• → European Space Agency

    • About Science & Technology

    • For Public

    • For Educators

    • ESA

    • Science & Technology

    • Mars Express

    • Missions
    • Show All Missions
    • Mission Home
    • Summary
    • Fact Sheet
    • Objectives
    • Mission Team
    • Orbit View
    • Background Science
    • Martian Interior
    • Martian Surface
    • Phobos
    • Science Results
    • Methane on Mars Workshop 2009
    • Workshop Mars III, Les Houches, 2010
    • Spacecraft…

      • Spacecraft
      • 3D Model
      • Engineering
    • Instruments…

      • Design
      • Objectives
    • Mission Operations…

      • Launch Vehicle
      • Launch Phase
      • Cruise Phase
    • Science Operations
    • Data Archive
    • Data workshops
    • Resources
    • News Archive
    • Multimedia Gallery
    • Publication Archive
    • Calendar of Events
    • Services
    • Contact Us
    • Subscribe
    • Terms and Conditions
    • Bookmark and Share

    Simulated levels of methane in the Martian atmosphere - lifetime of 200 days

    Date: 06 Aug 2009
    Depicts: Simulation of methane concentration in Martian atmosphere with a local source and an atmospheric lifetime of 200 days
    Copyright: © 2009 Nature Publishing Group, (from Lefèvre & Forget [2009])

    This map shows the column-averaged mixing ratio of methane in parts per billion by volume (p.p.b.v) as derived from a global climate-chemical model of Mars. The levels are for a solar longitude LS of 150° corresponding to late northern summer/southern winter. A local methane source was included, marked by the white square, active for only 120 Martian days around LS=150°, or LS=120°-183°.

    The amount of methane released from the source was set to balance the global loss integrated over the Martian year assuming an atmospheric lifetime for methane of about 200 Earth days. This lifetime is shorter than would be expected from currently understood chemical processes by a factor of about 600.

    Under these conditions the global model is able to produce the local enhancement and variation in the methane concentration recently reported by Mumma et al. (2009).


    Last Update: 06 Aug 2009

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=45388
    • Latest selection
    • Night-side ionosphere of Mars
    • Dayside ionosphere of Mars
    • Dayside and night-side profiles of the Martian ionosphere
    • Image Hi-Res Versions
    • Hi-Res [jpg]
      129.21 kb.
    • Related Images
    • Simulated levels of methane in the Martian atmosphere
    • See also
    • Reconciling methane variations on Mars
    • Related Publications
    • F. Lefèvre & F. Forget [2009]

    Connect with us

    • RSS
    • Youtube
    • Twitter
    • Flickr
    • Google Buzz
    • Livestream
    • Subscribe
    • App Store
    • ESA Science Twitter

    Follow ESA science

    • Copyright 2000 - 2013 © European Space Agency. All rights reserved.

    • Terms and Conditions