Related Experiment Video
Updated: Jun 26, 2026

Design and Use of a Full Flow Sampling System (FFS) for the Quantification of Methane Emissions
Published on: June 12, 2016
Strong release of methane on Mars in northern summer 2003
Michael J Mumma1, Geronimo L Villanueva, Robert E Novak
1NASA Goddard Space Flight Center, Mailstop 690.3, Greenbelt, MD 20771, USA. michael.j.mumma@nasa.gov
Abstract:
Living systems produce more than 90% of Earth's atmospheric methane; the balance is of geochemical origin. On Mars, methane could be a signature of either origin. Using high-dispersion infrared spectrometers at three ground-based telescopes, we measured methane and water vapor simultaneously on Mars over several longitude intervals in northern early and late summer in 2003 and near the vernal equinox in 2006. When present, methane occurred in extended plumes, and the maxima of latitudinal profiles imply that the methane was released from discrete regions. In northern midsummer, the principal plume contained approximately 19,000 metric tons of methane, and the estimated source strength (>/=0.6 kilogram per second) was comparable to that of the massive hydrocarbon seep at Coal Oil Point in Santa Barbara, California.
Related Concept Videos
Microbes and Climate Change
Microbes and Methanogenesis
Mass Spectrum
Mass Spectrometry: Branched Alkane Fragmentation
Mass Spectrometry: Long-Chain Alkane Fragmentation
Microbial Bioremediation of Hydrocarbons

