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The history of Martian volatiles

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Jakosky, Bruce M., Jones, John H.·1997·Reviews of Geophysics

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Abstract

The behavior of water and other volatiles on Mars is key to understanding the evolution of the climate. The early climate played a fundamental role in producing the observed surface morphology and possibly in enabling the existence of an early biosphere. Geochemical and isotopic data can be used to infer the history of volatiles. On the basis of the isotopic data from the atmosphere and from components of the surface (as measured in meteorites that come from Mars), there appear to be at least two reservoirs of volatiles, one that has undergone exchange with the atmosphere and has been isotopically fractionated, and a second that is unfractionated and may represent juvenile gases. The fractionation of the atmospheric component has occurred primarily through the escape of gas to space. In addition, the atmospheric gases have mixed substantially with crustal reservoirs of volatiles. Such exchange may have occurred in aqueous or hydrothermal environments. The history of escape to space, as driven by the properties of the Sun through time, is consistent with the surface geomorphology. Together, they suggest an early environment that was substantially different from the present one and the evolution through time to a colder, dryer climate.

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Authors: Jakosky, B. M., & Jones, J. H.
Affiliations: University of Colorado Boulder (US)
Johnson Space Center (US)
ORCID: Jakosky, Bruce M.
Jones, John H.
Venue: Reviews of Geophysics
Publisher: American Geophysical Union (AGU)
Published: 1997-02
Volume: 35
Issue: 1
Pages: 1-16
ISSN: 0096-1043 (ISSN-L)
8755-1209
1944-9208
DOI: 10.1029/96rg02903
OpenAlex: W2153597165
Cited by: 144
References: 104
Citations by year: 2026: 3 · 2025: 3 · 2024: 5 · 2023: 1 · 2022: 4 · 2021: 1 · 2020: 2 · 2019: 2 · 2018: 1 · 2017: 7 · 2016: 7 · 2015: 2 · 2014: 7 · 2013: 7 · 2012: 2
FWCI: 10.10
Type: journal article
Language: en
Open access: bronze
doi.org
Licence: onlinelibrary.wiley.com/termsAndConditions#vor (vor)
Locations: Reviews of Geophysics (publishedVersion)
Topics: Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Geology and Paleoclimatology Research
Keywords: Martian volatiles, water on Mars, Mars atmosphere, isotope fractionation, volatile reservoirs, atmospheric escape, hydrothermal environments, climate evolution, Martian meteorites

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The history of Martian volatiles

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