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Mars methane detection and variability at Gale crater

Authors :
Susanne P. Schwenzer
Christopher R. Webster
Tobias Owen
Mark T. Lemmon
Javier Martin-Torres
Sushil K. Atreya
Michael A. Mischna
John Bridges
P. Douglas Archer
G. Flesch
Patrice Coll
Kenneth A. Farley
Ralf Gellert
Alexander A. Pavlov
Daniel P. Glavin
Christopher P. McKay
Andrew Steele
Jennifer L. Eigenbrode
Paul R. Mahaffy
Timothy H. McConnochie
Rafael Navarro-González
John E. Moores
Charles Malespin
Pamela G. Conrad
Brad Sutter
Caroline Freissinet
María Paz Zorzano
Lance E. Christensen
Pierre-Yves Meslin
Source :
Science. 347:415-417
Publication Year :
2015
Publisher :
American Association for the Advancement of Science (AAAS), 2015.

Abstract

Of water and methane on Mars The Curiosity rover has been collecting data for the past 2 years, since its delivery to Mars (see the Perspective by Zahnle). Many studies now suggest that many millions of years ago, Mars was warmer and wetter than it is today. But those conditions required an atmosphere that seems to have vanished. Using the Curiosity rover, Mahaffy et al. measured the ratio of deuterium to hydrogen in clays that were formed 3.0 to 3.7 billion years ago. Hydrogen escapes more readily than deuterium, so this ratio offers a snapshot measure of the ancient atmosphere that can help constrain when and how it disappeared. Most methane on Earth has a biological origin, so planetary scientists have keenly pursued its detection in the martian atmosphere as well. Now, Webster et al. have precisely confirmed the presence of methane in the martian atmosphere with the instruments aboard the Curiosity rover at Gale crater. Science , this issue p. 412 , p. 415 ; see also p. 370

Details

ISSN :
10959203 and 00368075
Volume :
347
Database :
OpenAIRE
Journal :
Science
Accession number :
edsair.doi.dedup.....37b6657a8b524288c94ebe9c696105da