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Life on the Red Planet?

Posted by Science Oxford on December 19, 2009 | comments

Data from telescopic observations has shown Methane present in the Martian atmosphere. But not only is it present it is continually replenished, and there are only two possible sources, re­ac­tions be­tween vol­can­ic rock and wa­ter (cre­ating the meth­ane) or mi­crobes.
Read on to find out more:

Very little meth­ane gas can come to Mars from me­te­orites, sci­ent­ists have found. That leaves mi­crobes, they say, as one of just two re­main­ing pos­sible ex­pla­na­tions for me­thane’s ab­und­ance on the red plan­et.

Meth­ane, some­times al­so called marsh gas, is a flam­ma­ble, odor­less gas pro­duced by a range of bac­te­ria. The gas con­sists of car­bon atoms each of which has four smaller hy­dro­gen atoms cling­ing to to it.

Sci­en­tists an­a­lys­ing da­ta from tel­e­scop­ic ob­serva­t­ions and un­manned space mis­sions have found that Mars has meth­ane that is con­stantly re­plen­ished by an un­known source. With­out this re­plen­ish­ment, meth­ane would quickly van­ish from Mars be­cause a chem­i­cal re­ac­tion in the at­mos­phere, caused by sun­light, de­stroys it.

Re­search­ers had thought me­te­orites might be re­spon­si­ble for Mar­tian meth­ane be­cause when the rocks en­ter the plan­et’s at­mos­phere they un­dergo in­tense heat, caus­ing a chem­i­cal re­ac­tion that re­leases meth­ane and oth­er gas­es.

But the new stu­dy, by re­search­ers from Im­pe­ri­al Col­lege Lon­don, found that the vol­umes of meth­ane that could be re­leased in this way are too low to ex­plane the meth­ane hang­ing around the Mar­tian at­mos­phere. Pre­vi­ous stud­ies had al­so ruled out that the meth­ane might be de­liv­ered through vol­can­ic ac­ti­vity.

This leaves only two plau­si­ble the­o­ries, ac­cord­ing to the Im­pe­ri­al Col­lege re­search­ers: ei­ther re­ac­tions be­tween vol­can­ic rock and wa­ter cre­ate the meth­ane, or mi­crobes do so, probably as a byprod­uct of their me­tab­o­lism.

“As Sher­lock Holmes said, elim­i­nate all oth­er fac­tors and the one that re­mains must be the truth. The list of pos­si­ble sources of meth­ane gas is get­ting smaller and ex­cit­ing­ly, ex­tra­ter­res­tri­al life still re­mains an op­tion,” said study co-author Mark Seph­ton.

The find­ings are pub­lished Dec. 9 in the re­search jour­nal Earth and Plan­e­tary Sci­ence Let­ters.

The team say their study will help NASA and Eu­ro­pe­an Space Agen­cy sci­en­tists who are plan­ning a joint mis­sion to Mars in 2018 to search for the source of meth­ane. Now these agen­cy sci­en­tists can fo­cus on just two op­tions, the re­search­ers said.

The team used a tech­nique called Quantitative Pyrolysis-Fourier Trans­form In­fra­red Spec­tros­co­py to re­pro­duce the same sear­ing con­di­tions ex­pe­ri­enced by me­te­orites as they en­ter the Mar­tian at­mos­phere. The team heat­ed the me­te­or­ite frag­ments to 1000 de­grees Cel­si­us and meas­ured the gas­es re­leased us­ing an in­fra­red beam.

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