[ Back to EurekAlert! ] Public release date: 28-Aug-2013
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Contact: Tom Parkhill
tom@parkhill.it
39-349-238-8191
European Association of Geochemistry

We may all be Martians -- new research supports theory that life started on Mars

New evidence has emerged which supports the long-debated theory that life on Earth may have started on Mars.

Professor Steven Benner will tell geochemists gathering today (Thursday 29 Aug) at the annual Goldschmidt conference that an oxidized mineral form of the element molybdenum, which may have been crucial to the origin of life, could only have been available on the surface of Mars and not on Earth. "In addition", said Professor Benner "recent studies show that these conditions, suitable for the origin of life, may still exist on Mars."

"It's only when molybdenum becomes highly oxidized that it is able to influence how early life formed," explains Professor Benner, from The Westheimer Institute for Science and Technology in the USA. "This form of molybdenum couldn't have been available on Earth at the time life first began, because three billion years ago the surface of the Earth had very little oxygen, but Mars did. It's yet another piece of evidence which makes it more likely life came to Earth on a Martian meteorite, rather than starting on this planet."

The research Professor Benner will present at the Goldschmidt conference tackles two of the paradoxes which make it difficult for scientists to understand how life could have started on Earth.

The first is dubbed by Professor Benner as the 'tar paradox'. All living things are made of organic matter, but if you add energy such as heat or light to organic molecules and leave them to themselves, they don't create life. Instead, they turn into something more like tar, oil or asphalt.

"Certain elements seem able to control the propensity of organic materials to turn into tar, particularly boron and molybdenum, so we believe that minerals containing both were fundamental to life first starting," says Professor Benner. "Analysis of a Martian meteorite recently showed that there was boron on Mars; we now believe that the oxidized form of molybdenum was there too."

The second paradox is that life would have struggled to start on the early Earth because it was likely to have been totally covered by water. Not only would this have prevented sufficient concentrations of boron forming it's currently only found in very dry places like Death Valley but water is corrosive to RNA, which scientists believe was the first genetic molecule to appear. Although there was water on Mars, it covered much smaller areas than on early Earth.

"The evidence seems to be building that we are actually all Martians; that life started on Mars and came to Earth on a rock," says Professor Benner. "It's lucky that we ended up here nevertheless, as certainly Earth has been the better of the two planets for sustaining life. If our hypothetical Martian ancestors had remained on Mars, there might not have been a story to tell."

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Please mention the Goldschmidt Conference in any story from this press release

For more information, please contact Goldschmidt press officer, Tom Parkhill, email tom@parkhill.it Telephone: +39 349 238 8191 (Italian number).

Professor Benner is available at the following email: sbenner@ffame.org

Notes to editors:

1. The Goldschmidt Conference is jointly sponsored by the European Association of Geochemistry and the Geochemical Society. The annual, five-day event brings together around 4000 of the world's leading geochemists, covering topics as diverse as planetary formation, volcanoes, tectonics, climate change and oceans.

Goldschmidt2013 the 23rd Goldschmidt conference is being held in Florence between 25-30 August. It is managed this year by the European Association of Geochemistry (EAG). http://goldschmidt.info/2013/

2. Founded in 1985 to promote geochemical research, the European Association of Geochemistry (EAG) has now grown to a membership of over 3000. It is a not-for-profit organisation which provides a forum for the presentation and exchange of ideas between geochemists across Europe. EAG produces two journals Chemical Geology and Geochemical Perspective. http://www.eag.eu.com

3. The Geochemical Society (GS) was founded in 1955 with the aim of encouraging the application of chemistry to the solution of geological and cosmological problems. It now has over 3000 members and sponsors the journal Geochimica et Cosmochimica Acta. http://www.geochemsoc.org.

4. Professor Steve Benner began his career at Harvard and the Swiss Federal Institute of Technology in Zurich. He left a faculty position at the University of Florida in 2004 to found The Westheimer Institute of Science and Technology, named after his former PhD supervisor Frank Westheimer, and the Foundation for Applied Molecular Evolution. Benner's group was the first to synthesize a gene, creating the field of synthetic biology, and many of his advances in this field have had major significance in human medicine, for example in tests for HIV and hepatitis. His research seeks knowledge about the ancient origin of life, and looks for the essential, universal features of life by developing tests for life on other planets, by using paleogenetics to resurrect and study ancient proteins that may have belonged to long-extinct ancestors and by recreating pre-biotic chemistry to explain the chemical origin of life. Benner is also the founder of two successful companies, EraGen Biosciences and Firebird Biomolecular Sciences.



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