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….

NASA's MESSENGER spacecraft at Mercury-artist concept.

Photo by: NASA

I've been waiting for the "whole story" on Martian ice at the Phoenix lander site to unfold more completely, but the chemical analyses have not yet run their full courses-so I've decided to widen the focus on this blog to give a status report on current active robotic exploration of planets going on around the Solar System.

Limiting my scope to only planetary spacecraft, the list is still respectable. In no particular order, here's the round-up:

Spirit: Mars Exploration Rover Spirit's activities on the Martian surface have been reduced to save on power, but the robot remains alive. With the arrival of Martian winter, Spirit spends more power running heaters to keep key electronic and power equipment healthy. Spirit remains in the giant Gusev Crater, where it will spend its entire life on Mars.

Opportunity: Exploring a much smaller crater of its own, Victoria Crater-Spirit's twin, Opportunity, continues its investigation of the rock layers of Mars' geological history. As of June 10, Opportunity has clocked in at 7.26 miles of total "roving" on Mars, since its landing back in 2004.

Phoenix: The brand-spankin'-new Mars Phoenix lander has been digging into one of Mars' greatest scientific mysteries: water. Detailed chemical analysis of samples taken at Phoenix's site near the northern polar ice cap is underway, but the big question– is Phoenix standing on frozen Martian water– has been answered: yes.

Mars Reconnaissance Orbiter: The newest orbiter in the Martian fleet continues to send back its extreme-high-resolution imagery and its revealing chemical measurements, as well as to serve as a high-speed data and communication relay for other Mars-exploring robots.

Mars 2001 Odyssey: Credited with detecting the massive amounts of frozen water in Mars' northern hemisphere-the same ice that the Phoenix lander is now scraping at, Mars 2001 Odyssey continues its surveillance of Mars' chemistry and atmosphere.

Mars Express: The European orbiter that launched the ill-fated Beagle II lander has continued on a respectable career of exploration in its own right. Mars Express also helped support the landing of the Phoenix.

Cassini: Saturn's first robot-in-residence, Cassini, has concluded its initial 4-year mission and is now continuing on an extended mission. Cassini has given us unprecedented close-up images and measurements of many of Saturn's stunning moons, its complicated ring system, and the swirling, aurora-touched cloud formations of Saturn itself.

MESSENGER: The first spacecraft to visit the little-understood Mercury since 1975 made its first flyby of that planet last January, and will settle into a permanent orbit in March 2011. Even the few pics it snapped as it hurled by gave us far more detailed images of Mercury than ever before.

New Horizons: Launched a couple years ago on its outward bound, meteoric flight to Pluto, New Horizons has already performed some exploration duty, capturing images and data of Jupiter, Jupiter's volcanic moon Io, and Jupiter's long magnetic "tail." Now in "cruise mode," this little robot will fly past Pluto (dwarf planet; king of the Plutoids) in July 2015.

Voyagers 1 and 2: Do you remember the remarkable voyages of discovery made by the Voyager spacecraft, both launched in 1977? Since completing their primary missions of flying by the Gas Giant planets (Voyager 1 at Jupiter and Saturn, Voyager 2 at all four), these two veterans have continued to operate and send information back to Earth, and are now about 3 times more distant from the Sun than Pluto.

That's the wrap. If I missed anyone, my apologies!