some 1350 light years away, this rich arena of hot young stars, cold dust clouds and bright nebula is the epitome of stellar creation. The image reveals the submillimetre-wavelength glow in shades of orange and it is combined with visible light for a total visual experience. Note deep ribbons, sheets and bubbles… These are the product of gravitational collapse and the effects of stellar winds. Powerful stellar processes are at work here. The atmospheres of the stars are crafting the clouds much the same way a gentle breeze swirls the smoke from a fire.

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Credit: ESO/Nick Risinger (skysurvey.org), Digitized Sky Survey 2. Music: movetwo

As beautiful as it is, there is still science behind the imagery. Astronomers have employed the data taken with ESA’s Herschel Space Observatory, along with the APEX information, to aid them in their search for early star formation. At this point in time, the researchers have been able to verify more than a dozen candidate protostars – objects which appear far brighter at longer wavelengths rather than short. It’s a triumph for the researchers. These new observations could well be the youngest protostars so far observed and it brings astronomers just one step closer to witnessing the moment when a star ignites.

Original Story Source: ESO News Release.

Chris Hadfield’s 5-month Space Mission in 90 Seconds

Expedition 35 Commander Chris Hadfield of the Canadian Space Agency (CSA), left, Russian Flight Engineer Roman Romanenko of the Russian Federal Space Agency (Roscosmos), center, and NASA Flight Engineer Tom Marshburn sit in chairs outside the Soyuz Capsule just minutes after they landed in a remote area outside the town of Dzhezkazgan, Kazakhstan, on Tuesday, May 14, 2013. Hadfield, Romanenko and Marshburn are returning from five months onboard the International Space Station where they served as members of the Expedition 34 and 35 crews. Photo Credit: (NASA/Carla Cioffi)

Already missing him being in space? I’ve seen several tweets about people going through Hadfield withdrawal. But to tide you over until he starts tweeting again (just give him a little time to get his Earth-legs again) here’s a mashup/supercut of Chris Hadfield’s video and image highlights from his five-month stay on the International Space Station.

How to Plant a Garden on Mars — With a Robot

Sketch of the ‘AstroGardening’ robot within its Mars garden Credit: Vanessa Harden.

Editor’s note: This guest post is written by Louisa Preston, an Astrobiologist and Planetary Geologist. She is a TED Fellow, and Postdoctoral Research Associate at The Open University, UK.

In the last century humanity has taken gigantic leaps forward in the robotic exploration of the cosmos — not least in the search for habitable worlds and environments that could house life outside of the Earth. The next logical step is for humanity itself to leave the confines of our planet, and take on long-term human exploration of the Solar System. Mars in particular is a key target for future human planetary adventures even though on the face of it, it seems so hostile to human life. In fact Mars actually has the most clement environment of any planet in the Solar System outside of Earth and is known to have all of the resources necessary in some accessible form, to sustain life on the surface. So how might we survive on Mars? The crucial things for humans on Mars are the availability of oxygen, shelter, food and water, and not just endless consumables delivered to the planet from Earth. For humans to live long-term on Mars, they will need a self-sustaining habitat to be able to thrive in for generations.

In short, they’ll need a garden. And maybe a robot, too.

Any garden on Mars would need protection in the form of a greenhouse or geodesic dome that could keep the vegetables, fruits, grains and flowers sheltered from the extreme UV radiation that floods the Martian surface, whilst still allowing enough sunlight through to allow them to grow. This dome would also have to be strong enough to provide support and protection against potentially devastating Martian dust storms.

The crops would need to be kept warm, as outside the dome it will be on average a freezing -63 °C. Solar panels arranged outside the habitat and heating filaments underneath it could provide the desired warmth.

garden on mars

Liquid water is needed for irrigation of the plants and for future human consumption, but with water on Mars mainly frozen beneath the surface, we would need to mine the ice and melt it. The atmosphere on Mars is chiefly composed of CO2, which humans cannot use for any of our vital functions. However plants can! They can utilise this atmospheric CO2 to photosynthesise, which would actually create the oxygen we would need.

These are all important aspects of long-term human habitation of Mars that need to be tested and perfected before we arrive, but thankfully most of these can be investigated whilst safely here on the Earth in Mars analogue environments and specially designed spaces.

Our premise is that of a pioneer AstroGardening robot, designed and built by ourselves, to be sent to Mars to set up garden habitats in advance of the first human inhabitants. It will scatter ‘seed pills’ containing various seeds, clay and nutrients across the habitat and nurture the growing plants.

But before we actually go to Mars, we are working on an interactive ‘Mars Garden’ exhibit and AstroGardening Rover designed to educate and inspire.

Installation designer Vanessa Harden and I are building such a space; an interactive experience designed for museums and science centers to entertain and educate on the perils and benefits of gardening on Mars, the ways in which we need to design tools to do this, the plants that would best grow in Mars soil and the methods we might use to obtain liquid water.

Visitors to this Mars concept habitat will get to meet the AstroGardening robot himself and walk around a lush and tranquil Martian garden. They will also get to see the range of food stuffs that we can actually grow in the Martian soil such as asparagus, potatoes, sweet potatoes, radish, alfalfa, and mung bean.

Our aim for this exhibit is to communicate the science behind future human habitation of Mars, the effect we as humans can have on an environment, and the ethics and logistics of colonising other planets.

The exhibit has already been invited to tour around some of London’s most celebrated and beautiful venues such as observatories and planetariums, museums and art galleries, schools and universities, before heading across the ocean to the US and Canada.

But we need the public’s help to make this tour and exhibit a reality.

We have a Kickstarter page for this concept to raise the funds to begin building our vision. See our page and watch our video (below) to find out how you can help.

AstroGardening – Designing for Life on Mars from vanessa harden on Vimeo.