COSMOS
 
 
 
Mars water is heavy, Curiosity rover finds
Tuesday, 4 December 2012
 
by Bas den Hond

 
 
 
 
SAN FRANCISCO: Samples from a small mound of dust on Mars contain five 
times  as much ‘heavy water’, than you would find in a similar sample on Earth. 
The dust was analysed by the three soil experiments on board NASA’s latest  
rover on the planet, Curiosity. The _much-hyped_ 
(http://www.cosmosmagazine.com/news/6188/nasa-downplays-‘earth-shattering’-mars-finding)
  results of 
the experiments also included simple  organic compounds, the investigators 
announced at the Fall Meeting of the  American Geophysical Union in San 
Francisco. 
Water being a compound of hydrogen and oxygen, the measurement allows the  
calculation of how much normal hydrogen there is (with just a proton for a  
nucleus) compared to the heavy variant of the same element, deuterium, which 
has  a one-proton, one-neutron nucleus.  
UV light, low gravity lets hydrogen escape 
On Earth, just 0.016% of all hydrogen is heavy, and it is thought this was  
the percentage Mars started out with as well. But the thin atmosphere lets 
in UV  radiation from the Sun that splits water molecules into their 
constituent atoms.  
And because of the low gravity of the planet, hydrogen atoms escape easily  
into outer space, especially the lightest kind, normal hydrogen. This 
distilling  process results in a steadily rising radio of deuterium to hydrogen 
on Mars. 
That Mars air has been deuterium-enriched was already known – it was  
established by analysing how the Mars atmosphere transmitted light from the 
Sun.  
But according to Paul Mahaffy, who leads the Sample Analysis at Mars (SAM)  
experiment that Curiosity carries, knowing the precise deuterium content of 
Mars  water from soil samples can, in the future, be used to date them.  
Water that was incorporated into rocks or sediment long ago should still 
have  the deuterium-hydrogen ratio of that era.  
Dust measurement compare to other rovers 
The dust that Curiosity analysed came from a place on Mars called Rocknest, 
a  dust drift about 12cm (5 inches) in height that the rover encountered on 
its way  to Mount Sharp, its main destination. Rocknest was chosen because 
it looked very  much like the soil that earlier missions, Viking and the 
Spirit and Opportunity  rovers, had encountered.  
For these first measurements, in which soil was scooped up five times, were 
 first and foremost intended as a double check of all the instruments,  
duplicating earlier work as much as possible. 
Another goal of scooping up the dust was to ‘flush’ out of the system any  
possible remnants of Earth material in the equipment. Something may have  
survived the thorough pre-launch cleaning and get picked up by the sensitive  
spectrometers that Curiosity carries. If the measurements contain any such  
signal, it should be less present in later scoops of soil than in the 
earlier  ones. 
Carbon and chlorine also found 
Of the five scoops, four have now been analysed. Apart from the high 
content  of heavy water, the appearance of compounds of carbon and chlorine 
stands 
out in  the results.  
The chlorine is certainly a product of minerals in the soil, liberated as 
the  SAM experiment heats the sample, Mahaffy says. The carbon it then binds 
to could  be from complex organic molecules – which would be a very exciting 
find as it  would suggest Mars had once carbon-based life. But it could 
also simply be from  carbon dioxide, or even from carbon-containing molecules 
brought to the planet  by meteorites – or from contamination brought along 
from Earth. 
It will take many more measurements, again to do with discriminating among  
varieties of carbon with different masses, before anything definite can be  
announced, said Curiosity project scientist John Grotzinger.  
“We’re doing science at the speed of science. Curiosity works perfectly, 
we  have found organic compounds, but we don’t know whether these are Martian 
or  not," he said.

-- 
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