U.S. Geological Survey
Public Affairs Office

FEB. 13, 1997

USGS Scientist Describes Possibilities For Life On Mars

"There is mounting evidence that Mars is a water-rich planet that may have experienced warmer climates, and therefore, life, in the past,"according to Michael Carr, an astrogeologist with the U.S.Geological Survey in Menlo Park, Calif.

"Furthermore," said Dr. Carr, "early terrestrial life may have evolved in hydrothermal environments resembling those in Yellowstone Park and along mid-ocean ridges and such environments were likely common on early Mars."

Carr presented his assessment of the possibilities of life on Mars at the annual meeting of the American Association for the Advancement of Science, in Seattle, on Thursday, Feb. 13.

Carr said that both Earth and Mars experienced an early era of heavy meteorite bombardment that ended 3.8 billion years ago. Evidence for life is found in 3.8 billion year old terrestrial rocks, indicating that the Earth recovered remarkably quickly from this era of large and presumably sterilizing impacts. "We do not know what happened on Mars, but conditions on the two planets at that time could have been quite similar."

Carr said the prospects for life on Mars were given an additional boost last summer with the finding of organic compounds in Martian meteorites that have hit the earth, together with fossil-like structures and mineral assemblages that resemble some that have produced biologically here on Earth.

Carr pointed out that the U.S. has initiated a Mars exploration program that involves sending two spacecraft to Mars at every launch opportunity, or about every two years. He said the early focus of the program is to better understand Mars' climate history and distribution of water because of their importance for biology.

He briefly described the missions of the two U.S. spacecraft presently an their way to Mars: the Mars Global Surveyor that will map various properties of the surface from orbit, and Mars Pathfinder, that will land a small rover at the mouth of a large flood channel. Other missions will follow in the 1998 and 2001.

Carr said a major goal of those missions is to return samples to Earth later in the decade from "places that we judge will have the best chance of revealing whether there was life on Mars in the past."

FEB. 13, 1997

SEATTLE -- Subsurface life on Mars probably did exist and may still exist for the same reason it exists on Earth -- both these planets and many other planetary bodies in the solar system are made of similar stuff and provide similar conditions, a Cornell University astronomer said today (Feb. 13).

Microbes deep inside the Earth's crust get oxygen from rocks and use it to oxidize hydrocarbons that come streaming up from below, receiving energy by this process. It now seems probable that life evolved by such processes from the inside out, rather than commencing at the surface, said Thomas Gold, Cornell professor emeritus of astronomy. The same scenario is likely to be true for Mars and several other planetary bodies, he said.

Gold, a member of the National Academy of Sciences, described this theory at the annual meeting of the American Association for the Advancement of Science (AAAS) on Thursday, Feb. 13, at a session on "New Worlds and Old Worlds" in a talk called "Was There and Is There Life on Mars?"

His answer: Yes, there was and probably still is. "Microbial subsurface life has existed on Earth for billions of years and still does," Gold said. "It is very likely that we will find a deep, hot biosphere on Mars, as we have found on Earth, and probably on many other planetary bodies in our solar system."

Gold first proposed his theory in a 1992 paper, "The Deep, Hot Biosphere," in the Proceedings of the National Academy of Sciences (July 1992). In it he wrote that the Earth contains internal chemical energy sources in which microbes thrive, using hydrogen, methane and other liquids and gases that percolate up through cracks from the planet's interior, together with oxygen and other components of the local rocks. He suggested that such microbial life probably would be found in many areas below the surface of the Earth and will exist also on many other bodies, such as the moon, Mars, many asteroids between Mars and Jupiter, Titan (satellite of Saturn) and Triton (satellite of Neptune) and other satellites of the giant planets, and Pluto, the farthest known planet, where similar fluids have come up from below.

Further, he suggested in the 1992 paper that the known meteorites found on the Earth and identified as having come here from Mars should be examined for evidence of such microbial life. He also suggested that the search for such evidence of life would become a central issue in planetary research.

Last year one of these meteorites was found to contain what many scientists believe is evidence for such life. Gold considers this evidence to be particularly strong because the meteorite, Meteorite ALH84001, contains solids that are known on the Earth to be residues of such microbial activity.

The key to his theory, he said, is that petroleum has come up from great depth, not from biological sediments generated at or near the surface. The clearest evidence for that: helium.

The chemically inert gas, helium, is found to be strongly associated with petroleum all over the Earth, Gold said. This is true not only for great petroleum deposits, but also in detail in gases that are measured in thousands of locations at shallow depths. Yet no chemical process exists in which biological sediments would have concentrated this gas.

Helium is generated diffusely by the decay of uranium and thorium in the rocks. Gold is first to suggest that fluids, such as petroleum, that have washed through great distances in the rocks flush out the small quantities of helium that have accumulated along their way, increasing the helium concentration in such fluids.

"This is the only possible mechanism. Why else would helium be found together with petroleum?" Gold asks. "The association of helium with biological matter has not been accounted for in any other way."

If so, this requires that petroleum has come up from great depths, like 100 miles or more, rather than from just the upper four miles or so where there are biological sediments.

"In that case all the biological components that petroleum contains must have been additions it obtained later at the shallower levels from which we extract it," Gold said. What accounts for this biology? Microbial life, he said.

It was for this reason, Gold said, that he had to suppose that there was a huge amount of microbial life at all these shallower levels. "At the levels to which we drill, petroleum is a wonderful food for microbes," Gold said. "They thrive on that. With this combination we can understand why there is helium in petroleum and at the same time why there are biological molecules in it also."

And if it is true that hydrocarbons are cooked deep inside the Earth and then are mechanically washed up by geologic forces, where microbes then feed on them, then it's just a small step to wonder whether similar processes would not exist on other similar bodies in the solar system, he said.

"The Earth, then, has no particular prerogative to develop microbial life. Its subsurface is not unique. We know there are petrochemicals under the surfaces of many other bodies in the solar system, and in fact most other solid bodies have shown evidence of hydrocarbons."

The Martian meteorite ALH84001, which is thought to contain evidence of life, as announced in a paper in the journal Science (Aug. 16, 1996) by David McKay of NASA and others, has other similarities to Earthly subsurface life, Gold said.

"For example, unoxidized sulfur compounds and concentrations of small grains of the iron mineral magnetite, both not common in rocks, are found frequently around oil wells on Earth -- solid refuse left behind by microbial activity," Gold said. The meteorite ALH84001 has iron sulfide and magnetite, "very suggestive of the processes we see here," he said.

He added that the present or past surface condition on Mars is irrelevant to this problem. A huge impact was required to eject material from Mars, including the meteorites that have been found in Antarctica. Most of this ejected material would have come from deep inside the planet, from the crater this impact would have generated. A small distance down into such a crater, a mile or two, one would find liquid water and hydrocarbons, Gold said.

His 1992 suggestion on how to find evidence of life by spacecraft missions to Mars still holds, he said. There are areas on Mars where huge landslides have exposed material that once was at a depth of two miles or more, certainly into the depth range of liquid water. Why not select such locations for a robotic vehicle landing with a sample return capability? Gold asked. Now as a result of the meteorite investigation, NASA is planning to send probes on Mars missions to look for further evidence of life.

Said Gold: "As long as you think that life is possible only on planetary surfaces, the Earth is uniquely suitable. But when you talk about life deep below, the Earth is not unique at all. The deep, chemically supplied life may be common, not only in the solid bodies of the solar system, but throughout the universe."

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