Posted on by Nancy Atkinson

Enticing Trailer for New Movie about a Mission to Europa

Here’s a trailer from a new movie called “Europa Report” about a near-future mission to Jupiter’s moon, Europa, in search of extraterrestrial life. From the trailer, the film looks to be of extremely high quality, and it stars Sharlto Copley (District 9), with music score from composer Bear McCreary (Battlestar Galactica).

And while this is a sci-fi flick, the makers of “Europa Report” say they are trying to steep it in real science.

The PR for the film is just getting underway, but they have a realistic-looking website that appears to show webcam views from a spacecraft heading to Europa.

Screenshot:

Here’s the blurb from the website:

For decades, scientists have theorized the existence of liquid water oceans on Jupiter’s moon, Europa. We’ve recently discovered new, captivating evidence that these sub-surface oceans do exist and could support life.

We’ve sent six astronauts from space programs throughout the world on a three year journey to Europa to explore its oceans and confirm these findings.

We’re proud to be at the forefront of the effort to prove the existence of extra-terrestrial life within our solar system, within our lifetimes.

And yep, like any film about spaceflight, something has to go wrong during the mission.

The release date for the film has not yet been set.

Posted on by Elizabeth Howell

Google Honors Canadarm’s 31st Anniversary

Canada’s most famous robot is on the front page of Google.ca today. The Google doodle honors the 31st anniversary of the first use of Canadarm in space.

Canadarm is a robotic arm that flew on virtually every shuttle mission. The technology is still being used today in space.

According to the 1992 book A Heritage of Excellence, Canada was first invited to work in the shuttle program in 1969. Toronto engineering firm DSMA-Atcon Ltd. initially pitched a Canadian-built space telescope, but NASA was more interested in DSMA’s other work.

“The Goddard Space Flight Center in Maryland expressed interest in another of DSMA’s gadgets – a robot the company had developed for loading fuel into Candu nuclear reactors,” wrote Lydia Dotto in the book, which Spar commissioned to celebrate its 25th anniversary.

“It was just the thing for putting a satellite they were building into space.”

Dozens of astronauts have used the Canadarms during spacewalks, including Michael L. Gernhardt on STS-104. Credit: NASA

The Canadian government and NASA signed a memorandum of understanding in 1975 to build the arm. Legislation allowing the project to move forward passed the next year. Canadian company Spar became the prime contractor, with DSMA, CAE and RCA as subcontractors.

Engineers had to face several challenges when constructing the Canadarm, including how to grapple satellites. The solution was an “end effector“, a snare on the end of the Canadarm to grasp satellites designed to be hoisted into space.

Several NASA astronauts, including Sally Ride, gave feedback on the arm’s development. Canadarm flew for the first time on STS-2, which launched Nov. 12, 1981. (Ride herself used the arm on STS-7 when she became the first American woman to fly in space.)

Marc Garneau, the first Canadian astronaut in space, has said the arm’s success led to the establishment of the Canadian astronaut program. He flew in 1984, three years after Canadarm’s first flight.

Canadian astronaut Chris Hadfield during an EVA in 2001. Also in the image is the Canadarm2 robotic arm on the ISS. Credit: NASA

Some of the arm’s notable achievements:

– Launching space probes, including the Compton Gamma Ray Observatory, as well as short-term experiments that ran during shuttle missions;

– Retrieving satellites for servicing. One prominent example was the rescue of the INTELSAT VI satellite on STS-49, which required the first three-astronaut spacewalk;

– Launching the Hubble Space Telescope, then retrieving and relaunching it during each repair mission;

– Helping to build the International Space Station along with Canadarm2, its younger sibling;

– Scanning for broken tiles on the bottom of the shuttle. Astronauts used a procedure developed after Columbia, carrying seven astronauts, was destroyed during re-entry in 2003. A Canadarm was modified into an extension boom; another Canadarm grasped that boom to reach underneath the shuttle.

The arm was so successful that MacDonald, Dettwiler and Associates (which acquired Spar) built a robotic arm for the International Space Station, called Canadarm2. Canadian astronaut Chris Hadfield helped install the arm during his first spacewalk in 2001.

Canadarm2’s most nail-biting moment was in 2007, when astronauts used it to hoist astronaut Steve Parazynski (who was balancing on the extension boom) for a tricky solar panel repair on the station.

November 3, 2007 – Canadarm2 played a big role in helping astronauts fix a torn solar array. Here, Scott Parazynski analyses the solar panel while anchored to the boom. Credit: NASA

More recently, Canadarm2 was used to grapple the Dragon spacecraft when SpaceX’s demonstration and resupply missions arrived at the International Space Station this year.

MDA recently unveiled several next-generation Canadarm prototypes that could, in part, be used to refuel satellites. The Canadian Space Agency funded the projects with $53 million (CDN $53.1 million) in stimulus money. MDA hopes to attract more money to get the arms ready for space.

You can read more about the Canadarm’s history on the Canadian Space Agency website.

Posted on by Nancy Atkinson

New Bright and Blue Supernova in NGC 1365

Supernova 2012fr in NGC 1365. It is the bright blue “star” directly below the galaxy core. Credit: Rolf Wahl Olsen. Click the image for larger version.

A very bright supernova has shown up in NGC 1365, the galaxy also known as the Great Barred Spiral Galaxy, visible now for southern hemisphere observers. This already elegant galaxy lies about 56 million light-years away in the constellation Fornax. The supernova, a type Ia, was discovered by Alain Klotz with the TAROT telescope at the La Silla Observatory in Chile on October 27, 2012. “The supernova is a very nice addition to the already highly photogenic galaxy,” said Rolf Wahl Olsen, who took the gorgeous image above. “I’m amazed by how blue it is; it’s really intense.”

Supernova 2012fr is the bright and intensely blue star directly below the galaxy core. Olsen said that as of November 10, 2012 the supernova appeared to be nearing its peak, with an R magnitude of 11.90.

“To get an idea of how bright this event is we can calculate the absolute magnitude M of the supernova using the following formula where m is the apparent magnitude and D the distance in parsecs: M = m – 5(log10(D) – 1),” Olsen wrote. “This gives an absolute magnitude of -19.27 for SN2012fr. This means that if the supernova had occurred at a distance to us similar to Betelgeuse (643 light years), then its apparent magnitude would be -12.80, same as the full Moon!”

Details about Olsen’s image:
Date: 7th and 9th November 2012
Exposure: LRGB: 205:57:56:51m, total 6hrs 9mins @ -30C
Telescope: 10″ Serrurier Truss Newtonian f/5
Camera: QSI 683wsg with Lodestar guider
Filters: Astrodon LRGB E-Series Gen 2
Taken from his observatory in Auckland, New Zealand

See more of Olsen’s astrophotography at his Flickr page.

Posted on by Jenny Winder

Spaceflight: Taking it Lying Down

Caption: Bedrest volunteer in bed during a study conducted in 2005. Credit: ESA

As you get older, do feel you could do with more rest? Our bodies lose bone density and muscle strength as we age. Astronauts in space suffer similar changes but at a much faster rate. Finding ways to understand and combat this process is important to space agencies, hospital patients and all of us as we grow older. A new study is about to commence at the French Institute for Space Medicine and Physiology, in the clinical research facility in Toulouse, France, that hopes to understand and address changes in astronauts’ bodies in space as well as in bedridden people on Earth. 12 volunteers will spend 21 days in bed. Sound relaxing? Think again.

The volunteers taking part in the study, will lie for 24 hours a day with their heads tilted 6° below the horizontal. They will not be allowed to get up, for any reason. Not for a breath of fresh air, a change of scenery, a shower or to use the toilet, until the 21 days are over. This will cause their bodies to react in similar ways to being weightless, without the expense or  risks involved in sending them into space.

In microgravity, bone loss occurs at a rate of 1 to 1.5% a month. This bone demineralization increases the risks of kidney stones and bone fractures as well as altering the ability of bones to heal after fractures. Loss of muscle mass, strength and endurance, increases risk of fatigue and injury. The heart may experience diminished cardiac function and possible disturbances in heart rhythm.

Microgravity also causes body fluids to be redistributed away from the extremities, which results in puffiness in the face during flight. The body’s neurovestibular system that controls balance, stabilizes vision and body orientation in terms of location and direction may also become impaired, leading to disorientation and lack of coordination. The body can also suffer loss of blood volume, low red blood cell levels and immunodeficiency

Although many of the effects are reversible upon return to Earth, astronauts may have problems standing up, stabilizing their gaze, walking and turning, immediately after landing. Some astronauts find their blood pressure drops abnormally low when they move from lying down to a sitting or standing position.

The participants in this latest study will be scientifically scrutinised to see how they adapt to staying in bed for long periods, but they will also be divided into three groups to test a set of measures designed to counteract muscle and bone loss. The control group will be given no countermeasures, while a second group will use resistive and vibrating exercise machines. The last group will use the exercise machines and eat nutritional supplements of whey protein – a common supplement used by bodybuilders to train their muscles.

Each group of volunteers will participate in all the regimes, one after the other, over the course of the entire experiment of more than a year. They will be given four months between each bedrest session to recuperate. After the first 21-day session, they will return to the at the MEDES Space Clinic in Toulouse, for another session and once more in 2013 for a final session. After all that I bet they will need a rest.

Read more about this study here
And read diaries from participants in a similar study that ran for 60 days in 2005 here

Posted on by Nancy Atkinson

The Total Solar Eclipse Down Under: How to Watch it from Anywhere in the World

Scientists and interested skywatchers have been flocking to Cairns, Australia to witness one of the most spellbinding astronomical sights: a total solar eclipse. The November 13/14 total solar eclipse will only be visible in its entirety to ground-based observers watching from northern Australia, but several webcasts will be available so that people around the world can watch as well. At about 22:11:48 UT on November 13 (it will be the morning of Nov. 14th in Australia) the Moon will pass directly in front of the Sun, and totality will only last about 2 minutes, with the Sun having risen just 14 degrees above the eastern horizon. The total time of the event, from first contact to fourth contact (the end of a solar eclipse when the disk of the Moon completely passes from the disk of the Sun) will be about 3 hours.

During totality the Sun appears to have a white halo – a rare glimpse of the Sun’s million-degree plasma atmosphere, or corona, which is too washed out by the Sun’s brightness to be observed normally.

During an eclipse, “the Moon reveals the innermost corona, which manmade coronagraphs have trouble seeing,” said Shadia Habbal of the Institute for Astronomy in Hawaii, who will be in Australia for the event. “That is where all the magnetic field and physical processes responsible for heating the corona are evolving most rapidly.”

For this total solar eclipse, the path of totality will be about 174 km (108 miles) wide and will cover 14,500 km (9,000 miles) over a 3-hour period.

Below is a list of webcasts for those not in Australia, but an important note if you ARE going to be in an area where you can see the eclipse: DO NOT look directly at the Sun, and especially do not look through a telescope or binoculars at the Sun with your eyes directly. Doing so could cause serious and permanent eye damage. There are special eclipse glasses, or you can make your own eclipse viewers. Mr. Eclipse has a whole list with instructions for pinhole cameras, and other safe viewing methods. If you have a telescope, the folks from Galileoscope have instructions for how to build a Sun-funnel for safe viewing.

Proba-2 image of the solar disc taken during the total eclipse of July 2010, combined with ground-based images taken at the same time to reveal the exquisite details of the solar corona. Credit: ESA

Slooh will be having their webcast at Slooh.com, starting Tuesday, November 13th at 11:30 AM PST / 2:30 PM EST / 19:30 UTC. Viewers can watch the show on their PC or mobile device and will have the ability to ask questions to the Slooh team, including the crew located in Cairns, using the Slooh Conversations section on the Slooh homepage. Viewers will also be able to snap the live pictures directly from the Slooh homepage using Pinterest. The broadcast team includes Patrick Paolucci, Bob Berman, Lucie Green, Matt Francis and Paul Cox.

Another feed will be from the Cairns Eclipse 2012 Ustream channel, broadcast from over Cairns and the Great Barrier Reef, Australia: http://www.ustream.tv/CairnsEclipse2012, and their website is http://www.eclipse2012.org.au

This channel will be live from 11 a.m. PT (2 p.m. ET) on Nov. 13, and 5 am November 14th 2012 (AEST). It is considered the official destination website for the total solar Eclipse over Cairns and Great Barrier Reef will feature Terry Cuttle from the Astronomical Association of Queensland as the host. He will be joined by Kate Russo (eclipse chaser and author), Ben Southall (winner of the ‘Best Job in the World’ promotion and tourism ambassador), Richard Fitzpatrick (an underwater cameraman, will be live from under water) and Alan Hale (from Hale-Bopp comet who is studying comets close to the Sun which can only be seen during an eclipse).

Still another feed will be the Panasonic channel: Broadcast from Sheraton Mirage Port Douglas Resort:
http://www.ustream.tv/channel/panasonic-eclipse-live-by-solar-power-1

Panasonic’s project, described as, “Filming the Sun, using the Sun” aims to capture and broadcast to the world a solar eclipse using only the power of sunlight. They’re using Panasonic’s high efficiency solar power-generating system, “HIT” to generate power with a portable battery back for power storage. They’ll then be able to broadcast the eclipse images captured on a Lumix GH2.

2012 Eclipse live from a Cairns Hot Air Balloon
http://www.hotair.com.au
Up to a dozen hot air balloons floating west of Cairns, Queensland Australia, with visitors from 20 different countries will be part of a live webcast of the 2012 total solar eclipse.

Cairns City Eclipse 2012 webcam
http://www.eclipsecairns.com
Can’t make it to Cairns to see the Eclipse? No problem! Just check back on November 14 before 6:39am AEST (GMT+10) to see it live on their webcam.

GLORIA Project
http://live.gloria-project.eu
Videos and pictures of the eclipse will be broadcast live on the internet starting at 20:30 UT. Additionally meteorological data will be collected to allow students to perform an interactive experiment. During the broadcast there will be live commentary in Spanish and English.

Live Web Camera from Port Douglas Australia 2012
http://www.zincportdouglas.com/solar_eclipse_port_douglas.html

We’ll be embedding a few of the feeds when they go live.

Find out more about the eclipse here.

Posted on by Nancy Atkinson

Astrophoto: Deep Sky Treasury

The view of the Paranal Observatory: Credit: ESO/Babak Tafreshi

A new image captures the stunning view of the night sky over ESO’s Paranal Observatory, with a treasury of deep-sky objects. The image was taken by Babak Tafreshi, an astronomer, journalist and director of The World at Night (TWAN).

It shows the Carina Nebula, glowing intensely red in the middle of the image. Below Carina is the the Wishing Well Cluster (NGC 3532); then to the right is the Lambda Centauri Nebula (IC 2944) – which is also called the Running Chicken Nebula. Above this nebula and slightly to the left is the Southern Pleiades (IC 2632), an open cluster of stars that is similar to its more familiar northern namesake.

In the foreground, is three of the four Auxiliary Telescopes (ATs) of the Very Large Telescope Interferometer (VLTI).

See more information about this image from ESO.

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.

Posted on by John Williams

A Primer on Cosmic Sprinklers

The planetary nebula Fleming 1, as seen with ESO’s Very Large Telescope. Credit: ESO/H. Boffin

The neat thing about planetary nebulae is that they are like snowflakes: no two are quite the same. Some look like pools of hot water, some look like glowing eyes in the night and others, like this image of Fleming 1, have twin jets of material spiraling outward from the center resembling a huge cosmic sprinkler.

And for the first time, astronomers with the European Southern Observatory have paired new Very Large Telescope images of Fleming 1 with computer models to explain how the intricate dance between two dead stars result in these bizarre nebulae that appear to be flinging material out into space. The team’s findings were published in the November 9, 2012 issue of the journal Science.

“The origin of the beautiful and intricate shapes of Fleming 1 and similar objects has been controversial for many decades,” says team leader Henri Boffin in a press release. “Astronomers have suggested a binary star before, but it was always thought that in this case the pair would be well separated, with an orbital period of tens of years or longer. Thanks to our models and observations, which let us examine this unusual system in great detail and peer right into the heart of the nebula, we found the pair to be several thousand times closer.”

The team using ESO’s VLT to study Fleming 1’s central star, toward the constellation Centaurus, found not one but two white dwarfs at its core. The two white-hot dead stars slightly smaller than our Sun circle each other every 1.2 days. Binary stars have been found at the heart of planetary nebulae before, but two white dwarfs circling each other is very rare, say the scientists.

Planetary nebulae have nothing to do with planets. Astronomers in the eighteenth century likened these glowing bubbles of light to planets because they resembled the distant orbs Uranus and Neptune in their small telescopes. Planetary nebulae are actually a brief stage at the end of a sun-like star’s life. As a star with a mass up to eight times that of our Sun nears the end of its life, it sloughs off its outer shells in an immense bubble. As more and more mass is lost to space, the white-hot stellar core is exposed. This white dwarf gives off a stiff solar wind that pushes the bubble ever wider. Blistering ultraviolet radiation from the dead star excites atoms in the expanding cloud causing it to glow.

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This animation shows how the two stars at the heart of a planetary nebula like Fleming 1 can control the creation of the spectacular jets of material ejected from the object. Credit:ESO/L. Calçada. Music: delmo “acoustic”

Gazing into a planetary nebulae rarely reveals a quiet environment. Complex knots and filaments form intricate patterns. For cosmic sprinklers like Fleming 1 material seems to be shooting from both poles with an S-shaped pattern between the star and the outermost wavefront. Scientists say that as the stars aged, they expanded and one sucked material from its companion; a kind of starry vampire, forming a spinning disk of material. As they rapidly orbited each other, the pair began to wobble like a spinning top, a type of motion called precession. The team’s study shows that precessing accretion disks within binary star systems form the symmetrical arcs of material in planetary nebulae like Fleming 1.

The VLT images revealed even more surprises about Fleming 1, named after Scottish astronomer Williamina Fleming in 1910. Scientists found a knotted ring of material within the inner nebula of Fleming 1. Scientists look for these rings as a sign of a binary system.

Source: European Southern Observatory

Posted on by Jason Major

Here There Be Planets: Stellar Disk Gap May Reveal Newborn Worlds

HiCIAO near-infrared image of the protoplanetary disk around PDS 70. The circular mask hides the star itself, as well as a smaller internal disk structure. (Credit: NAOJ)

Over the past couple of decades astronomers have figured out several methods for finding planets around other stars in our galaxy. Some have revealed their presence by the slight “wobble” they impart to their host stars as they orbit, while others have been discovered as they pass in front of their stars from our perspective, briefly dimming the light we see.

Now, some astronomers think they may have identified the presence of multiple planets, based on a large gap found in the disk of  gas and dust surrounding a Sun-like star 460 light-years from Earth.

Using the High Contrast Instrument for the Subaru Next Generation Adaptive Optics (HiCIAO) mounted on Japan’s 8.2-meter optical-infrared Subaru telescope atop Mauna Kea in Hawaii, an international team of astronomers targeted PDS 70, a young star (10 million years old) about the same mass as the Sun located 460 light-years away in the constellation Centaurus.

The near-infrared observations made by HiCIAO reveal a protoplanetary disk surrounding PDS 70. This disk is composed of gas and dust and extends billions of miles out from the star. Quite literally the stuff that planets are made of, it’s a disk much like this that our solar system likely started out as over 4.6 billion years ago.

“Thanks to the powerful combination of the Subaru Telescope and HiCIAO, we are able to probe the disks around Sun-like stars. PDS 70 shows how our solar system may have looked in its infancy. I want to continue this kind of research to understand the history of planetary formation.”

– Team Leader Jun Hashimoto (NAOJ)

Within PDS 70’s disk are several large gaps positioned at varying distances from the star itself, appearing as dark regions in the near-infrared data. These gaps — especially the largest, located about 70 AU from the star — are thought to be the result of newly-formed planets having cleared the surrounding space of dust and smaller material. It’s also believed that multiple planets may be present since, according to the team, “no single planet, regardless of how heavy or efficient it is in its formation, is sufficient to create such a giant gap.”

In addition to the large disk structure and outer gap, PDS 70 also has a smaller disk located only 1 AU away. (This disk is obscured by the HiCIAO mask in the image above.)

Further observations will be needed to locate any actual exoplanets directly, since the light from the star and scattered light within the disk makes it difficult — if not impossible with current technology — to detect the incredibly faint light reflected by planets.

Still, it’s fascinating to come across what may very well be a solar system in its infancy, giving us a glimpse back in time to our own formation.

“Direct imaging of planets in the process of forming in protoplanetary disks would be ideal so that we can learn when, where, and how planets form,” said team leader Ruobing Dong of Princeton University.

Read more on the NAOJ website for the Subaru Observatory here.

The goal of the Strategic Exploration of Exoplanets and Disks with Subaru (SEEDS) Project is to study the disks around less massive stars like the Sun.

Inset image: Artist’s rendition of PDS 70 and its two protoplanetary disks (NAOJ)

Posted on by John Williams

Swirling Vortex and Mini Moons: Spectacular Views of the Little Things Around Saturn

High-altitude clouds in Titan’s seasonal south polar swirl glow dimly in this image from NASA’s Cassini spacecraft.

With wild storms and a vast ring system, nothing seems small around Saturn. But as NASA’s Cassini spacecraft loops high over Saturn’s poles, scientists are taking time to explore the little things including a swirling vortex, the miniature moon Mimas, and another tiny ovoid moon named Methone.

Titan’s swirling vortex, lower right, glows brightly against the south polar clouds in this new image from NASA’s Cassini spacecraft. Scientists are monitoring the development of the swirling mass of gas to try and understand the weather related to the coming winter to the moon’s south pole. For a color closeup of the vortex, see Titan’s Colorful South Polar Vortex. If you’re more into a moving visualization, check out the vortex in motion.


Cassini acquired the view of the vortex on Titan on August 31, 2012 using a special filter sensitive to light in the near-infrared. Cassini took this image from a distance of about 1.2 million kilometers (750,000 miles) above the south pole of Titan. That’s nearly three times the distance between Earth and the Moon. The smallest detail on this image is about 4 miles across.

“Note the motions and beautifully detailed cloud patterns,” wrote Carolyn Porco, Cassini imaging team lead on the CICLOPS website, “very likely the result of open-cell convection — already visible in this fascinating phenomenon that we on Cassini have been fortunate to capture, for the first time, in the process of being born.”

Methone looks like a tiny gray egg in this image from NASA’s Cassini spacecraft.

Last week, the Cassini imaging team released two stunning images of Saturn. Tiny, egg-shaped Methone (pronounced meh-tho-nee) is barely 3 kilometers (2 miles) across. Cassini discovered this moon in 2004 hanging out between Mimas and Enceladus at just 194,000 km (120,000 miles) above Saturn. From Methone’s smooth surface, Saturn must be a true wonder. Small moons like Methone are generally non-round. Scientists believe they just don’t have the mass to pull themselves together into a round shape. The leading side of Methone is lit in this image and at a distance of just 4,000 km (2,500 miles) the smallest feature that can be seen is about 27 meters (88 feet).

Saturn’s moon Mimas is dwarfed by Saturn and its rings in this spectacular image from NASA’s Cassini spacecraft

Don’t blink or you might miss a tiny dot just to the upper left of Saturn. Mimas is dwarfed not only by Saturn’s rings, but also by the gigantic storms visible in the northern and southern hemisphere’s Mimas is just 396 km (246 miles) across and is the solar system’s 20th largest satellite. The moon could easily fit within the borders of Spain and most western states in the U.S. Cassini took this spectacular image from a distance of 2.4 million kilometers (1.5 million miles) from Saturn.

Source: NASA Jet Propulsion Laboratory and Cassini Imaging Central Laboratory for Operations (CICLOPS)

Posted on by Nancy Atkinson

Curiosity Rover Update: Sniffing Mars’ Atmosphere

What has Curiosity been up to lately? The rover’s Sample Analysis at Mars (SAM) instruments makes up more than half the science payload on board MSL, and it is now searching for compounds of the element carbon — including the enticing methane that has been observed in Mars’ atmosphere from telescopes and instruments on Earth. These are the elements that are associated with life, and SAM is trying to determine if methane can be detected from the surface, as well. So far, the rover has not found “definitive evidence” beyond data uncertainty of methane in Mars’ thin atmosphere. But that doesn’t close the door on the subject. It is still early in the mission, and the methane on Mars has been cyclical in nature.

“A search for methane was made on multiple nighttime runs, but so far we have no definitive detection of methane,” said Chris Webster, the team lead for MSL’s Tunable Laser Spectrometer. The instrument has detected values of no methane at all up to 5 parts per billion, but the “data uncertainty is larger than this,” Webster said. “We do plan on additional runs, of course, to look for variability.”

But, of course, methane has been detected in certain areas, not necessarily planet-wide.

The Sample Analysis at Mars (SAM) instrument, at NASA’s Goddard Space Flight Center, Greenbelt, Md., will analyze samples of material collected by the rover’s arm. Credit: NASA/JPL

“In the Gale Crater, at the moment, we don’t have a definite detection of methane,” said Sushil Atreya, a co-investigator with the SAM instruments. “On the other hand, the source doesn’t have to be at Gale Crater. If there is a source of methane elsewhere, it does not take very long for it to get distributed all over the planet. It takes on the order of about three months. That is all we can say at this point.”

Methane is enticing because it could indicate life of some sort, perhaps microbial life. But methane can also be produced by certain geologic processes, and recently, a team of researchers suggested that methane could even be produced by Martian dust devils.

But as Pan Conrad, deputy principal investigator for SAM says in the video above, the team will continue to explore ways in which methane could be generated and then destroyed in the Martian ecosphere, and make the most of these extremely sensitive instruments that are now on Mars.

“SAM will continue to sniff the Martian atmosphere and look for changes over time,” Conrad said. “That will tell us something about the dynamics between the exchange between the surface and the atmosphere.”