Détail du document
Identifiant

oai:arXiv.org:2411.01150

Sujet
Astrophysics - Earth and Planetary...
Auteur
Kane, Stephen R. Ernst, Richard Gillmann, Cedric Jones, Christopher Lyons, Timothy Tino, Christopher
Catégorie

sciences : astrophysique

Année

2024

Date de référencement

06/11/2024

Mots clés
evolution earth
Métrique

Résumé

Understanding planetary habitability is one of the major challenges of the current scientific era, particularly given the discovery of a large and diverse terrestrial exoplanet population.

Discerning the primary factors that contribute to planetary habitability may be extracted through a detailed examination of the terrestrial planets within the Solar System, most particularly Venus, Earth, and Mars, and the evolution of their interiors and atmospheres through time.

Here, we provide a detailed description of the fundamental properties of these three planets, the effects of solar evolution, and the potential contributions of these various aspects toward driving their evolutionary pathways.

We argue that evolution of Venus, Earth, and Mars provide essential templates from which a more comprehensive approach toward the study of planetary habitability may be derived.

;Comment: 45 pages, 3 figures, accepted for publication in "The Archean Earth" (ed.: M. Homan, P. Mason, R. Ernst, T. Lyons, C. Heubeck, D. Papineau, E. Stueeken, R. Mazumder, A. Webb, W. Altermann), Elsevier

Kane, Stephen R.,Ernst, Richard,Gillmann, Cedric,Jones, Christopher,Lyons, Timothy,Tino, Christopher, 2024, Our Solar System Neighborhood: Three Diverging Tales of Planetary Habitability and Windows to Earth's Past and Future

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