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Paris, 10 september 2012

Martian clays were not all formed by the action of liquid water

Discovered in 2005, the clays of the southern hemisphere of Mars are often considered to be evidence for the existence of liquid water on the planet at a period in the very distant past between 4.5 and 4 billion years ago. However, work carried out by a French-US team led by researchers at the Institut de Chimie des Milieux et Matériaux in Poitiers (CNRS/Université de Poitiers)(1) calls this interpretation into question. In an article to be published on September 9 on the website of the journal Nature Geosciences, they show that these clays were probably of magmatic origin. The many similarities between these Martian clays and clays of volcanic origin collected on the Mururoa Atoll support this hypothesis.

Mars' oldest rocks are found in its southern hemisphere: the crust of this region formed between 4.5 and 4 billion years ago. It is there that iron- and magnesium-rich clays were discovered in 2005. The presence of this type of mineral, considered to have originated from the decomposition of rocks through the action of liquid water, was interpreted as indicating that water was present on the Martian surface in the distant past. However, a team of researchers has shown that these clays are probably of magmatic origin.  

To lend weight to their hypothesis, the researchers studied basalts from the Mururoa Atoll (French Polynesia). These basalts are composed of well-formed crystals between which there are small spaces filled with a finely-crystallized material called mesostasis. This contains ferro-magnesian clays similar to those detected on Mars. The researchers have shown that these clays formed from residual water-rich magmatic liquids trapped in the empty spaces between the crystals. When the magma finally cooled, the constituents of these residual fluids precipitated, forming various minerals including clays. In this case, no aqueous alteration took place.

The scientists noticed that the Martian magma fulfilled all the conditions, in particular a high water and chlorine content, for this process to have been able to produce abundant clays on the basaltic surface of Mars. In addition, it is known that shortly after Mars' formation it was covered by a magma ocean, just like the early Earth.  During this period clays could have formed. On top of this, they also showed that the infrared spectrum of the Martian clays measured by the orbiters Mars Express and Mars Reconnaissance Orbiter is identical to that of the Mururoa clays.  

This work may have repercussions on the search for indicators of life on Mars. Although the presence of liquid water around 3 billion years ago is attested to by traces of rivers, lakes and alluvial fans, there is nothing to suggest that it existed at periods as remote as 4.5 to 4 billion years ago, as believed until now.  The period of time favorable to the emergence of life on Mars may have been much shorter than thought.  The Curiosity mission, which will explore part of the Gale crater on Mars, whose sedimentary formations are evidence of the presence of liquid water at a much more recent period, should make it possible to clear up a certain number of doubts. 
Clay

© A. Meunier and S. Riffaut

Particles of clay cover the surfaces of crystals in the subaerial basalt flow of the Mururoa Guyot (French Polynesia). Similar clays may have formed in the basaltic rocks of the Noachian crust on Mars (in yellow) which were probably not totally degassed. They could not have formed in Hesperian rocks (in green) which were totally degassed.


Notes:

(1) In France, this work also involved the Centre de Biophysique Moléculaire (CNRS). More about the Institut de chimie des milieux et matériaux de Poitiers: View web site

References:

Magmatic precipitation as a possible origin of Noachian clays on Mars. Alain Meunier, Sabine Petit, Bethany L. Ehlmann, Patrick Dudoignon, Frances Westall, Antoine Mas, Abderrazak El Albani and Eric Ferrage, Nature Geosciences, on line 9 September 2012.

Contact information:

Researchers l Abder El Albani l T +33 (0)5 49 45 39 26 l abder.albani@univ-poitiers.fr
Alain Meunier l T +33 (0)5 49 45 37 34 l alain.meunier@univ-poitiers.fr
CNRS Press Office l Priscilla Dacher l T +33 (0)1 44 96 46 06 l priscilla.dacher@cnrs-dir.fr


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