Gullies in wall of Hale Crater. Credit: NASA/MROOut of about 40 robotic missions launched toward Mars since the early 1960's, about 17 of them have been successful (I say "about" to hedge my bets, because the "success" of some of those missions is a bit gray), and of all of those, three orbiters, two rovers, and maybe—MAYbe—one lander are still active.

Here's a quick status on the active ones:

Mars Reconnaissance Orbiter: The most recent arrival at Mars (2006), MRO's 5-year mission (hmmm—sound vaguely familiar?) is to study the history of water and climate on Mars, as well as to serve as a telecommunications relay for other spacecraft. Armed with a suite of powerful instruments to study the atmosphere, surface, and subsurface of Mars—including a camera, HiRISE, that can almost read the license plates on Martian automobiles—MRO has to date sent back more data than all other Mars missions combined. It's not been a glitchless flight, however: in 2009, MRO's computer reset itself four times for unknown reasons; the last reset, in August, was followed by a 4-month operational hiatus as Earth-side controllers performed some careful programming updates to help guard against effects of any future resets. MRO resumed operation in December.

Mars Odyssey 2001: NASA's 2001 Odyssey is still going fine after nine years—although the computer glitchiness out around Mars seems to be catching: Odyssey's computer put itself into a safe mode last November 2009 in response to a memory error. This was corrected and Odyssey has resumed doing science. Among Odyssey's major discoveries was the detection of huge expanses of water ice just under the surface of polar lowlands, and the surveying of deposits of water-related minerals in various locations around the planet.

Mars Express: Arriving at Mars in 2004, Mars Express became the European Space Agency's first mission to another planet, which was recently extended to 2012. Though the Beagle 2 lander component of the mission fell to Mars and was never heard from again, the Mars Express orbiter has sent back years of captivating images and important data, including the confirmation of methane in Mars' atmosphere (whose source is in all likelihood subsurface, and the origin of which—organic or inorganic processes—is being debated).

Mars Exploration Rover Opportunity: After six years of crawling around Meridiani Planum discovering chemical and geological evidence for past water on Mars, Opportunity is now on a long march to a large impact crater, which it will reach (if it can keep on running) in about two years. Currently, the rover has stopped to RAT out chemical and geological information from a rock called Marquette Island—the RAT is its rock abrasion tool, or rock grinder. Still going….

Mars Exploration Rover Spirit: Also still alive after six years—almost 25 times longer than it was planned to run—Spirit has been stuck in a sand bog for the last six months. With a couple of wheels on the fritz, Earth-side operators have been confounded in trying to free the robot—but Spirit has continued to make scientific measurements anyway…and in fact made a significant discovery in the course of trying to get unstuck.

Phoenix lander: Although it's been in the deep dark freeze of a Martian winter since November 2008, the Phoenix lander has an outside chance of survival. Now that light is returning to Phoenix's landing site, NASA is listening for the robot's radio signal, in case the return of solar power means that Phoenix will rise from the frost and live again! So far, no such signal….

Next up: The Mars Science Laboratory rover, "Curiosity."

NASA's rover Spirit has churned up sulfate minerals in the
attempt to free itself from loose soil.
(Credit: NASA/JPL/Cornell)Some robots are born to greatness, and some have greatness forced upon them by circumstance. NASA's Mars rover Spirit has recently fallen into the latter category by making an accidental discovery in the course of trying to free itself from a sand trap….

Has it been six years since the twin rovers, Spirit and Opportunity, landed on Mars to begin their careers? Just about—next month is their landing anniversary.

Both rovers have shown signs of wear and tear, but Spirit, in its exploration range in Gusev Crater, has had the harder knocks. In fact, Spirit has driven backward for a couple of years now, due to a wheel that stopped working and which it was forced to drag through the Martian soil—a robot's form of limping.

About six months ago, Spirit became bogged down in loose soil, spinning its wheels but unable to break free of the trap—not unlike what happened to my car in Death Valley one time…and Spirit can't call upon the assistance of a National Park Ranger with an SUV and winch to help….

Over the months of entrapment, Spirit's handlers on Earth have continued to make measurements with the rover's instruments while trying to free it from its soil trap by manipulating its wheels in different ways (probably not unlike some of the strategies I tried to get my car out of the sand). But to no avail (either for Spirit or my car). Alas, is Spirit destined to remain a stationary explorer until its lifetime finally comes to an end?

Perhaps—but as it turns out, this doesn't mean Spirit can't still make significant discoveries–like a recent one it in fact made. All that wheel spinning and grinding and rocking back and forth have chewed up the soil in which Spirit sits—and has broken through a layer of soil to expose a surprise hiding beneath: a crust of sulfate minerals.

Sulfates—compounds containing sulfur—can be formed in the presence of water, like boiling water or steam escaping from a hydrothermal vent. It may be that these sulfates formed in the distant past when the area was active with volcanism and hydrothermal steam vents. That was then.

This is now: the layer of sulfate (calcium sulfate) Spirit's churning wheels broke through is crusty—a property that may point to more recent water activity than the original sulfate-forming steam vents. Scientists think that the crust may have been formed by the seasonal shifting of water from the Martian polar regions when it warms up in its summer, sending the water toward the equator–where it can even fall out as snow. Then, soil beneath the layer of snow warms the bottom layer of ice and causes it to melt. In turn, the melt water seeps down into the soil, dissolving and carrying away water soluble iron sulfate and leaving behind the crust of calcium sulfate.

In one fell swoop trying to escape sure peril, Spirit appears to have uncovered clues about the nature of Martian water action in the distant past as well as more recent times.

As serendipitous as Spirit's entrapment is to this accidental discovery, it's even better: the rover is stuck square on the edge of a small meteorite crater, allowing it to compare the sulfate concentrations in the sulfate-rich crust and the more typical soil medium, side by side.

Way to go! That's the spirit!

Scene from the 1951 film The Thing From Another WorldFor decades, if not longer, we Earthlings have been collectively waiting for that definitive day when we make First Contact with life from somewhere else in the universe, whether it's a Closer Encounter of the Third Kind kind of advent or the detection of a microbe on another world. Are we there yet? Well, no, not yet–but we may be a healthy step closer to that day now.

On Monday, November 30th, 2009, NASA/Johnson Space Center announced that a recent study strengthens the argument that chemical and structural features in a Martian meteorite—ALH84001—may be evidence of fossilized microbial life on Mars from the distant past. While not absolutely conclusive that the meteorite bears the remains of ancient Martian life, the results of the study show that alternate, non-biological explanations for some of the meteorite's properties are not consistent with new findings.

Meteorite ALH84001, discovered in Antarctica in 1984 and chemically identified as having originated on Mars, hit the news in 1996 when researchers hypothesized that microscopic features and chemical constituents in the rock could possibly be the fossilized remains of ancient Martian microbial life. The hypothesis was controversial among scientists, and alternate, non-biological processes were offered by opponents as possible explanations for the meteorite's features.

The recent reexamination of the meteorite was focused on one of the leading non-biological explanations for the existence of magnetite crystals in the sample. Magnetite is an iron-bearing, magnetic mineral that can be produced both biologically and through inorganic processes. Some forms of life on Earth—including microbes–produce magnetite crystals in their cells that help them orient to Earth's magnetic field.

The NASA/JSC team that performed the new analysis of ALH84001 concluded that new data on the magnetite crystals, obtained with more powerful analytic instrumentation than used in the 1996 study, are not consistent with the leading non-biological explanations. This, they argue, strengthens the biological explanation for the origin of the magnetite.

The new analysis also obtained scanning electron microscope data that yielded more detail on shapes within the alleged microbe fossils. The new shapes that emerged from the data closely resemble shapes within Earthly microbe fossils—further strengthening the hypothesis that the meteorite contains fossils of life, and thus that life at one time existed on Mars.

The evidence for the possibility of life on Mars, past or present, has been growing over the past decade, or longer—evidence that Mars was once much warmer and wetter than it is now, and that it had rivers, lakes, and possibly oceans of water, making it an environment possibly conducive to the formation of life. We have also detected methane rising out of the soil of Mars, which some suggest could be a byproduct of current biological activity, underground.

NASA will continue to examine the Martian meteorite, focusing their study on further detailing the structures of alleged microbe fossils and possible chemical signatures of life that remain in the rock.

So, we're still waiting for the day—but with all the tantalizing clues emerging from our exploration of Mars and the Martian meteorite, it feels very much like that day is somewhere on the horizon. But, wouldn't it be ironic if we were to make the first definitive detection of extraterrestrial life right here on Earth, with evidence that's been just laying around since before the beginning of human civilization?

Geek Out by taking the Mars Survival Challenge

Forget the challenging landscapes of the Arctic or Everest; if you want a true survival test, how about Mars? Our red neighbor has inspired thousands of intrepid explorers (and a number of awful movies) to formulate colonization plans. With a little help from Google Mars, you can choose plot near all the important landmarks: Valles Marineris, Olympus Mons, or even the famous northern polar ice caps.

Thanks to our friends at the Lawrence Hall of Science, you too can help the colonization effort. At their Geek Out event on 11/18, you’ll be able to design your own Mars Base. There will be experts on hand from the SETI Institute and NASA to provide some info on the Martian landscape and what it takes to survive there.

You’ll be able to videotape your landscape to share with the rest of the universe. Who knows, the first ever Martian colony could be named after you!

This is the 2^nd LHS Geek Out event, a new monthly science series for adults. The evening will be full of interactive science, music, and cocktails. There is also a free shuttle from the Downtown Berkeley BART to the museum. For a primer, check out this video from the 1^st Geek Out event.

LHS Geek Out: Mars Survival Challenge
When: Wednesday 11/18, 7-10 PM
Where: Lawrence Hall of Science, Berkeley
Cost: $10, $8 for members and UC Berkeley Students
Details: Come to Lawrence Hall of Science, grab a drink and a friend, and get ready for some downright nerdy fun. All events include full access to exhibits, a cash bar, hors d’oeuvres, and of course the best view in the East Bay. Program is for adults only.

Block Island—a half-ton meteorite found on Mars by NASA's
Opportunity rover.Image credit, NASA/MER OpportunityEver been driving down a lonely desert highway when you suddenly glimpse something in the corner of your eye that makes you think, "What was that?!" You brake, tires screech, you spin the wheel and make a wild U-turn, cutting into the shoulder and leaving a rooster-tail of dust as you floor the gas to get back to what you thought you saw….

Okay, dramatic desert car scene ended. That would be the Hollywood movie version of what NASA's Mars Exploration Rover Opportunity did recently, on the lonely desert highway that it's scouting on Mars.

On its determined long trek from Victoria Crater to the larger Endeavour Crater (a 12-mile span that Opportunity has completed about one fifth of over the past year), the rover passed by an X-box-sized block of iron that presented the appearance of a meteorite. It snapped a picture in passing, which was eventually transmitted to Earth and examined. By this time, Opportunity had already traveled about 180 meters beyond the block (dubbed "Block Island"). This is when the rover was commanded to backtrack all the way to the find (though it's doubtful it worked up a rooster tail).

Upon returning to Block Island—quite obviously an iron-nickel meteorite by appearance alone, but whose composition was confirmed by the rover's alpha particle X-ray spectrometer instrument—Opportunity took more pictures, including extreme close-ups with its microscope camera, which revealed surface patterns similar to those found on Earth iron-nickel meteorites that have been exposed to long-term weathering by wind and sand.

As interesting as stumbling upon a half-ton meteorite on the dusty plains of Mars' Meridiani Planum is, what this particular chunk of weathered iron is telling scientists sparks the imagination. In a nutshell, given the thinness of Mars' current atmosphere, scientists wouldn't expect a meteorite of this size to survive impact intact, at the speed it would be going. One of the possible explanations for Block Island's rock-houndable state is that when it fell to Mars, Mars' atmosphere was substantially thicker than it is now.

Further examination of the meteorite may reveal clues as to how long ago it fell through Martian skies. Evidence that Mars' atmosphere was warmer and thicker in the distant past, as well as the possibility that there was liquid water on the surface, has been mounting over the years. The age of this meteorite-fall could shed more light on the history of Mars' environment. If it fell billions of years ago, Block Island would weigh in as more evidence to support our current suspicions. If, however, we find that it fell more recently, then this could indicate that the atmosphere was more substantial later in Mars' history than we thought.

Imagine, if you will, a Mars that looks even more Earthlike than it does now: seas of water with waves rolling into shorelines, great clouds sending downpours of rain and snow onto mountains and plains, streams and rivers snaking through the landscape. Maybe, maybe, even some form of life?

All that from a rock? Yes, rocks talk, if we listen.

Mars as seen through Chabot Space & Science Center’s 20-inch telescope near the 2003 close encounter. Credit: Conrad Jung/Chabot Space & Science CenterIf you take away no other message from this blog, just remember this: the planet Mars is NOT passing close to Earth this August and will NOT appear as large as the Full Moon. There; disclaimer delivered.

As August approaches, the ghost of Mars returns to haunt us, in the form of emails and phone calls from people asking if it's true that Mars is about to get closer to Earth than it has been in a gazillion years—so close that it will look as big as the Full Moon.

I say "ghost" because it simply isn't true, here in 2009. I say "haunt" because, six years ago, it was true—at least, partly.

The time: August 27, 2003. The scene: Earth and Mars. The event: Mars is coming into opposition—the time when Earth passes directly between Mars and the Sun, and consequently Mars is closest to us and at the opposite point in the sky from the Sun—hence "opposition." A routine encounter, one that happens about every 2.2 years. But what's different with this Mars opposition is the distance between Earth and Mars at closest approach: the two planets are closer together than they have been in a very long time: a bit less than 35 million miles.

This was a very big deal, you may recall. We remember it very well at Chabot: On one of the evenings that weekend, we had 2000 people who came up to see Mars through our telescopes…. A close opposition is the best time to see a planet, and this was closer than average for Mars by maybe 10 million miles. (It was at another very close opposition of Mars when Percival Lowell made his famous "Martian canals" observations and Martian civilization hypothesis, back in 1894.)

At the time of the 2003 opposition, there were a lot of reports—emails, websites, blogs—flying around describing the event, in some cases with exaggeration. One exaggeration is the amount of time since the previous closest encounter with Earth. Different accounts suggested a thousand years, ten thousand years, even one hundred thousand years. Technically this may have been true, if one were calculating down to the inch. Practically speaking, however, the opposition in 1924 was almost as close, by a difference of only 12,000 miles (one and a half Earth diameters).

The other (gross) exaggeration was a statement made that at opposition Mars would appear as large as the Full Moon. That would be spectacular! However, at some point a piece of information was lost from the original message: the part about needing to look at Mars through a telescope to achieve the advertised view.

The final piece of information missing from that message—which gave birth to the annual Mars Hoax –was the year, 2003, omitted along the way and making every August 27th a day to view the splendor of Mars in all its glory. But, alas, the ghost of Mars.

For the record, the next extra-close opposition of Mars will occur on August 15th, 2050, when it will be only 200,000 miles farther than the 2003 near-miss….

Google Mars view from the slopes of the Olympus Mons caldera. Credit: Google Earth

I was sitting at my computer the other day, quietly exploring minute details of the surface of planet Mars, when I realized once again that in my lifetime planetary exploration has gone from telescopic-view-only to robotic rovers poking microscopes close up at Martian geology!

Did I say quietly exploring the surface of Mars? Yes I did—and you can, too. First of all, if you're not familiar with Google Earth, please go and google Google Earth and get your free download today (this is NOT a sales pitch!). A modestly powered computer with a decent graphics card is all you need to probe every nook and cranny of planet Earth, sometimes to the detail of spotting people walking in the streets….

But there's a magic button on Google Earth (it looks like planet Saturn, for some reason) that instantly transports you to planet Mars—Google Mars, that is. It's a simple button click to explore Mars, Google Earth style.

This detailed digital Mars has been created with all of the data collected by the fleet of robots we've sent—from Viking to Mars Global Surveyor to Mars Odyssey to Mars Express to Mars Reconnaissance Orbiter (MRO), and of course Pathfinder, Phoenix, and the Mars Exploration Rovers, Spirit and Opportunity.

First on my itinerary was Olympus Mons, that extinct, Arizona-sized shield volcano that rises 15 miles above the average global terrain. Swooping into the San Francisco Bay-sized caldera, I got a sense of what it would be like to be there, standing on the caldera rim. There were even strips of super-high resolution imagery provided by MRO's HIRISE camera, allowing me to hover maybe a hundred feet above the ground and see rocks and piles of sand!

Next on the list had to be that other famous gargantuan feature, Valles Marineris, the "Grand Canyon of Mars" which, if it were moved to Earth, could stretch from Oakland, California to New York City—putting Grand Canyon National Park within a day's drive of anyone in the US…. Google Earth/Mars has a flight simulation mode that allows you to pilot an aircraft over and through (and into) the terrain.

Like a kid in a science supply shop (okay, that's the kind of kid I was), next I hopped on up to the landing site of NASA's Phoenix lander, on the wide flat plains near the Northern Polar Ice Cap. Yup, those plains are really flat. To my delight, I found that someone had inserted a panoramic picture taken by the orbiting MRO spacecraft when it captured Phoenix descending through the atmosphere.

Onward, planetary explorer…. I had to feel—not just see, but feel—what the landscapes that Spirit and Opportunity have been exploring for 5 years are like. On Spirit's side of the globe, Gusev Crater, I poked about the Columbia Hills, following in the tracks of the robot. Over at Opportunity's digs, I dropped into Victoria Crater, enveloping myself in "Street View"-style panoramas that almost set my feet down on Martian soil.

Okay, I could go on telling you about my adventures on Mars for days—but since you can do it yourself now, I'll let you go to it. Have fun, and send back a postcard! (Which, by the way, you can do from Google Mars….)

NASA/Mars Reconnaissance Orbiter; Fans of dark dust on Mars'
southern ice cap, apparently blasted from beneath the ice
by thawing carbon dioxide."

It's spring again, that time of year when my thoughts return to…blasts of carbon dioxide gas jetting up from beneath the frigid layer of dry ice below, carrying rusty red dust in plumes that jet toward the pale skies….

At least, that's what happens at the polar ice cap on the planet Mars. I'd sure love to be there to see it, even if there are no flowers in bloom. Still, there seems to be plenty of "blossoming" going on….

NASA's Mars Reconnaissance Orbiter—the spacecraft with that high powered camera that could spot a beach ball on Mars' surface—has captured images of the aftermath of some of Mars' springtime polar action. Appearing as dark fan-shaped bursts strewn across the thinning springtime polar ice, these features are explained as plumes of Martian dust that have settled after being blasted into the air by releases of gas pressure from under the surface of the ice.

To describe what's going on, let me paint a picture of the Martian polar region as it emerges from the deep freeze of winter into spring.

Mars' year is almost twice as long as Earth's—and so too are its seasons. Winter at the southern pole of Mars lasts almost six months. In that time, the normally freezing temperatures on the Red Planet plummet to as low as -225 degrees Fahrenheit at the pole. During this time, Mars' permanent water ice cap acquires a layer of frozen carbon dioxide (dry ice) on top, formed from carbon dioxide freezing directly out of the atmosphere.

This seasonal dry ice cap also forms around the edges of the water ice cap, covering adjacent ice-free surfaces as well. The carbon dioxide ice cap may grow to as much as a meter thick.

Then, as spring approaches and the ice cap gradually comes out of the dark and receives more and more sunlight, it begins to warm up (though don't get the impression that it is ever "warm" anywhere on Mars' surface! Air temperatures recorded by the Viking landers in Mars' more temperate latitudes was barely ever higher than 1 degree Fahrenheit). Spring Equinox in Mars' southern hemisphere was on December 26th.

As the layer of solid carbon dioxide heats up, its ices turn to gas, both at the top of the layer and beneath it as well. The gases forming underneath build up pressure, which seeks a path to escape. Evidently the pressurized carbon dioxide gas can actually carve channels in the Martian soils under the ice as it flows—said channels have been seen in the past after the seasonal ice cap dissipates entirely.

When the gases find a weak point in the ice, they can erupt upward, bursting into the air, sometimes carrying dust with it. The dust rockets skyward and is blown by prevailing winds, settling out on the ice in great dark fans—which is what Mars Reconnaissance Orbiter has shown us.

Ah, to be on Mars in springtime….

Methane concentrations revealing a plume in Mars' northern
hemisphere during its summer season. Credit: NASAMethane on Mars? Really? What does that mean?

We've known about the existence of methane gas on Mars for several years now, from independent observations.  Further observations have led to the detection of "plumes" or clouds of methane gas apparently emanating from specific locations on Mars.  One plume is estimated to contain 19,000 metric tons of the stuff.

Why is this exciting news? If you know anything about the source of most of Earth's atmospheric methane gas, you already know the answer:  possible life.  Not, I should say, necessarily life on Mars, but maybe a strong piece of evidence in that direction.

On Earth, methane (CH₄) is produced by living organisms—mostly by the activity of microbes, but some by the digestive processes in larger organisms (yes, like humans, and cows).  Methane is the major constituent of natural gas, which fuels gas powered ovens and heaters in homes, as well as natural gas power plants.  Methane is also produced by decaying organic matter—that's where "swamp gas" comes from.

On Mars, methane gas cannot exist for long in the atmosphere; it is relatively quickly broken down by solar radiation.  So, the methane detected in Mars' atmosphere must be replenished by something, continually.

So the big question right now is, where is the methane coming from? Under the surface of Mars, almost certainly.  By biological processes—life—underground? Could be.  By non-biological means? Could be, too; methane can be produced through inorganic chemical processes.  We don't know yet.  The next step in finding out more will be the Mars Science Laboratory, a large rover scheduled to be launched to Mars sometime in the near future.

In one form or another, humans have been trying to see, or find, life on Mars for a long time.  Percival Lowell squinted at Mars' small, blurry disk through his 24-inch telescope in Flagstaff, and perceived markings he saw to be vast canal complexes, ostensibly built by a desert Martian civilization thirsty for water harvested from their planet's polar ice caps. This led to much of the science fiction relating to life on Mars in the 20^th Century.

Earth-bound telescopes noted seasonal changes in Mars' color and brightness, and some attributed this to possible seasonal growth of Martian vegetation—though it was later found that these variations were the effects of seasonal planet-wide dust storms.

The Viking landers' primary mission in the 1970's was to search for life.  They didn't find any by scratching around Mars' surface and testing the soils there.

The 1990's saw the controversy over microscopic structures in meteorites found on Earth but determined to have originated on Mars.  Some argued that these structures were fossils of Martian microbes that lived on Mars long ago.  Whether these findings were in fact fossils and not just geologic structures was never conclusive.

The determination that liquid water once flowed on the surface of Mars, and still exists under its surface at least as ice, is pretty much scientific fact today.  Evidence of past liquid flows have been imaged and mapped from space, and the Phoenix lander found water ice in the north polar regions last year.  And there's the rover Opportunity that has confirmed gray hematite, a mineral that forms in the presence of water.

It's almost certain that there are no Martian cows grazing the rusty desert plains out there.  But there seems to be a lot of evidence for the possibility that something is going on below Mars' surface—perhaps the presence of liquid water, perhaps the presence of some form of life.  We don't know yet, but it sure feels like we're onto something here….

Terrestrial snow at Chabot on December 16, 2008
Photo by Craig CoryellDriving to work today, I was amused to notice that the raindrops falling on my windshield were a bit grainy–and getting more so the higher up the hill I drove. I starting to think, is it starting to sleet? By the time I reached Chabot–at 1500 feet elevation–the precipitation had turned to bona fide snow!

This is quite unusual for the Oakland Hills, of course. In the ten years I've worked here, this is the second, maybe third, dusting I've witnessed. I recall the great freeze of '74, when it actually snowed in Oakland close to sea level—that's the year all the eucalyptus in the hills froze and died.

My mind wandered—pretty far out in space (an occupational hazard at Chabot). I started thinking about all the recent news and discoveries from around the Solar System, my thoughts guided by the fat white flakes drifting down all around the observatory domes.

Last September, NASA's Mars Phoenix Lander detected snow falling high in the atmosphere–about 4 kilometers high. This Martian snow, however, quickly evaporated in Mars' thin, dry air, never reaching the ground. Phoenix used a laser probe to make the detection–so we don't actually have picture to look at!

Snows of the Solar System may also fall out of the plumes of "cryovolcanoes"–the frigid outer Solar System's version of volcanism (may it live long and prosper). On moons such as Saturn's Enceladus and Neptune's Triton, plumes of material have been detected spouting from fissures and cracks–probably fueled by heat generated by tidal forces from their parent planets.

On Enceladus, the geyser plumes contain water vapor and ice crystals, and are believed to come from subsurface lakes of "warm" water (32 degrees Fahrenheit–in other words, ice water… but that's a veritable hot spring, or magma chamber, on a cold moon like Enceladus!).

The ice crystals in the geysers' plumes mostly fall back to Enceladus–maybe in a diffuse fall of "snow" across the globe? I'm waiting for those pictures…

Saturn's large moon Titan is speculated to possibly have a form of cryvolcanism, though no direct detection has yet been made. Still, any water vapor that might erupt from a Titanian cryovolcano might be expected to fall in a form of snow….

Triton, much farther from the Sun than Saturn, is even colder than Enceladus. In fact, it's been called the coldest measured surface in the Solar System, at -391 degrees Fahrenheit. Here, nitrogen freezes solid. Triton cryovolcanoes, or geysers, may be partially solar-heated, but tidal heating within Triton is probably dominant. Triton's geysers spout nitrogen gas and dark material, which falls across the landscape in dark streaks and lighter deposits of frozen nitrogen–a form of extreme cryo-snow, to my imagination!

Now, are you as cold as I am just thinking about it? Time for a cup of cocoa…