Impact degassing and atmospheric erosion on Venus, Earth, and Mars during the late accretion-Reference-Cited by-同舟云学术

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Impact degassing and atmospheric erosion on Venus, Earth, and Mars during the late accretion

Published:2019-01 Issue: Volume:317 Page:48-58
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Sakuraba Haruka,Kurokawa Hiroyuki^ORCID,Genda Hidenori^ORCID

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference59 articles.

1. The formation of an impact-generated H2O atmosphere and its implications for the early thermal history of the Earth;Abe;J. Geophys. Res.: Solid Earth,1985

2. Evolution of an impact-generated H2O–CO2 atmosphere and formation of a hot proto-ocean on Earth;Abe;J. Atmos. Sci.,1988

3. The fossilized size distribution of the main asteroid belt;Bottke;Icarus,2005

4. The irregular satellites: the most collisionally evolved populations in the solar system;Bottke;Astron. J.,2010

5. Atmospheric Evolution on Inhabited and Lifeless Worlds;Catling,2017

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1. The evolutionary divergence of Mars, Venus, and Earth;Reference Module in Earth Systems and Environmental Sciences;2024

2. The spirited youth of Venus;Nature Astronomy;2023-12-14

3. Magma Ocean, Water, and the Early Atmosphere of Venus;Space Science Reviews;2023-09-20

4. Variability Catalog of Stars Observed during the TESS Prime Mission;The Astrophysical Journal Supplement Series;2023-08-18

5. The Habitability of Venus;Space Science Reviews;2023-02-22

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