PIA16461: Potential Sources and Sinks of Methane on Mars


Potential Sources and Sinks of Methane on Mars

Caption:

If the atmosphere of Mars contains methane, various possibilities have been proposed for where the methane could come from and how it could disappear.

Potential non-biological sources for methane on Mars include comets, degradation of interplanetary dust particles by ultraviolet light, and interaction between water and rock. A potential biological source would be microbes, if microbes have ever lived on Mars. Potential sinks for removing methane from the atmosphere are photochemistry in the atmosphere and loss of methane to the surface.

Background Info:

Researchers are using Curiosity's 10 instruments to investigate whether areas in Gale Crater ever offered environmental conditions favorable for microbial life. JPL, a division of the California Institute of Technology in Pasadena, manages the project for NASA's Science Mission Directorate, Washington, and built Curiosity. The SAM instrument was developed at Goddard with instrument contributions from Goddard, JPL and the University of Paris in France.

For more information about Curiosity and its mission, visit: http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl .

Cataloging Keywords:

Name Value Additional Values
Target Mars
System
Target Type Planet
Mission Mars Science Laboratory (MSL)
Instrument Host Curiosity Rover
Host Type Rover
Instrument Sample Analysis at Mars (SAM)
Detector
Extra Keywords Atmosphere, Color, Comet, Crater, Dust, Methane, Ultraviolet, Water
Acquisition Date
Release Date 2012-11-02
Date in Caption
Image Credit NASA/JPL-Caltech, SAM/GSFC
Source photojournal.jpl.nasa.gov/catalog/PIA16461
Identifier PIA16461