A Martian Baltic Sea

by | Sep 9, 2004 | Astrobiology and SETI

A University of Colorado study, using data from the Mars Global Surveyor and Mars Odyssey orbiters, has concluded that the area surrounding the rover Opportunity’s landing site once contained a huge body of water — up to 330,000 square kilometers. That makes this Martian sea comparable to the Baltic or, as investigator Brian Hynek of the Laboratory for Atmospheric and Space Physics puts it, ‘all of the Great Lakes combined.’

Hynek’s paper on the Martian sea (“Implications for hydrologic processes on Mars from extensive bedrock outcrops throughout Terra Meridiani”) appears in the September 9 issue of Nature, and you can find CU’s press release on his work here.

The physicist used the thermal emission imaging system on-board Mars Odyssey to infer the size of rocks, studying how larger and smaller particles change temperature at different rates in daylight and at night. His thermal maps show wide areas of bedrock, and tell him that water once extended far beyond the landing area. To quote the press release:

Hynek speculated that if the outcrops at the landing site are the result of sea deposition, as believed, the body of water must have been deep enough and persisted long enough to build up sediments roughly one-third of a mile deep. “For this to occur, the ancient global climate of Mars must have been different from its present climate and have lasted for an extended period,” Hynek wrote in the Nature paper.

This is good news for the hunt for life, at least in microbial form, and implies that conditions were once far more favorable for its formation.

0 Comments

Now Reading

Charter

In Centauri Dreams, Paul Gilster looks at peer-reviewed research on deep space exploration, with an eye toward interstellar possibilities. For many years this site coordinated its efforts with the Tau Zero Foundation. It now serves as an independent forum for deep space news and ideas. In the logo above, the leftmost star is Alpha Centauri, a triple system closer than any other star, and a primary target for early interstellar probes. To its right is Beta Centauri (not a part of the Alpha Centauri system), with Beta, Gamma, Delta and Epsilon Crucis, stars in the Southern Cross, visible at the far right (image courtesy of Marco Lorenzi).

Recent Posts

On Comments

If you'd like to submit a comment for possible publication on Centauri Dreams, I will be glad to consider it. The primary criterion is that comments contribute meaningfully to the debate. Among other criteria for selection: Comments must be on topic, directly related to the post in question, must use appropriate language, and must not be abusive to others. Civility counts. In addition, a valid email address is required for a comment to be considered. Centauri Dreams is emphatically not a soapbox for political or religious views submitted by individuals or organizations. Human comments only, please -- cut and paste from AI will not be acceptable. A long form of the policy can be viewed on the Administrative page. The short form is this: If your comment is not on topic and respectful to others, I'm probably not going to run it.


Advanced Propulsion Research

Beginning and End

Archives