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Results tagged “mars” from Breaking Orbit

The Mars rovers are true survivors. Although Spirit and Opportunity were slated to work for just 90 Martian days, they've been putting in some serious overtime—they're now at just over 2,000 days on the job and counting.

For its part, Spirit has continued toiling away on Mars even after it broke a "foot," wore down one of its favorite tools, almost starved due to a strong dust storm blotting out sunlight, and suffered a series of memory glitches.

Then, this past May, the robust rover got stuck in the sand.

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A screen shot from a computer simulation shows Spirit's current predicament.
—Picture courtesy NASA/JPL-Caltech

In the midst of a routine drive near Gusev crater, Spirit broke through a thin crust of soil over a filled-in crater. Its wheels became half buried in the soft sand, and the rover was struggling to gain traction on the slippery sulfates below.

So Spirit has stayed put for months while mission managers on Earth have raced to come up with an escape plan.

On Monday, NASA says, after working various tests, computer models, and presumably late nights, engineers will make the first attempt to free the venerable rover.

"This is going to be a lengthy process, and there's a high probability attempts to free Spirit will not be successful" Doug McCuistion, director of the Mars Exploration Program at NASA Headquarters, said in a statement.

"Mobility on Mars is challenging, and whatever the outcome, lessons from the work to free Spirit will enhance our knowledge about how to analyze Martian terrain and drive future Mars rovers," McCuistion said.

The drive to freedom will start with a forward march up a mild slope, which mission managers hope will steer Spirit past a rock lying underneath. Data collected from the first drive attempt will help NASA figure out its next move, and it's anticipated that efforts to edge Spirit out of the crater will continue into early 2010.

But even if the rover can't be budged, Spirit has been learning a lot from its unexpected surroundings.

"The soft materials churned up by Spirit's wheels have the highest sulfur content measured on Mars," said Ray Arvidson, deputy principal investigator for the science payloads on Spirit and Opportunity.

"We're taking advantage of its fixed location to conduct detailed measurements of these interesting materials."

Tracking a Mars Rover

Posted on August 17, 2009 | 0 Comments

rover-traverse-map.jpg

—Image courtesy NASA/JPL/University of Arizona

Those of you who think it's cool to drill into Google Maps and find, for example, your car sitting in your driveway, probably know that it's all about coming to a resolution.

The higher a camera's resolution, the more details you can capture in a single image, and the deeper you can zoom in.

Google gets many of its images from Earth-orbiting probes that have eyes sharp enough to see 19.7 inches (50 centimeters) per pixel.

Such satellites have a counterpart orbiting Mars: the High Resolution Imaging Science Experiment, or HiRISE, camera aboard the Mars Reconnaissance Orbiter.

HiRISE can see in resolutions of 9.8 to 19.7 inches (25 to 50 centimeters) per pixel, enough to take snapshots of features as small as an office desk from about 186 miles (300 kilometers) above the planet's surface.

And like Earthlings scanning web maps for their tricked-out Hondas, Mars mission managers can peer into the more detailed shots of the Martian terrain to pick out their vehicles in action.

Case in point: Last week HiRISE treated us to a glorious new shot of Victoria Crater, which the Mars rover Opportunity had risked life and limb to explore in 2007.

Now peer closely at those scalloped edges, and you can just see where it looks like someone was playing connect the dots up near the crater's left-hand rim.

Those are Opportunity's tacks, preserved in the Martian dust after all this time!

rover-tracks.jpg

—Image courtesy NASA/JPL/University of Arizona

After about a year in the crater, the rover clambered back out and headed south, and NASA's been using its orbiters to follow the rover's path since then.

Using such "traverse maps," like the one featured above, Emily Lakdawalla over at the Planetary Society did some heavy lifting and tracked down the rover itself in the full version of the new crater picture.

She's zoomed in so you can clearly see Opportunity ambling across the red planet's dunes after it had stopped to investigate a Martian meteorite.

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—Image courtesy NASA/JPL/University of Arizona

Now is that freakin' sweet or what?

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—Image courtesy NASA/JPL-Caltech/Cornell University

Dubbed "Block Island," the conspicuous space rock is now the largest confirmed meteorite found on the red planet, NASA announced today.

The Mars rover Opportunity snapped the above portrait of Block Island on July 31, as it moved in closer to touch the meteorite.

Opportunity's examinations revealed that the two-foot-wide object is an iron-nickel meteorite, although where it came from exactly is still anybody's guess.

Although Opportunity and its twin, Spirit, have found several candidate rocks during their five-plus years on Mars, Block Island is only the second official Martian meteorite.

The first—known as Heat Shield Rock, but formally named Meridiani Planum—was found in late 2004.

On the flip side, meteorites from Mars are also pretty rare, all things considered.

According to NASA, of the 24,000 or so space rocks that have been found on Earth, just 34 are known to be from Mars, presumably broken off from the red planet when something else smashed into its surface.

Any allergy sufferer will tell you that dust can be a killer. But those dust bunnies under the couch have nothing on the planet-wide storms that periodically engulf Mars in late spring and early summer.

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—Image courtesy NASA, J. Ball (Cornell), M. Wolff (SSI), and the Hubble Heritage Team (STScI/AURA)

Such storms are kind of a big deal to the twin Mars rovers Spirit and Opportunity, which rely on well-lit solar panels to keep themselves running.

A couple summers ago, dust blocked more than 99 percent of direct sunlight reaching the rovers and nearly spelled doom for the plucky robots, which have been toiling away on Mars since 2001.

rover-spirit-dust-cover.jpg

To try and stay ahead of the curve, the rovers each point a camera toward the sun every day to check for atmospheric clarity, allowing researchers on Earth to adjust the bots' power needs.

Spirit goes into stealth mode?
—Image courtesy NASA/JPL-Caltech/ Cornell

The rovers get some extra help from the Mars Reconnaissance Orbiter, which—among its many talents—can act like a weather satellite and track dust storms from the sky.

"We can identify where dust is rising into the atmosphere and where it is moving from day to day," Michael Malin of Malin Space Science Systems, which operates one of the orbiter's cameras, said in a NASA statement.

Such knowledge is key, as science missions can get interrupted or delayed if there's even a hint that an oncoming storm will drain power reserves.

The orbiter's "weather reports" in recent weeks "have let us be more aggressive about using the rovers," Mark Lemmon, a rover-team atmospheric scientist, said in the statement.

"There have been fewer false alarms. Earlier in the mission, we backed off a lot on operations whenever we saw a small increase in dust. Now, we have enough information to know whether there's really a significant dust storm headed our way."

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—Image courtesy NASA/JPL-Caltech/MSSS

The latest composite image shows almost the whole globe, with billowing clouds of dust being lifted into the air by a storm near the south polar ice cap. (The blurry bits running vertical in the image aren't dust, fyi, but an effect of the camera's viewing geometry.)

Luckily the same wild winds that churn up the occasional dust storm also help clean particles that accumulate on the rover's solar panels. According to NASA, the rovers would have died years ago from dusty buildup if it wasn't for these regular wipe-downs.

Bill Nelson, the rovers' engineering chief, said that this spring "we're all hoping we'll get another good cleaning."

Mars Volcanoes' Watery Tales

Posted on March 5, 2009 | 0 Comments

Is it mold on a bathroom wall? A close-up of a Dalmatian? The results of a tragic toner-cartridge accident?

mars-volcano-frost.jpg

—Image courtesy NASA/JPL/University of Arizona

In fact, it's a Martian volcano in the process of defrosting. The ancient cauldron is part of a group of volcanoes that rings the Hellas impact basin on the red planet's southern hemisphere.

The imaging team with the recently reactivated Mars Reconnaissance Orbiter released the picture this week. Taken in January, the shot shows the volcano covered in frost, except for a few dark patches where the icy sheath is starting to melt away.

Researchers aren't sure why the patchy areas are so special, although they suggest that the spots could be dark sand dunes that soak up the sun's heat better than the surrounding soil.

This particular volcano is a patera, a type of volcanic crater where lava once erupted from vents inside the depression. Research has suggested that some of Mars's paterae could be the tops of shield volcanoes—gently sloping peaks like Hawaii's Mauna Loa—that got buried by later lava flows.

Others could have formed when groundwater mixed with magma, triggering an explosion that created the signature scalloped bowl shape.

Today Mars's volcanoes are no longer active, so it's hard to get a clear picture of how they formed. Some of the youngest known lava flows are anywhere from 20 million to 200 million years old.

Olympus Mons, the solar system's biggest volcano, appears to be a shield volcano, but it has an odd asymmetrical shape that geologists can't quite account for.

olympus-mons-photo.jpg

In a new study released this week, geophysicists used a computer model to see how Olympus might have formed.

What they found is that a bed of clay sediments would have been needed to reduce friction as the lava spread out, creating the lopsided shield. And those clays needed water to form.

—Image courtesy NASA

Evidence for water-requiring minerals on Mars is kinda old news at this point. But the new study is making waves because it also offers the tantalizing hint that liquid water—a key ingredient for life—could still be lurking underneath the massive volcano.

"This deep reservoir, warmed by geothermal gradients and magmatic heat and protected from adverse surface conditions, would be a favored environment for the development and maintenance of thermophilic organisms," the study authors conclude in last month's issue of the journal Geology.

In other words, if there's still heat under the mountain's skirts, Martian life could be hiding in its belly.

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In the animal world, the fight-or-flight instinct is a pretty common response to danger. But when you're a multimillion-dollar spacecraft, caution is usually the only response you get preprogrammed with.

Adding to poor beleaguered NASA's spate of recent glitches, the Mars Reconnaissance Orbiter went into safe mode on Monday after suffering what appears to have been an unexpected power surge.

Initial analysis of the flight data shows that the batteries are charged and the solar panels are doing their thing. The orbiter is also "talking" normally to mission control.

"We are going to bring the spacecraft back to normal operations, but we are going to do so in a cautious way, treating this national treasure carefully," MRO project manager Jim Erickson said in a NASA statement. "The process will take at least a few days."

That means, for the time being, science operations are stalled until NASA can be sure the craft is healthy enough to get turned back on.

Aside from returning what could be some of the most artful images of Mars, since 2006 the craft has been a steady source of pretty cool science.

For example, just yesterday a joint NASA-USGS team announced MRO's high-resolution camera caught what appear to be the first evidence for columnar joints on any planet other than Earth.

mars-columnar-joints.jpg

—Image courtesy NASA/JPL-Caltech/University of Arizona

Columnar joints are fractures that form as lava cools and contracts. These particular joints, found inside an unnamed crater on Mars, resemble features seen on Earth when water gushes over and cools down basalt flows.

Study author Moses Milazzo, of the USGS, notes in the press release that his favorite place to see columnar joints up close is Grand Falls, east of Flagstaff, Arizona.

"If you hike down to the bottom during the dry season, you'll cross some perfect examples of columnar joints, which formed when enormous amounts of water flooded the cooling lava," he said.

Here's hoping the MRO can safely get back to work soon!

Google Mars 3-D Preview

Posted on February 4, 2009 | 0 Comments

[2-6-09 update: now with video!]

In case you are curious but a tad download-shy, I spent a little time exploring Mars today via Google Earth and took a selection of screen shots.

I think I'm in love with the colorized topography layer, which makes abundantly clear the huge demarcation between the southern basin and the northern highlands. Plus it makes Olympus Mons looks like a throbbing pustule.

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—Image courtesy Google

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Those sneaky folks at Google. Even as waves of coverage come pouring forth about the newly launched oceans layer in Google Earth, a short NASA press release and no more than a few lines in a couple news articles note that, oh, yeah, and by the way, there's a new 3-D Mars layer too.

Wha?!?!?

Sure enough, it's in the new Google Earth version 5.0, and It's beautimous. Just launch Earth, click the top tab with the Saturn-looking icon on it, and toggle between Earth, Sky, and Mars.

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—Google Earth, Mars layer screenshot

[Google Sky, btw, was launched in 2007 and features a ridonkulous amount of astronomy data, from pretty pictures to current and historical sky charts. Fun.]

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HiRISE Spies a Young Martian Crater

Posted on January 23, 2009 | 0 Comments

By now folks used to reading about Mars have gotten pretty spoiled by the amazing images from the High Resolution Imaging Science Experiment (HiRISE) aboard the Mars Reconnaissance Orbiter.

This fabulous camera came online in 2006 and returned its first color images of Mars in 2007.

The current catalog of more than 8,700 images is a study in how science can become art—rippling sand dunes and scalloped craters in gentle hues of blue and red can look more like exhibits at the MoMA than data on planetary geology.

So at first blush it can be a bit of a downer when a HiRISE image looks like this:

mars-young-crater.jpg

—Image courtesy NASA/JPL/University of Arizona

But hey, this is a science experiment, and this contrasty crater is just busting with science.

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Active Mars Belches Methane

Posted on January 15, 2009 | 0 Comments

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For a planet at the center of so many discussions about life, Mars can seem like a really dead world.

It's cold, dry, and dusty with a thin atmosphere that doesn't block out much solar radiation. There's minerals and gullies that suggest water flowed there more than three billion years ago, but aside from a few wandering robots, a big landslide, and the occasional planet-wide dust storm, modern Mars doesn't seem to see a lot of action.

Or maybe we just haven't been looking in the right places.

Today a group of university and NASA scientists announced they've found plumes of methane that could be coming from some mysterious underground source on Mars's northern hemisphere.

mars-plumes.jpg

—Image courtesy NASA

Over a three-year span starting in 2003, ground-based observatories saw that the plumes appeared and disappeared, varying with the seasons. At one point Mars spewed out about 19,000 metric tons of methane at nearly 0.6 kilograms a second. Take that, Aussie sheep.

And so comes the big question: Does active methane mean life in motion?

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Phoenix, Gone But Not Forgotten

Posted on January 9, 2009 | 0 Comments

Great stars don't die, they just fade away.

It's been almost two months since NASA lost contact with the Phoenix Mars Lander, which had been studying icy soils near the red planet's north pole.

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The lander's surface stereo imager made a mosaic to show the craft from a few feet in the air—that black spot is where the camera is mounted.
—Image courtesy NASA/JPL/University of Arizona/Texas A&M University

As summer moved into fall, sunlight began to fade and temperatures dropped too far for the lander to keep up operations, bringing the just over five-month mission to a nominal end.

One thing that's been made clear is that 2008 was the summer of the Phoenix.

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It's IYA, Baby!

Posted on January 4, 2009 | 1 Comments

After shaking off the daze induced by family, bubbly, and the vast amounts of tamales that accompany my winter holidays, I have washed up on the shores of Long Beach, California, where almost 2,500 astronomers are gathered for the 213th meeting of the American Astronomical Society.

The biggest astro-nerd fest of the year is even bigger for 2009, because the meeting is playing host to the U.S. kick-off of the International Year of Astronomy, tied to the 400th anniversary of Galileo's telescope. Woot!

Having peeked at the press conference sked and session lists, I can tell there's some fun things in the works, including the imminent arrival of Galileo's *actual* original telescope to the U.S. But that comes later.

In a neat little cosmic alignment, the start of the meeting also coincides with the five-year anniversary of the twin Mars rovers Spirit and Opportunity, those plucky little workhorses that have been roaming the Martian landscape since 2004.

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Opportunity snaps dunes in Endurance Crater tinted blue in false color due to the presence of hematite-rich spherules known as blueberries
—Image courtesy NASA/JPL

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Carbonated Mars

Posted on December 19, 2008 | 0 Comments

Today folks using the Mars Reconnaissance Orbiter announced the discovery of a mineral called magnesium carbonate on Mars.

mars-carbonates.jpg

—Image courtesy NASA/JPL/JHUAPL/MSSS/Brown University

At first blush this seems like a pretty dry finding [pardon the pun]. What is a carbonate, and why should I care, you might ask.

When I tell you that it's a mineral that requires liquid water to form, and its presence in bedrock almost certainly means early Mars had liquid water, you might reply, Yeah, and?

Even among scientists, it's not gonna be news that Mars probably had bodies of water billions of years ago. What does make the finding cool is that carbonates dissolve readily in liquids with a low pH, aka, acids.

Deposits of carbonates dating back to early Mars therefore mean that water in at least some regions wouldn't have been very acidic, and therefore could have given rise to life.

All this was revealed today during a briefing at the fall meeting of the American Geophysical Union, and I plan to have a proper news piece about it posted tomorrow. But even with the infinite space of the Web, there's always some detail that has to be cut in news articles for the sake of getting to the point.

As luck would have it, I was seated next to a scientist who would relentlessly snicker every time a reporter asked a question about whether the new discovery would have any bearing on where to set down the Mars Science Laboratory.

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The holiday season has officially descended upon us, and many a child is eagerly waiting for that jolly red roundness with a snowy white cap to appear in the sky.

Meanwhile, anyone whose day job requires listening for and deciphering radio signals from Mars is probably only too glad that white-capped red ball has hidden itself behind the sun, and will stay that way through the end of 2008.

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Peek-a-boo!
—Image courtesy ESA

Last Friday Mars slipped into place behind the sun directly opposite to Earth observers, and over the next few weeks the red planet will drift through a line of sight very close to our stormy star.

This means that solar noise effectively blocks radio communications with the five craft now orbiting or actively exploring the face of Mars—and that means Mars mission engineers can take a bit of a breather.

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Next Mars Rover Held Up Until 2011

Posted on December 4, 2008 | 0 Comments

The fevered race to pick a landing site and a new name for the Mars Science Lab seems to have come to a screeching halt today, as NASA announced that the mission will have to wait until fall 2011 to launch.

mars-science-lab.jpg

—Image courtesy NASA/JPL

Citing technical issues and a too-tight testing schedule, NASA officials told reporters at a press briefing that the planned fall 2009 takeoff would have to wait, and the next launch window wouldn't come for another two years.

Aside from the delay in collecting a whole new swath of data about the red planet and its past climate conditions, the delay means that an already over-budget MSL will cost almost a billion more U.S. dollars than it was approved to spend.

At the briefing, NASA administrator Michael D. Griffin said that agency officials think they can get by without canceling any other NASA programs, although it's almost certain that some projects will see delays due to budget cuts.

Bloated costs have definitely been an issue for NASA before, and Ed Weiler, the agency's associate administrator for its science missions, was quick to point out the roller coaster ride that accompanied the early days of the Hubble Space Telescope.

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"Invisible" Auroras Mapped on Mars

Posted on November 21, 2008 | 0 Comments

Earth isn't the only planet that puts on a flashy light show.

earth-auroras.jpg

Last week Saturn was the exhibitionist, showing off a vibrant blue aurora around its northern polar hexagon. And Jupiter made the crowds cheer in 2007 with a shot of its "hyper-auroras" lighting up both poles.

—Photo by Bruce Dale/NGS

Not to be outdone, Mars is the headliner this week. A team using ESA's Mars Express orbiter used a combination of onboard instruments to track nine auroral emissions on the red planet.

Their data allowed the team to draw the first map of auroras on Mars, showing that the events coincide with regions on Mars that have the strongest magnetic fields.

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An artist's impression of auroras on Mars's night side
—Image courtesy M. Holmström (IRF)/ESA

Auroras on Mars are pretty unusual cases, because unlike Earth and the gas giants, Mars no longer has an internal dynamo generating a planet-wide magnetic field.

On Earth it's the magnetic field lines that channel streams of charged particles from the sun through the atmosphere, getting molecules all excited and causing them to emit light in the form of breathtaking auroral displays.

What Mars has are sections of the crust that were somehow magnetized, and the teams thinks it could be these regions that are attracting streams of particles, allowing auroras to occur.

The trick is that Mars's thin atmosphere is low in oxygen and molecular nitrogen, which are the elements that create visible light in Earthly auroras.

The Mars Express team's instruments see only in ultraviolet and so can't tell if any future human missions to Mars would be in for a show.

"There's now a large domain of physics that we have to explore in order to understand the aurorae on Mars," noted team member Francois Leblanc of France's Service d'Aéronomie.

After what sounded like some pretty exhilarating deliberations back in September, JPL announced today the final four candidate sites for landing the Mars Science Lab, NASA's next big rover bound for the red planet.

Sayonara, Miyamoto. Farewell, Nili Fossae. And so long South Meridiani. These three of the seven under consideration were voted off the proverbial island.

That leaves proponents of Eberswalde Crater, Gale Crater, Holden Crater, and Mawrth Vallis to duke it out and name a winner in time for the lab's planned fall 2009 launch.

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A false-color map of Mars shows the four candidate landing sites for the lab as well as the positions of NASA's current and previous missions to Mars.
—Image courtesy NASA/JPL-Caltech

Each remaining site has it's own unique set of features and local geology that would provide the roving lab with a different set of challenges.

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Will the Phoenix Rise Again?

Posted on October 29, 2008 | 0 Comments

Late last night the Mars Phoenix Lander put itself to sleep after experiencing a malfunction brought on by its deteriorating power supply.

The craft also unexpectedly switched over to its backup electronics and shut off one of its batteries.

The news was surely a disappointment, but not entirely a surprise, for NASA engineers, who had been expecting problems with the rugged lander right about now.

That's because the Martian arctic is moving into fall, and as the days get shorter, poor Phoenix has been losing its fire [in the form of sunlight to power its instruments].

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An image from the Mars Reconnaissance Orbiter shows the Martian north pole, with the Phoenix lander at about the 10 o'clock position
—Image courtesy NASA/JPL-Caltech/Malin Space Science Systems

It's not just the scientific equipment that needs power.

Mars is pretty frigid even in summer, and right now it doesn't get much warmer than -50 degrees Fahrenheit (-45 degrees Celsius) during the day, with overnight temperatures plummeting to -141 degrees Fahrenheit (-96 degrees Celsius).

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There's always a twinkle in a science writer's eye when real life imitates art.

In 2005 we had a snapshot of gases and dust around a star that seemed to be auditioning for the next Lord of the Rings film.

Then in 2007 there came the news that the universe could be packed with double-sunned planets like Star Wars' Tatooine.

Earlier this year a Mars orbiter sent in high-resolution shots of a body called Phobos, highlighting its massive Stickney Crater and its uncanny resemblance to the Empire's ultimate weapon.

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With apologies to Sir Alec Guinness, this time that is a moon—Phobos is the larger of the two known natural satellites orbiting Mars.

—Image courtesy NASA/JPL-Caltech/University of Arizona

Although it was discovered way back in 1877, Phobos has remained fairly enigmatic.

In the late 1950s, its odd orbit inspired Russian astronomers to suggest that the moon is a hollow shell, and an artificial one at that.

It took almost a decade to silence that offbeat theory, based on better calculations of the moon's orbit combined with new density measurements and eventually images from the Viking mission.

But Phobos still boasts some unusual characteristics, prompting much speculation about what the moon is made of and how it took up residence around Mars.

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Let It Snow [on Mars]

Posted on September 29, 2008 | 0 Comments

NASA's Phoenix Mars Lander has seen snow falling on the red planet!

One of the probe's atmospheric instruments detected ice crystals coming from clouds about 2.5 miles (4 kilometers ) above, although the flakes seem to have vaporized before they reached the ground.

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—Image courtesy NASA/JPL-Caltech/University of Arizona/Canadian Space Agency

This probably isn't a huge surprise, as we already knew Mars has glaciers and ice caps that grow and retreat with the seasons, so it was a good bet it still has a hydrological cycle of some sort. Still, way cool to be potentially seeing it in action.

NatGeo News reporter Anne Minard has the full scoop, including other data from Phoenix that bolster Mars's likely history as a wet and wild world.

The news got me to thinking: Which other bodies in our solar system have snowfall?

After a quick roll around teh Internets, it seems the answer depends on how one defines "snow."

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This summer's successful touchdown of, and subsequent science results from, the Phoenix Mars Lander have been setting the stage for NASA's next big payload bound for the red planet: the Mars Science Laboratory (MSL), due to launch next fall.

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An artist's rendition of the MSL
—Image courtesy NASA/JPL-Caltech

Even as I type, planetary researchers are gathered in Monrovia, California, to argue the scientific merits of seven proposed landing sites for the upcoming mission.

Figuring out where to position the craft might not seem like that big a deal, since the science lab is actually a rover—the biggest NASA has ever tried to land on Mars—that's designed for long-range mobility.

Unlike its famously long-lived but distance-challenged predecessors, the rovers Spirit and Opportunity, MSL will have the potential to travel up to 12 miles (19.3 kilometers) from its initial landing site.

But on a world more than 4,000 miles (kilometers) wide, location really will be key to the mission's ultimate goal of figuring out whether the red planet could ever have supported life.

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About This Blog

The moon
From dwarf planets to hot Jupiters, join NatGeo News space and tech editor Victoria Jaggard in a global discussion about all things extraterrestrial.


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