Image Caption: Scooping Mars at ‘Rocknest’ mosaic shows a before and after view of the spot where Curiosity dug up her 1st Martian soil sample on Sol 61 (Oct 7. 2012). Navcam camera mosaic at left shows the arm at work during scooping operations. Image at right shows the tiny scooped trench measuring about 1.8 inches (4.5 centimeters) wide. See NASA JPL scooped sample vibration video below. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
“Here’s the scoop: I like my regolith shaken!” tweeted NASA’s Curiosity Mars rover a short while ago in a nod to the 50th anniversary of the premiere of the 1st James Bond action flick.
And the “proof” is in the video as they say. See below a short NASA video clip showing the 1st Martian material collected using the small table spoon sized scoop on Curiosity’s robotic arm and subsequently being vibrated inside the scoop after it was lifted from the ground of Gale Crater this past weekend on Sol 61, Oct. 7, 2012.
Scooping Mars at ‘Rocknest’ mosaic above shows a before and after view of the spot where Curiosity was working at on Sol 61.
“So excited to dig in! One scoop of regolith ripple, coming right up!” she tweeted in the midst of the action.
Video Caption: This 256 frame video clip of Mastcam images shows the 1st sample of Martian material being vibrated inside Curiosity’s table spoon sized scoop on Oct. 7, 2012. Credit: NASA/JPL-Caltech/MSSS
Yeah baby ! Just as the rover’s science and engineers announced last week, the 6 wheeled mega robot Curiosity scored a major success by scooping up her very first sample of windblown Martian sand from the ‘Rocknest’ ripple she arrived at just last week.
The plan ahead is to use the collected “Red Planet” material to cleanse the interior of the rover’s sample-handling system of a residual layer of oily contamination of “Home Planet” material that could interfere with unambiguously interpreting the results.
For sure the science team doesn’t want any false positives with respect to any potential detection of the long sought organic compounds that could shed light on whether a habitant supporting Martian microbes ever existed in the past or present.
The newly collected material will be vibrated at 8 G’s and then be fed into Curiosity’s Collection and Handling for In-Situ Martian Rock Analysis (CHIMRA) device on the robotic arm turret.
Curiosity’s motorized scoop measures 1.8 inches (4.5 centimeters) wide, 2.8 inches (7 centimeters) long. The images reveal the scoop left behind a small hole about 1.8 inches (4.5 centimeters) wide.
Image Caption: Sol 61 Navcam raw image shows the hole dug up by Curioisty’s scoop on Oct. 7, 2012 Credit: NASA/JPL-Caltech
Image Caption: Mastcam 100 telephoto close up image of Rocknest trench on Sol 61. Credit: NASA/JPL-Caltech/MSSS
At last week’s Oct. 4 media briefing, the rover team said they would make three deliveries of scooped soil to cleanse out the sample acquisition system over the next two week or so before pouring sieved Mars material into the SAM and Chemin analytical chemistry labs on the rover’s deck for detailed evaluation of the elemental and mineralogical composition.
Image caption: Context view of Curiosity working at ‘Rocknest’ Ripple. Curiosity’s maneuvers robotic arm for close- up examination of ‘Rocknest’ ripple site and inspects sandy material at “bootlike” wheel scuff mark with the APXS (Alpha Particle X-Ray Spectrometer) and MAHLI (Mars Hand Lens Imager) instruments positioned on the rotatable turret at the arm’s terminus. Mosaic was stitched together from Sol 57 & 58 Navcam raw images and shows the arm extended to fine grained sand ripple in context with the surrounding terrain and eroded rim of Gale Crater rim on the horizon. Rocknest patch measures about 8 feet by 16 feet (2.5 meters by 5 meters).See NASA JPL test scooping video below. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
NASA’s Curiosity rover is set to scoop up her 1st sample of Martian soil this weekend at a soil patch nicknamed ‘Rocknest’ -see our context mosaic above – and will funtion as a sort of circulatory system cleanser for all the critical samples to follow. This marks a major milestone on the path to delivering Mars material to the sample acquisition and processing system for high powered analysis by the robots chemistry labs and looking for the ingredients of life, said the science and engineering team leading the mission at a media briefing on Thursday, Oct 4.
Since landing on the Red Planet two months ago on Aug. 5/6, Curiosity has trekked over 500 yards eastwards across Gale crater towards an intriguing area named “Glenelg” where three different types of geologic terrain intersect.
This week on Oct. 2 (Sol 56), the rover finally found a wind driven patch of dunes at ‘Rocknest’ with exactly the type of fine grained sand that the team was looking for and that’s best suited as the first soil to scoop and injest into the sample acquisition system.
See NASA JPL earthly test scooping video below to visualize how it works:
“We now have reached an important phase that will get the first solid samples into the analytical instruments in about two weeks,” said Mission Manager Michael Watkins of NASA’s Jet Propulsion Laboratory in Pasadena, Calif.
The rover used its wheels to purposely scuff the sand and expose fresh soil – and it sure looked like the first human “bootprint” left on the Moon by Apollo 11 astronauts Neil Armstrong and Buzz Aldrin.
Curiosity will remain at the “Rocknest” location for the next two to three weeks as the team fully tests and cleans the walls of most of the sample collection, handling and analysis hardware – except for the drilling equipment – specifically to remove residual contaminants from Earth.
Image caption: ‘Rocknest’ From Sol 52 Location on Sept. 28, 2012, four sols before the rover arrived at Rocknest. The Rocknest patch is about 8 feet by 16 feet (1.5 meters by 5 meters). Credit: NASA/JPL-Caltech/MSSS
The purpose of this initial scoop is to use the sandy material to thoroughly clean out, rinse and scrub all the plumbing pipes, chambers, labyrinths and interfaces housed inside the complex CHIMRA sampling system and the SAM and CheMin chemistry labs of an accumulation of a very thin and fine oily layer that could cause spurious, interfering readings when the truly important samples of Martian soil and rocks are collected for analysis starting in the near future.
The scientists especially do not want any false signals of organic compounds or other inorganic materials and minerals stemming from Earthly contamination while the rover and its instruments were assembled together and processed for launch.
“Even though we make this hardware super squeaky clean when it’s delivered and assembled at the Jet Propulsion Laboratory, by virtue of its just being on Earth you get a kind of residual oily film that is impossible to avoid,” said Daniel Limonadi of JPL, lead systems engineer for Curiosity’s surface sampling and science system. “And the Sample Analysis at Mars instrument is so sensitive we really have to scrub away this layer of oils that accumulates on Earth.”
The team plans to conduct three scoop and rinse trials – dubbed rinse and discard – of the sample acquisition systems. So it won’t be until the 3rd and 4th soil scooping at Rocknest that a Martian sample would actually be delivered for entry into the SAM and CheMin analytical chemistry instruments located on the rover deck.
“What we’re doing at the site is we take the sand sample, this fine-grained material and we effectively use it to rinse our mouth three times and then kind of spit out,” Limonadi said. “We will take a scoop, we will vibrate that sand on all the different surfaces inside CHIMRA to effectively sand-blast those surfaces, then we dump that material out and we rinse and repeat three times to finish cleaning everything out. Our Earth-based testing has found that to be super effective at cleaning.”
Limondi said the first scooping is likely to be run this Saturday (Oct 6) on Sol 61, if things proceed as planned. Scoop samples will be vibrated at 8 G’s to break them down to a very fine particle size that can be easily passed through a 150 micron sieve before entering the analytical instruments.
The team is being cautious, allowing plenty of margin time and will not proceed forward with undue haste.
“We’re being deliberately slow and incredibly careful,” said Watkins. “We’re taking a lot of extra steps here to make sure we understand exactly what’s going on, that we won’t have to do every time we do a scoop in the future.”
Curiosity’s motorized, clamshell-shaped scoop measures 1.8 inches (4.5 centimeters) wide, 2.8 inches (7 centimeters) long, and can sample to a depth of about 1.4 inches (3.5 centimeters). It is part of the CHIMRA collection and handling device located on the tool turret at the end of the rover’s arm.
“The scoop is about the size of an oversized table spoon,” said Limonadi.
Image caption: Curiosity extends 7 foot long arm to investigate ‘Bathurst Inlet’ rock outcrop with the MAHLI camera and APXS chemical element spectrometer in this mosaic of Navcam images assembled from Sols 53 & 54 (Sept. 29 & 30, 2012). Mount Sharp, the rover’s eventual destination is visible on the horizon. Thereafter the rover drove more than 77 feet (23 meters) eastwards to reach the ‘Rocknest’ sand ripple. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
During the lengthy stay at Rocknest, the rover will conduct extensive investigations of the surrounding rocks and terrain with the cameras, ChemCam laser, DAN, RAD as well as weather monitoring with the REMS instrument.
After finishing her work at Rocknest, Curiosity will resume driving eastward to Glenelg, some 100 meters (yards) away where the team will select the first targets and rock outcrops to drill, sample and analyze.
At Glenelg and elsewhere, researchers hope to find more evidence for the ancient Martian stream bed they discovered at rock outcrops at three different locations that Curiosity has already visited.
Curiosity is searching for organic molecules and evidence of potential habitable environments to determine whether Mars could have supported Martian microbial life forms, past or present.
Image Caption: Curiosity at work on Mars inside Gale Crater. Panoramic mosaic showing Curiosity in action with her wheel tracks and the surrounding terrain snapped from the location the rover drove to on Sol 29 (Sept 4). The time lapse imagery highlights post drive wheel tracks at left, movement of the robotic arm from the stowed to deployed position with pointing instrument turret at right with Mt Sharp and a self portrait of Curiosity’s instrument packed deck top at center. This colorized mosaic was assembled from navigation camera (Navcam) images taken over multiple Martian days while stationary beginning on Sol 29. Click to Enlarge. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
NASA’s Mega Martian Rover Curiosity is swiftly trekking across the Red Planet’s science rich terrain inside Gale Crater as she approaches the two month anniversary since the daring atmospheric plunge and pinpoint touchdown on Aug. 5/6 beside her eventual destination of the richly layered mountainside of Mount Sharp.
In this ultra short span of time, Curiosity has already fulfilled on her stated goal of seeking the signs of life and potentially habitable environments by discovering evidence for an ancient Martian stream bed at three different locations – at the landing site and stops along her traverse route – where hip deep liquid water once vigorously flowed billions of years ago. Liquid water is a prerequisite for the origin of life.
Curiosity discovered a trio of outcrops of stones cemented into a layer of conglomerate rock – initially at “Goulburn” scour as exposed by the landing thrusters and later at the “Link” and “Hottah” outcrops during the first 40 sols of the mission.
If they find another water related outcrop, Curiosity Mars Science Laboratory (MSL) Project Manager John Grotzinger told me that the robotic arm will be deployed to examine it.
“We would do all the arm-based contact science first, and then make the decision on whether to drill. If we’re still uncertain, then we still have time to deliberate,” Grotzinger told me.
Image caption: Remnants of Ancient Streambed on Mars. NASA’s Curiosity rover found evidence for an ancient, flowing stream on Mars at a few sites, including the rock outcrop pictured here, which the science team has named “Hottah” after Hottah Lake in Canada’s Northwest Territories. It may look like a broken sidewalk, but this geological feature on Mars is actually exposed bedrock made up of smaller fragments cemented together, or what geologists call a sedimentary conglomerate. Scientists theorize that the bedrock was disrupted in the past, giving it the titled angle, most likely via impacts from meteorites. This image mosaic was taken by the 100-millimeter Mastcam telephoto lens on Sol 39 (Sept. 14, 2012). Credit: NASA/JPL-Caltech/MSSS
“This is the first time we’re actually seeing water-transported gravel on Mars. This is a transition from speculation about the size of streambed material to direct observation of it,” said Curiosity science co-investigator William Dietrich of the University of California, Berkeley.
Image Caption: Curiosity conducts 1st contact science experiment at “Jake” rock on Mars. This 360 degree panoramic mosaic of images from Sols 44 to 47 (Sept 20-23) shows Curiosity arriving near Jake rock on Sol 44. The robot then drove closer. Inset image from Sol 47 shows the robotic arm extended to place the science instruments on the rock and carry out the first detailed contact science examination of a Martian rock with the equipment positioned on the turret at the arms terminus. Jake rock is named in honor of recently deceased team member Jake Matijevic. This mosaic was created in tribute to Jake and his outstanding contributions. Click to Enlarge. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
The one-ton robot soon departed from her touchdown vicinity at “Bradbury Landing” and set off on a multi-week eastwards traverse to her first science target which the team has dubbed “Glenelg”.
See our panoramic Curiosity mosaics herein showing the rovers movements on various Sols as created by Ken Kremer and Marco Di Lorenzo from NASA raw images.
Curiosity is also now closing in on the spot from which she will reach out with the advanced 7 foot long (2.1 meter) robotic arm to scoop up her very first Martian soil material and deliver samples to the on board chemistry labs.
At a Sept. 27 briefing for reporters, Grotzinger, of Caltech in Pasadena, Calif., said the team hopes to find a suitable location to collect loose, gravelly Martian soil within the next few sols that can be easily sifted into the analytical labs. Curiosity will then spend about 2 or 3 weeks investigating the precious material and her surroundings, before continuing on to Glenelg.
The science team chose Glenelg as the first target for detailed investigation because it sits at the intersection of three distinct types of geologic terrain, affording the researchers the opportunity to comprehensively explore the diverse geology inside the Gale Crater landing site long before arriving at the base of Mount Sharp. That’s important because the rover team estimates it will take a year or more before Curiosity reaches Mount Sharp, which lies some 10 kilometers (6 miles) away as the Martian crow flies.
As of today, Sol 53, Curiosity has driven a total distance of 0.28 mile (0.45 kilometer) or more than ¾ of the way towards Glenelg. Yestersol (Sol 52), the six wheeled robot drove about 122 feet (37.3 meters) toward the Glenelg area and is using visual odometry to assess her progress and adjust for any wheel slippage that could hint at sand traps or other dangerous obstacles.
The longest drive to date just occurred on Sol 50 with the robot rolling about 160 feet (48.9 meters).
Curiosity recently conducted her first detailed rock contact science investigation with the robotic arm at a rock named “Jake”, in honor of Jake Matijevic, a recently deceased MSL team member who played a key and leading role on all 3 generations of NASA’s Mars rovers. See our 360 degree panoramic “Jake rock” mosaic created in tribute to Jake Matijevic.
Curiosity is searching for hydrated minerals, organic molecules and signs of habitats favorable for past or present microbial life on Mars.
Image Caption: “Hottah” water related outcrop. Context mosaic shows location of Hottah” outcrop (bottom right) sticking out from the floor of Gale Crater as imaged by Curiosity Navcam on Sol 38 with Mount Sharp in the background. The Glenelg science target lies in the terrain towards Mt Sharp. This is what an astronaut geologist would see on Mars. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
Alluvial Fan Where Water Flowed Downslope. This image shows the topography, with shading added, around the area where NASA’s Curiosity rover landed on Aug. 5 PDT (Aug. 6 EDT). The black oval indicates the targeted landing area for the rover known as the “landing ellipse,” and the cross shows where the rover actually landed.An alluvial fan, or fan-shaped deposit where debris spreads out downslope, has been highlighted in lighter colors for better viewing. On Earth, alluvial fans often are formed by water flowing downslope. New observations from Curiosity of rounded pebbles embedded with rocky outcrops provide concrete evidence that water did flow in this region on Mars, creating the alluvial fan. Credit: NASA/JPL-Caltech/UofA
Why is everyone so excited about these dusty Mars rocks?
This week’s big news was the announcement of evidence for flowing water on Mars, based on images of what appear to be smooth river rock-type pebbles found by Curiosity. Of course that’s a big statement to make, and for good reason — identifying water, whether present or past, is one step closer to determining whether Mars was ever a suitable place for life to develop. Yet here we are, not even two months into the mission and Curiosity is already sending us solid clues that Mars was once a much wetter place than it is now.
JPL released a video today providing a brief-but-informative overview of what Curiosity has discovered in Gale Crater and why it’s gotten everyone so excited.
Check it out so you’ll have something to talk about over the weekend:
MSL Long Term Planner Sanjeev Gupta reviews Curiosity’s latest discovery
Raw image of Phobos above Mars, taken by Curiosity's Mastcam in September 2012. Credit: NASA/JPL-Caltech
Mars’ moon Phobos is captured in a daytime image by Curiosity (NASA/JPL-Caltech/MSSS)
A raw image taken on September 21 by Curiosity’s right Mastcam shows a daytime view of the Martian sky with a crescent-lit Phobos in the frame… barely visible, yes, but most certainly there. Very cool!
The image above is a crop of the original, contrast-enhanced and sharpened to bring out as much detail as possible.
The 13-km-wide Phobos has been spotted several times before by Mars rovers, most recently during a solar transit on September 13 (sol 37) but I’m not sure if it’s ever been clearly captured on camera during the day before (i.e., not passing in front of the Sun.) If not, this will be a first!
See the latest news from the Curiosity mission here.
Added 9/28: According to Universe Today publisher Fraser Cain, this is “the most dramatic space picture of the year”… whether you agree or not, hear what he had to say on this and other recent news during the September 27 episode of the Weekly Space Hangout.
Just one of several weather stations set up at Chott El Jerid, a Tunisian saltpan, measuring temperature, humidity, ultraviolet radiation, wind direction and velocity. Image credit: Felipe Goméz/Europlanet
From orbit and on the ground, Mars looks inhospitable. But it doesn’t look much different than the freezing Antarctic plains, sun-baked saltpans in Tunisia or Spain’s corrosively acidic Rio Tinto, according to a few explorers from the Centro de Astrobiología (CAB) in Madrid, who today presented some of their findings of life during a press conference at the European Planetary Science Congress.
The biggest difference, however, is that life still thrives in these extreme locales on Earth.
“The big questions are: what is life, how can we define it and what the requirements for supporting life?” asks project leader Dr. Felipe Goméz. “To understand the results we receive back from missions like Curiosity, we need to have detailed knowledge of similar environments on Earth. Metabolic diversity on Earth is huge. We have found a range of complex chemical processes that allow life to survive in unexpected places.”
Over the past four years, Goméz and his colleagues have checked Earth’s most inhospitable locales; the Chott el Jerid saltpan in Tunisia, the Atacama Desert in Chile, Rio Tinto in southern Spain and Deception Island in Antarctica.
While visiting Chott el Jerid, the team tracked huge changes in environmental conditions throughout the day but it was a small rise in surface temperature after dusk that caught their eye. “We found that this is caused by water condensing on the surface and hydrating salts which releases heat in an exothermic reaction,” he said in the press release. This is very interesting from the perspective of the REMS instrument on Curiosity — it gives us away to follow when liquid water might be present on the surface.”
The team also built a three-dimensional picture of the subsurface in the saltpan by measuring the electrical properties of the soil. While drilling several meters into the subsurface at Chott el Jerid and in the Atacama Desert, researchers found bacteria at depth that was completely isolated from the surface. The researchers found not only bacteria, but also single-celled halophilic organisms that are able to oxidize metabolites under both aerobic and anaerobic conditions.
Along the surface of Chott El Jerid, which is made up of very pure sodium chloride with a trace of other salts, the team found small pieces of organic matter within the salt crystals. Once analyzed, they found populations of halophilic, salt-loving, dormant bacteria. In the laboratory, they were able to rehydrate the samples and bring the bacteria back to life, Goméz said.
Another unexpected find occurred while studying outcrops of the mineral jarosite at Rio Tinto in Spain. Jarosite, found on the surface of Mars by the Mars Exploration Rover Opportunity, forms only in the presence of water that contains high concentrations of metals, such as iron. The outcrops at Rio Tinto also are extremely corrosive. Yet, sandwiched between layers in the salt crusts, the team found photosynthetic bacteria. Unexpectedly, iron in the salt crust seems to protect bacteria from ultraviolet radiation, Goméz said. Samples of bacteria with iron present were exposed with high levels of ultraviolet radiation. They survived while bacteria samples without iron were destroyed.
“What the bacteria we found in Rio Tinto show is that the presence of ferric compounds can actually protect life. This could mean that life formed earlier on Earth than we thought. These effects are also relevant for the formation of life on the surface of Mars,” says Goméz. The team also found that salt provides stable conditions that can allow life to survive in very hard environments.
“Within salts, the temperature and humidity are protected from fluctuations and the doses of ultraviolet radiation are very low,” explained Goméz. “In the laboratory, we placed populations of different bacteria between layers of salt a few millimetres thick and exposed them to Martian conditions. Nearly 100% of deinoccocus radiodurans, a hardy type of bacteria survived being irradiated. But fascinatingly, about 40% of acidithiobacillus ferrooxidans – a very fragile variety of bacteria – also survived when protected by a salt crust.”
The findings have implications not only for studying possible life on Mars, but also for the development of life on early Earth.
Source: European Planetary Science Congress (EPSC) 2012 Press Release
Image Details: Photosynthetic bacteria at Rio Tinto. Credit: Felipe Goméz
About the author: John Williams is owner of TerraZoom, a Colorado-based web development shop specializing in web mapping and online image zooms. He also writes the award-winning blog, StarryCritters, an interactive site devoted to looking at images from NASA’s Great Observatories and other sources in a different way. A former contributing editor for Final Frontier, his work has appeared in the Planetary Society Blog, Air & Space Smithsonian, Astronomy, Earth, MX Developer’s Journal, The Kansas City Star and many other newspapers and magazines. Follow John on Twitter @terrazoom
Plaque on the exterior of Mars Science Laboratory, aka “Curiosity” (NASA/JPL-Caltech/MSSS)
Curiosity drops a few rather big names in recent images taken with its MAHLI (Mars Hand Lens Imager) camera: here we see a plaque affixed to its surface bearing the names and signatures of U.S. President Barack Obama, Vice President Joe Biden, Office of Science and Technology Director John Holdren, NASA Administrator Charles Bolden and other key figures responsible for making the Mars Exploration Program possible.
You never know… even on another planet it can’t hurt to have friends in high places!
The image was captured by MAHLI on September 19, the 44th sol of the MSL mission. (See the original raw downlink here.)
The rectangular plaque is made of anodized aluminum, measuring 3.94 inches (100 mm) high by 3.23 inches (82 mm) wide. It’s attached to the front left side of Curiosity’s deck with four bolts. (Explore Curiosity in 3D here.)
Dust, pebbles and variously-sized bits of Mars can be seen scattered around the plaque and deck, leftover detritus from the rover’s landing.
The complete list of signatures is:
Barack Obama, President, United States of America
Joe Biden, Vice President
John P. Holdren, Director, Office of Science and Technology Policy
Charles F. Bolden, Jr., Administrator, National Aeronautics and Space Administration
Edward J. Weiler, Associate Administrator, Science Mission Directorate (2008–2011)
James Green, Director, Planetary Sciences Division
Doug McCuistion, Director, Mars Exploration Program
Michael Meyer, Program Scientist, Mars Exploration Program
David Lavery, Program Executive, Mars Science Laboratory
In another image taken on the same sol, Curiosity shows some national pride with a circular medallion decorated with the stars and stripes of the American flag. The 68-mm-wide circular aluminum plate is affixed to one of the rover’s rocker arms. It’s just one of its four “mobility logos” — the others having the NASA logo, the JPL logo and the Curiosity mission logo.
Curiosity’s “stars and stripes” American flag mobility logo (NASA/JPL-Caltech/MSSS)
The main purpose of Curiosity’s MAHLI camera is to acquire close-up, high-resolution views of rocks and soil at the rover’s Gale Crater field site. Developed for NASA by Malin Space Science Systems in San Diego, CA, the camera is capable of focusing on any target at distances of about 0.8 inch (2.1 centimeters) to infinity, providing versatility for other uses, such as views of the rover itself from different angles.
Once again, it’s time for the Weekly Space Hangout – our round up of all the big space news stories that you should be aware of. This week we talked about the following interesting stories in space and astronomy:
Yes, Mars gets eclipses too! This brief animation, made from ten raw subframe images acquired with Curiosity’s Mastcam on September 13 — the 37th Sol of the mission — show the silhouette of Mars’ moon Phobos as it slipped in front of the Sun’s limb.
The entire animation spans a real time of about 2 minutes.
As a moon Phobos really is an oddity. In addition to its small size – only 8 miles (13 km) across at its widest – and irregular shape, it also orbits its parent planet at a very low altitude, only 5,840 miles (9,400 km) and thus needs to travel at a relatively high velocity in order to even stay in orbit. Phobos actually orbits Mars over three times faster than Mars rotates, appearing to rise in Mars’ western sky. And its orbit is so low that it can’t even be seen from the polar regions!
Since Phobos, and its even more petite sibling Deimos, are so small, the Mars rovers won’t ever see a total solar eclipse. In fact these events are often referred to as transits rather than actual eclipses.
This isn’t the first time an eclipse was captured by a Mars Exploration Rover; Opportunity witnessed a similar partial eclipse of the Sun by Phobos in December 2010, and Spirit caught a lunar (or “Phobal?”) eclipse on camera back in 2005, when the moon passed into the shadow of Mars.
Curiosity’s find was no accident, either, as mission engineers had the Mastcam already positioned to capture the event. Preparation really pays off!
See the latest images and news from the MSL mission here.
Images: NASA/JPL-Caltech/Malin Space Science Systems. Animation by Jason Major. Inset image: Phobos as seen by Mars Express ESA/DLR/FU Berlin (G. Neukum)
UPDATE 9/19/12: See a close-up animation of the eclipse event here.
The slopes of Gale Crater as seen by Curiosity are reminiscent of the American southwest (NASA/JPL-Caltech)
“Mars ain’t no kind of place to raise your kids; in fact it’s cold as hell” sang Elton John in “Rocket Man”, and although the song was released in 1972 — four years before the first successful landing on Mars — his weather forecast was spot-on. Even though the fantastic images that are being returned from NASA’s Curiosity rover show a rocky, ruddy landscape that could easily be mistaken for an arid region of the American Southwest one must remember three things: this is Mars, we’re looking around the inside of an impact crater billions of years old, and it’s cold out there.
Over the first 30 sols, air temperature has ranged from approximately -103 degrees Fahrenheit (-75 Celsius) at night to roughly 32 degrees Fahrenheit (0 Celsius) in the afternoon. Two factors conspire to cause such a wide daily range (most day-night fluctuations on Earth are about 10 to 30 degrees Fahrenheit). The martian atmosphere is very thin; with fewer molecules in the air to heat up and cool down, there’s more solar power to go around during the day, and less atmospheric warmth at night, so the magnitude of temperature shifts is amplified. There is also very little water vapor; water is particularly good at retaining its heat, and the dryness makes the temperature swings even more pronounced.
In that way Mars is like an Earthly desert; even after a blisteringly hot day the temperatures can plummet at night, leaving an ill-prepared camper shivering beneath the cold glow of starlight. Except on Mars, where the Sun is only 50% as bright as on Earth and the atmosphere only 1% as dense, the nighttime lows dip to Arctic depths.
“Deserts on Earth have very extreme temperature ranges,” says Mars Science Laboratory Deputy Project Scientist, Ashwin Vasavada. “So if you take a desert on Earth and put it in a very thin atmosphere 50% farther from the Sun, you’d have something like what we’re seeing at Gale Crater.”
And although the afternoon temperatures in Gale may climb slightly above freezing that doesn’t mean liquid water will be found pooling about in any large amounts. Curiosity’s in no danger from flash floods on Mars… not these days, anyway.
With atmospheric pressure just above water’s thermodynamic triple point, and temperatures occasionally hovering around the freezing point, it is likely that local niches are seeing above-zero temperatures, and Vasavada acknowledges, “liquid water could exist here over a tiny range of conditions.” But don’t expect a Culligan water plant in Gale Crater any time soon. “We wouldn’t expect for Curiosity to see liquid water, because it would evaporate or re-freeze too quickly,” explains Vasavada. “With so little water vapor in the atmosphere, any liquid water molecules on the surface would quickly turn to gas.”
So when on Mars, drink your coffee quickly. (And pack a blanket.)
“Gale Crater may look like the dusty, basaltic basins of the American southwest, but one look at the thermometer will send you running for the winter coat.”
