[meteorite-list] Scientists Discover How Atmosphere of Mars Turned To Stone

[Ron Baalke]

http://www.gla.ac.uk/news/headline_293811_en.html

Scientists discover how the atmosphere of Mars turned to stone
University of Glasgow
October 21, 2013

Scientists at the Scottish Universities Environmental Research Centre, 
the University of Glasgow and the Natural History Museum in London may 
have discovered how Mars lost its early carbon dioxide-rich atmosphere 
to become the cold and arid planet we know today. This research provides 
the first direct evidence from Mars of a process, called "carbonation" 
which currently removes carbon dioxide from our own atmosphere, potentially 
combating climate change on Earth.

It is widely recognised that accumulation of carbon dioxide in the Earth's 
atmosphere is contributing to global warming. The loss of carbon dioxide 
from the atmosphere of Mars, however, around 4000 million years ago is 
likely to have caused the planet to cool. So understanding how carbon 
dioxide was removed from the Martian atmosphere could lead to new ways 
of reducing the accumulation of greenhouse gases in our own atmosphere.

[Image]
This image is a false colour image of the Lafayette meteorite (sample 
code: USNM 1505-5) from a scanning electron microscope showing evidence 
of carbonation, with siderite (orange) replacing olivine (blue).

In a paper published in the journal Nature Communications, the research 
team describe analyses of a Martian meteorite known as Lafayette, sourced 
from the research collections of the Natural History Museum in London 
and the Smithsonian Institution in Washington. It formed from molten rock 
around 1300 million years ago, and was blasted from the surface of Mars 
by a massive impact 11 million years ago. Since its discovery in Indiana, 
USA, in 1931, Lafayette has been studied by scientists around the world.

This research focused on a carbon-rich mineral called siderite. Although 
found in Lafayette previously, the team discovered that the siderite had 
formed by the process of "carbonation", whereby water and carbon dioxide 
from the Martian atmosphere reacted with rocks containing the mineral 
olivine. These reactions then formed siderite crystals, replacing the 
olivine, and in so doing captured the atmospheric carbon dioxide and 
permanently stored it within the rock.

Lafayette provides direct evidence for storage of carbon dioxide in the 
fairly recent history of Mars, some time after 1300 million years. However 
as all of the ingredients for carbonation were present on early Mars, 
in the form of olivine, water and carbon dioxide, this reaction may explain 
how carbon dioxide was removed from the planet's atmosphere changing its 
climate from warm, wet and hospitable to life, to cold, dry and hostile.

Whilst this process also occurs naturally on Earth, and is the focus of 
research examining methods of permanently locking up carbon dioxide from 
power stations, the magnitude of the effect on early Mars indicates that 
it has the potential to be effective on a planetary scale.

Dr Tim Tomkinson of the Scottish Universities Environmental Research Centre, 
Research Associate at the University of Glasgow and lead author of the 
paper, said "Mars once had a thick atmosphere that was rich in water and 
carbon dioxide, and so this process of carbonation may help answer the 
mystery of why the Martian climate deteriorated around 4000 million years 
ago."

"This discovery is both significant in terms of the way in which scientists 
will study Mars in the future but also to providing us with vital clues 
to how we can limit the accumulation of carbon dioxide in the Earth's 
atmosphere and so reduce climate change."

Dr Caroline Smith, Curator of Meteorites at London's Natural History Museum, 
and co-author of the paper said, "Our findings show just how valuable 
meteorites from Museum collections like those we have here at the Natural 
History Museum really are. There is so much important and useful scientific 
information locked away in these rare rocks. Our study shows that as we 
learn more about our planetary next door neighbour, we are seeing more 
and more similarities with geological processes on Earth."