Mars Water and D/H Evolution From 3.3 Ga to Present-Reference-Cited by-同舟云学术

Mars Water and D/H Evolution From 3.3 Ga to Present

Published:2019-12 Issue:12 Volume:124 Page:3344-3353
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Alsaeed N. R.¹²³^ORCID,Jakosky B. M.²⁴^ORCID

Affiliation:

1. Department of Astrophysical and Planetary SciencesUniversity of Colorado Boulder Boulder CO USA

2. Laboratory for Atmospheric and Space Physics Boulder CO USA

3. Mohammed bin Rashid Space Center Dubai UAE

4. Department of Geological SciencesUniversity of Colorado Boulder Boulder CO USA

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JE006066

Reference53 articles.

1. Geomorphological Evidence for Water on Mars

2. Ancient oceans, ice sheets and the hydrological cycle on Mars

3. Distribution of Hydrogen in the Near Surface of Mars: Evidence for Subsurface Ice Deposits

4. Widespread excess ice in Arcadia Planitia, Mars

5. Cangi E. Chaffin M. Deighan J. Stewart I. &Schneider N.(2018).Effect of variations in temperature and water vapor profiles in photochemical modeling of H and D escape from Mars. InAAS/Division for Planetary Sciences Meeting Abstracts(Vol. 50).

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