The Spirit Rover’s Big Discovery

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Amazingly, the two Mars rovers, Spirit and Opportunity, have been working diligently on the surface of the Red Planet for almost four years now. So far, Opportunity has grabbed most of the spotlight, finding evidence for past water on Mars within months after landing on the smooth plains of Meridiani Planum. While Spirit has been working just as hard, if not harder, climbing hills and traversing the rocky terrain of Gusev Crater, she hasn’t yet caused quite the stir that her twin has. But now, a recent discovery by Spirit at an area called Home Plate has researchers puzzling over a possible habitat for past microbial organisms.

What Spirit found is a patch of nearly pure silica, a main ingredient in window glass.

“This concentration of silica is probably the most significant discovery by Spirit for revealing a habitable niche that existed on Mars in the past,” said Steve Squyres, principal investigator for the rovers’ science payload.

The silica could have been produced from either a hot-spring type of environment or another type of environment called a fumarole, where acidic steam rises through cracks in the planet’s surface. On Earth, both of these types of environments teem with microbial life.

“The evidence is pointing most strongly toward fumarolic conditions, like you might see in Hawaii and in Iceland,” said Squyres. “Compared with deposits formed at hot springs, we know less about how well fumarolic deposits can preserve microbial fossils. That’s something needing more study here on Earth.”

Squyres said the patch that Spirit has been studying is more than 90 percent silica, and that there aren’t many ways to explain such a high concentration. One way is to selectively remove silica from the native volcanic rocks and concentrate it in the deposits Spirit found. Hot springs can do that, dissolving silica at high heat and then dropping it out of solution as the water cools. Another way is to selectively remove almost everything else and leave the silica behind. Acidic steam at fumaroles can do that. Scientists are still assessing both possible origins.

One reason Squyres favors the fumarole story is that the silica-rich soil on Mars has an enhanced level of titanium. On Earth, titanium levels are relatively high in some fumarolic deposits.

Meanwhile both rovers are hunkering down for another winter season on Mars. Spirit’s solar panels are currently coated with dust from the huge dust storm the rovers endured this summer, and Spirit will need to conserve energy in order to survive the low light levels during the winter.

“The last Martian winter, we didn’t move Spirit for about seven months,” said John Callas, project manager for the rovers. “This time, the rover is likely to be stationary longer and with significantly lower available energy each Martian day.”

I’m keeping my fingers crossed for another solar panel cleaning windstorm event, which has happened previously, giving the rovers a boost in power.

Original News Source: Jet Propulsion Laboratory News Release

Building Blocks of Life Can Form on Cold, Rocky Planets — Anywhere

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Our old friend and headline-maker is back in the news. Meteorite ALH84001 — the Mars rock that sent the world of astrobiology into a tizzy back in 1996 — hasn’t been just sitting around collecting dust. Researchers have been re-examining the famous meteorite in an effort to learn more about the early history of Mars. Not only did ALH84001 help determine that the building blocks of life actually did form on early Mars, but also that those same building blocks have the potential to form on a cold rocky planet anywhere in the Universe.

The meteorite, found in the Alan Hills region of Antarctica, grabbed the headlines over 11 years ago when scientists claimed to have found the remains of bacteria-like life forms within the rock from Mars. The claims have been hotly debated, with both sides still holding firm in their convictions.

But scientists at the Carnegie Institution’s Geophysical Laboratory took the research into ALH84001 a step further, and have shown for the first time that building blocks of life formed on Mars early in its history. Organic compounds that contain carbon and hydrogen form the building blocks of all life here on Earth. Previously, some scientists thought that organic material in ALH84001 was brought to Mars by meteorite impacts, and others felt the material might have originated from ancient Martian microbes, while still others thought any organics in the rock probably were introduced after it arrived on Earth.

The Carnegie-led team made a comprehensive study of the ALH 84001 meteorite and compared the results with data from related rocks found on Svalbard, Norway. The Svalbard samples came from volcanoes that erupted in a freezing Arctic climate about 1 million years ago — possibly mimicking conditions on early Mars.

“Organic material occurs within tiny spheres of carbonate minerals in both the Martian and Earth rocks,â€? said Andrew Steele, lead author of the study. “We found that the organic material is closely associated with the iron oxide mineral magnetite, which is the key to understanding how these compounds formed.”

“The results of this study show that volcanic activity in a freezing climate can produce organic compounds,” said Hans E.F. Amundsen, a co-author in the study from Earth and Planetary Exploration Services. “This implies that building blocks of life can form on cold rocky planets throughout the Universe.”

The organic material in the Allan Hills meteorite may have formed during two different events. The first, similar to the Svalbard samples, was during rapid cooling of fluids on Mars. A second event produced organic material from carbonate minerals during impact ejection of ALH84001 from Mars.

“Our finding sets the stage for the Mars Science Laboratory (MSL) mission in 2009,” said Steele, who is a member of the Sample Analysis on Mars (SAM) instrument team onboard MSL. “We now know that Mars can produce organic compounds. Part of the mission’s goal is to identify organic compounds, their sources, and to detect molecules relevant to life. We know that they are there. We just have to find them.”

This makes the MSL mission all the more exciting and anticipated. And perhaps the team of scientists who made the claims about microbes in ALH 84001 back in 1996 have something to strengthen their case.

Original News Source: Carnegie Institution For Science Press Release

Water or Land: The Orion Landing Choice

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Work is progressing on designing the new Orion Crew Exploration Vehicle (CEV), the next generation of NASA spacecraft that will take humans to the International Space Station, back to the Moon, and hopefully on to Mars. But one major question about the spacecraft has yet to be answered. On returning to Earth, will the CEV splash down in water, or land on terra firma?

NASA officials discussed various aspects of development that is currently underway for the Constellation program at a media briefing on December 10. The mobile launch platform for the Ares rocket is being built, landing parachutes have been tested and the first capsule structure of the new CEV will be constructed starting in early 2008. Design requirements for the booster rockets have been completed and just ahead are final design definitions for operational capabilities such as ground procedures at Kennedy Space Center, mission control in Houston and other areas such as spacesuit design.

Additionally research on the International Space Station has begun to help prepare for long duration spaceflights such as a measurements of microbe growth, a study of the formation of kidney stones, and a nutritional study to help understand what is “normal” for the human body in space.

But questions from the media focused mainly on the yet unmade decision of whether the CEV will land in the water or on land.

NASA originally explored multiple options for landing in both water and land. After initial studies, the first assessment by NASA and the contractor for the CEV, Lockheed Martin, was that landing on land was preferred in terms of total life cycle costs for the vehicles. But now a splashdown in water seems to be favored.

“There are a couple of aspects that pop out at us,” said Jeff Hanley, Manager for the Constellation Program. “One is the safety and the risks involved in landing. Looking at the landing itself, the event of actually touching down, water comes out to be preferable as less risk. Another aspect is the performance of the Orion vehicle as it is sent to the moon. In looking at what it takes to get a pound of spacecraft to low lunar orbit in terms of the cost, every pound that you send toward the moon is precious. From an efficiency and performance point of view, carrying 1500 lbs of landing bags to the moon and back when we have a perfectly viable mode of landing in the water near a US coastal site didn’t seem like a good trade in performance. We’ve tended toward updating our point of departure concept to now be a nominal US coastal water landing.”

The Constellation program has always considered that for the first few missions, the spacecraft would land in water until the guidance system had been tested thoroughly and proven in actual landings.

But NASA is continuing to look at landing on land as a possibility for future flights. “We want to be able to land on land in a contingency and have the crew be able to get out and walk away. Ther are limitation of what you can do on land but by the time we get done really looking at what the minimal capability of landing on land and having the crew walk away, we’ll see what the design looks like, and if the design is robust enough we could return to having nominal land landings.”

One challenge for the Constellation program has been getting the CEV light enough for the Ares rockets to be able to launch it, and therefore eliminating the 1500 lb airbags for landing has its appeal.

“The predominant design philosophy for Orion and Ares 1 has been that we are designing for lunar missions,” continued Hanley. “We will service the International Space Station within that set of capabilities. From that perspective, designing a lot of mass into the spacecraft just to enable land landings has not traded out to be an effective use of our performance. That’s the major consideration in play. Right behind that are life cycle costs.”

Making the decision of land vs. water is the goal for 2008 for the Constellation program. “We’ve studied and have cost estimates for water landings against the infrastructure costs of having multiple landing sites on land and they are comparable,” said Hanley. Right now, NASA is looking at a single target landing zone off the coast of California with one or two recovery vessels.

But they are keeping their options open for a land landing. “If the Orion team is able to come in at the preliminary design review later this next year with a concept for be able to land on land that is fairly robust but not cost a lot of mass to have to hurl to the moon and back, then it becomes an operational decision,” said Hanley.

There has been much debate about what type of landing would be best. “There’s been a lot of assumptions made that landing on land is going to be better, but there are lot of people in the technical community that do not buy into that,” said Hanley. “There’s been a lot of debate surrounding whether or not land landing truly is better from a life cycle cost perspective and there isn’t a lot of quantitative data to really pull from.”

Hanley feels there are assumptions being made but not a lot of substantive date to clarify what the right answer is. So the next steps are to get the spacecraft to a detailed preliminary design and really interrogate the water vs. land issue. That includes further developing the operational concepts , such as how long does the capsule stay in the water, and what loads does the spacecraft see from landing on water and land. Those are all questions that need to be answered in order to make a final decision on the type of landing that will be used.

Stay tuned, as 2008 should be a year of decision for many details about Constellation and the CEV.

Original News Source: NASA News Audio

Shuttle Launch Delayed Until January 2

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Space shuttle Atlantis’ STS-122 mission to the International Space Station has been further delayed and now is targeted to launch no earlier than Jan. 2. The liftoff date hinges on the resolution of a repeat failure of the shuttle’s fuel sensor system. NASA has not yet made a final decision if repairs to the system will be done on the launch pad or if Atlantis will need to be rolled back to the Vehicle Assembly Building where the external tank can be removed.

“It would depend on what we find…but we have a lot of options in front of us,� said NASA’s Mission Management Team chairman LeRoy Cain at Sunday morning press briefing. Cain added that if they do decide to roll back, that probably would not support a January 2 launch. However, STS-122 Launch Director Doug Lyons said he couldn’t envision a scenario that would necessitate a rollback. “We have almost limitless access (to the tank) and there are not many things we can’t do on the launch pad that we could do at the VAB.�

Early Sunday, one of the four engine cutoff (ECO) sensors inside the liquid hydrogen section of Atlantis’ external fuel tank gave a false reading while the tank was being filled. NASA’s new and updated Launch Commit Criteria require that all four sensors function properly. Following Friday’s launch scrub, the MMT decided to shorten the launch window to one minute in an effort to work around the sensor problem. Upon launch, this would send the shuttle on a direct trajectory to the space station, and would save fuel. Fuel depletion is what drives the need for the ECO sensors which protect the shuttle’s main engines by triggering engine shut down if fuel runs unexpectedly low. But the MMT also added the criteria that a failure of any of the four sensors would prompt a launch scrub.

Previously, the criteria required that three of the four sensors had to function properly. Atlantis’ scheduled launch on Thursday, Dec. 6, was delayed after two liquid hydrogen ECO sensors gave false readings. A third sensor gave a false reading while the tank was being emptied.

Meanwhile, ISS flight controllers informed space station commander Peggy Whitson that she and crewmate Dan Tani likely will be asked to carry out a spacewalk later this month to inspect a problematic solar array rotary joint on the right side of the lab’s main power truss. If the launch of STS-122 had gone as planned, a team of shuttle astronauts would have conducted the inspection.
The crew of STS-122 will come out of quarantine and return to Houston.

The main objective of Atlantis’ mission is to deliver, install and activate the European Space Agency’s Columbus laboratory, which will provide scientists around the world the ability to conduct a variety of life, physical and materials science experiments.

Following STS-122, the next two flights on the shuttle manifest for space station construction are scheduled for launch in mid February and late April. The next flight after that is an August mission to service the Hubble Space Telescope. Bill Gerstenmaier, Associate Administrator of spaceflight operations at NASA said that this delay shouldn’t affect NASA’s ability to complete station construction before the shuttle is scheduled to be retired in 2010. “This doesn’t impact the overall manifest. With the remaining time we can accomplish all the flights,� Gerstenmaier said.

Original News Source: NASA TV

Shuttle Launch No Earlier Than Saturday

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The crew of STS-122 and the Columbus science module will have to wait a little longer for their ride to space. The launch of space shuttle Atlantis has been pushed back to no earlier than Saturday, December 8. After assessing the problem with the engine cutoff sensors that scrubbed Thursday’s scheduled liftoff, NASA’s Mission Management Team decided they needed more time to look at the problem. But even a Saturday launch is a best-case scenario, and further delays loom as a possibility.

Engineers continue to examine the circuitry and NASA will hold a briefing at 5 pm EST today to announce when another launch will be attempted. A Saturday launch would be at 3:43 pm and Sunday at 3:20 pm EST. The forecast for Saturday calls for a 60 percent chance of good weather, improving to 70 percent on Sunday.

Based on data received during fueling on Thursday, engineers believe the problem may involve an open circuit between the sensors in the hydrogen portion of the external fuel tank and an electronic box in the shuttle main engine compartment. Two of four sensors failed in a test that is routinely done during tanking. The fuel cutoff sensor system is one of several that protect the shuttle’s main engines by triggering their shut down if fuel runs unexpectedly low. Launch Commit Criteria require that three of the four sensor systems function properly before liftoff. The sensors also gave another false reading while the tank was being emptied, but are now currently indicating correctly the tank is dry.

The current launch window closes on December 13. If the shuttle can’t launch before then, the next earliest launch date wouldn’t be until January 2. While NASA officials initially said they would try to launch today, after a five hour meeting the Mission Management Team decided to hold off for another day. “We need more time,â€? said LeRoy Cain, Chairman of the MMT. “This (problem) is a little bit new, so we want to sleep on it. I can almost guarantee you we will have some new thinking after we let this team go home and rest.”

Since engineers think the problem lies in an open circuit, currently, NASA doesn’t believe any major repairs in hardware will need to be done, which would cause a longer delay for the launch.

“We’re still hoping, and have reason to believe, that we’re going to get off in December,” said Doug Lyons, NASA’s shuttle launch director, “and that’s what we’re shooting for.”

Atlantis will carry the crew of STS-122 to the International Space Station to deliver the Columbus Science Module. Columbus is the European Space Agency’s major contribution the ISS.

Officials from the ESA were disappointed in the delays, but said that safety is most important. “This is perfectly normal,” said Alan Thirkettle, the ESA’s space station program manager, of the launch delay. “We want to launch on time, but we want to launch right.”

Original News Source: NASA TV

Shuttle Launch Postponed

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A problem with space shuttle Atlantis’ fuel sensors has prompted a scrub of today’s scheduled launch of the STS-122 mission to the International Space Station. During fueling of the shuttle’s external tank, two of four engine cutoff sensors failed. Engineers are working on fixing the problem and NASA will try to launch again tomorrow, Friday, December 7 at 4:09 pm EST.

Sensors located in the hydrogen portion of the tank “failed wet” during fuel loading this morning. That means the sensors could falsely indicate the tank still contains hydrogen in the last stages of the shuttle’s climb to space when it actually is empty. The engines would continue to run, and without fuel, the engines could ignite and explode.

Problems with the engine cutoff sensors have occurred before during tanking, including the first shuttle mission after the Columbia accident, STS-114 with space shuttle Discovery. The failed sensors caused a one-day delay in the launch and after the flight the problem was traced to a faulty connection in electrical cables. NASA hopes that in emptying the tank and then refueling tomorrow the sensors will reset correctly, as was the case with the STS-114 launch.

This shuttle mission, STS-122, will bring the Columbus science module to the ISS. Columbus is the European Space Agency’s cornerstone contribution to the space station. Two ESA astronauts, Hans Schlegel from Germany, and Leopold Eyharts from France, are part of the shuttle crew, and Eyharts will remain on board the station to lead the activation of the new lab. The other astronauts for the mission are Commander Stephen Frick, pilot Alan Poindexter and mission specialists Rex Walheim, Stanley Love, and Leland Melvin.

STS-122 is expected to be an 11 day mission. It is the 121st shuttle flight and the 24th mission to the ISS.

Original News Source: NASA TV

‘Tis the Season to Explore the North Pole on the Moon

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Mention the North Pole this time of year and perhaps what comes to mind are visions of snowy, candy cane-lined streets leading to a candle-lit workshop. But how about sun-drenched regolith dotted with craters cast in permanent shadows? Those are the types of images revealed in a new detailed map of the north pole — on the moon.

A mosaic created from data obtained by the SMART-1 spacecraft shows detailed features of the geography and illumination of the lunar north pole. These maps can be used by future explorers as an aid for traveling and traversing on the moon.

The lunar poles are of interest for science and the upcoming exploration of the moon mainly because of their exposure to sunlight. There are areas that are continually bathed in sunlight, but within craters in the same region are dark areas that rarely receive any light, and therefore could contain water ice. Both these aspects would be important for potential lunar base sites.

“Solar illumination makes these areas ideal for robotic outposts or lunar bases making use of solar power, ” said the European Space Agency’s Bernard Foing, who is Project Scientist for the SMART-1 Spacecraft.

Any water ice on the moon would be useful for the inhabitants of a lunar base.

The SMART-1 north pole map covers an area of about 800 by 600 km and shows the geographical locations of several craters. Of special interest is Peary Crater, the largest impact crater that is close to the lunar north pole. At this latitude the interior of the crater receives little sunlight, but SMART-1 was able to observe it during phases when the crater floor was sufficiently illuminated for imaging.

Also imaged was Crater Plaskett, located on the northern far side of the moon, about 200 kilometers from the north pole. Because of the location of this crater it receives sunlight at a low angle and it has been suggested as a lunar base that could be used for a possible analog to simulate conditions of a manned mission to Mars.

Foing also said that the discovery of water ice on the moon could help us understand Earth’s history as well. “If the layers of ice come from the volatiles deposited by comets or water-rich asteroids, we could better understand how, and how much, water and organic material was delivered to Earth over its history,” he said.

Using electric propulsion navigation, SMART-1 reached lunar orbit in November of 2004 and performed a year and a half of scienctific observations. The mission ended with a controlled impact on the moon’s surface in September of 2006.

The polar mosaics were presented and discussed at the 9th International Lunar Exploration Working Group (ILEWG) lunar conference in October 2007.

SMART-1 science investigations include studies of the chemical composition of the Moon, of geophysical processes such as volcanism, tectonics, cratering, and erosion, and high resolution studies in preparation for future steps of lunar exploration.

Original News Source: ESA Press Release

Columbus to Set Sail for Space

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For European scientists and space enthusiasts, the wait will soon be over. The Columbus module, the European Space Agency’s (ESA) major component for the International Space Station, will finally be delivered to the ISS aboard space shuttle Atlantis on STS-122. The launch is scheduled for Thursday, December 6, 2007 at 4:31 pm EST. Flying along with Columbus are two ESA astronauts, Hans Schlegel from Germany, and Leopold Eyharts from France.

The ESA considers Columbus as the most important European mission to the ISS to date and the cornerstone of Europe’s contribution to this cooperative international endeavor.

Creating a human-capable science module for a space station was first proposed by Europeans back in 1985. At that time France was considering building a mini space shuttle called Hermes to fly to a proposed space station called the Man Tended Free Flyer (MTFF) to be built by Germany and Italy. But with the postponement of MTFF in 1991 and the termination of Hermes in 1993, the planned Columbus module was left with no ride to space and nowhere to go.

When the ESA joined as an ISS partner in 1995, the Columbus science module was a logical contribution for the Europeans. The module was completed in 2000, and the original date for delivery of Columbus to orbit was 2004. But that date was pushed back following the Columbia space shuttle accident in 2003.

Columbus is 7 meters (23 feet) long and 4.5 meters (15 feet) in diameter and will hold specialized experiments for multidisciplinary research into biology, physiology, material science, fluid physics, technology, life science and education. Columbus can hold ten science racks, but will launch with only five in place, as future missions will bring more science racks on board. Additionally, there are two stands bolted to the outside of the module that can be used for research on materials and for unfiltered views of space. Columbus will be attached to the Harmony node’s starboard docking port.

Schlegel will play a key role in two of the three spacewalks or EVA (Extra-Vehicular Activity) scheduled for the mission, helping to install and power up the laboratory.

Eyharts will stay aboard the ISS for a long duration mission, replacing Dan Tani who will return to Earth on the shuttle. Eyharts will play a key part in the installation, activation and in-orbit commissioning of Columbus and its experimental facilities.

Once in orbit, Columbus will be monitored from ESA’s Columbus Control Centre located within DLR’s German Space Operations Centre in Oberpfaffenhofen, near Munich.

The American astronauts on Atlantis are Commander Stephen Frick, pilot Alan Poindexter and mission specialists Rex Walheim, Stanley Love, and Leland Melvin.

The forecast for Thursday’s launch is 80 percent “go,” decreasing to 60 percent on Friday and Saturday.

Original News Source: ESA Press Release

NASA’s New Look

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NASA unveiled a new look for its website over the weekend, and hopes that blogs, interactive features, and a customizable layout will especially appeal to 18-25 year olds.

A New York Times article reported that NASA is concerned that the social networking generation hasn’t shown enough interest in NASA, and the space agency hopes their new webpage will attract the MySpace crowd. This is the first major overhaul for NASA’s website since 2003, and NASA now hopes to compete with Space.com and CNN’s more chic presentations of space exploration. Numerous rollovers, links, and spectacular graphics can keep a visitor engaged for quite awhile, and readers can now Digg, del.icio.us or StumbleUpon stories that they like or want to share. The “Image of the Day” Gallery also benefited with a much-needed upgrade.

Critical Mass, the company that assisted NASA with the new design, says on their website that NASA’s site will now “inspire, involve and inform” and will unify over 3,500 different sites into a “cohesive information gateway.”

One past criticism of the different NASA webpages is that there was sometimes redundant or conflicting information. Critical Mass and their partner eTouch Systems claim the new site will fuel NASA’s efforts to “reconnect with the public and re-capture significance as one of the world’s most visionary and imaginative organizations.”

Still, Brian Dunbar, Internet Services Manager for NASA estimates that even before the overhaul, NASA’s website received approximately one million unique visitors each month. Not bad for an aging, old-fashioned, 50-year old.

Chime in with your thoughts about NASA’s revamped webpage on the BAUT Forum.

Original Source: New York Times

Meteorites Reveal Mars’ Past: Molten Surface, Thick Atmosphere

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If Mars ever had water flowing on its surface, as the many canyons and riverbed-like features on the Red Planet seem to indicate, it also would have needed a thicker atmosphere than what encircles that planet today. New research has revealed that Mars did indeed have a thick atmosphere for about 100 million years after the planet was formed. But the only thing flowing on Mars’ surface at that time was an ocean of molten rock.

A study of Martian meteorites found on Earth shows that Mars had a magma ocean for millions of years, which is surprisingly long, according to Qing-Zhu Yin, assistant professor of geology at the University of California- Davis. For such a persistent event, a thick atmosphere had to blanket Mars to allow the planet to cool slowly.

Meteorites called shergottites were studied to document volcanic activities on Mars between 470 million and 165 million years ago. These rocks were later thrown out of Mars’ gravity field by asteroid impacts and delivered to Earth — a free “sample return mission” as the scientists called it — accomplished by nature.

By precisely measuring the ratios of different isotopes of neodymium and samarium, the researchers could measure the age of the meteorites, and then use them to work out what the crust of Mars was like billions of years before that. Previous estimates for how long the surface remained molten ranged from thousands of years to several hundred million years.

The research was conducted by the Lunar and Planetary Institute, UC Davis and the Johnson Space Center.

Planets form by dust and rocks coming together to form planetisimals, and then these small planets collide together to form larger planets. The giant collisions in this final phase would release huge amounts of energy with nowhere to go except back into the new planet. The rock would turn to molten magma and heavy metals would sink to the core of the planet, releasing additional energy. The molten mantle eventually cools to form a solid crust on the surface.

Although Mars appears to no longer be volcanically active, NASA’s Mars Global Surveyor Spacecraft discovered that the Red Planet hasn’t completely cooled since its formation 4.5 billion years ago. Data from MGS in 2003 indicated that Mars’ core is made either of entirely liquid iron, or it has a solid iron center surrounded by molten iron.

Original News Source: UC Davis Press Release