Hydrogen escape from Mars is driven by seasonal and dust storm transport of water

Author:

Stone Shane W.1ORCID,Yelle Roger V.1ORCID,Benna Mehdi23ORCID,Lo Daniel Y.1ORCID,Elrod Meredith K.24ORCID,Mahaffy Paul R.5ORCID

Affiliation:

1. Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85711, USA.

2. Planetary Environments Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.

3. Center for Research and Exploration in Space Science and Technology, University of Maryland Baltimore County, Baltimore, MD 21250, USA.

4. Center for Research and Exploration in Space Science and Technology, University of Maryland College Park, College Park, MD 20742, USA.

5. Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.

Abstract

Dust storms cause Mars to lose water Mars was once a wet planet, but it has lost most of its water through reactions that produce hydrogen, which escapes from the upper atmosphere into space. Stone et al. used data from the Mars Atmosphere and Volatile Evolution spacecraft to study how water is transported to the upper atmosphere and converted to hydrogen. They found that water can reach higher altitudes than previously thought, especially during global or regional dust storms. Photochemical modeling shows that this process dominates the current loss of water from Mars and influenced the evolution of its climate. Science , this issue p. 824

Funder

National Aeronautics and Space Administration

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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