The Exosphere as a Boundary: Origin and Evolution of Airless Bodies in the Inner Solar System and Beyond Including Planets with Silicate Atmospheres

• Published in: Space science reviews Vol. 218; no. 3
• Main Authors: Lammer, Helmut, Scherf, Manuel, Ito, Yuichi, Mura, Alessandro, Vorburger, Audrey, Guenther, Eike, Wurz, Peter, Erkaev, Nikolai V., Odert, Petra
• Format: Journal Article
• Language: English
• Published: Dordrecht Springer Netherlands 01.04.2022; Springer Nature B.V
• Subjects: Aerospace Technology and Astronautics; Astronomical instruments; Astrophysics and Astroparticles; Atmosphere; Building envelopes; Depletion; Exosphere; Extrasolar planets; Fractionation; Inner solar system; Lunar surface; Magma; Mercury; Mercury (planet); Micrometeoroids; Moon; Observatories; Parameter modification; Physics; Physics and Astronomy; Planet formation; Planetary atmospheres; Planetology; Process parameters; Radiation; Solar system; Solar wind; Space Exploration and Astronautics; Space Sciences (including Extraterrestrial Physics; Space telescopes; Stellar radiation; Surface-Bounded Exospheres and Interactions in the Inner Solar System; Telescopes; Terrestrial planets; Dust; Young Sun; Rocky close-in exoplanets; Planetary embryos; Moon; Mercury
• ISSN: 0038-6308; 1572-9672
• DOI: 10.1007/s11214-022-00876-5

In this review we discuss all the relevant solar/stellar radiation and plasma parameters and processes that act together in the formation and modification of atmospheres and exospheres that consist of surface-related minerals. Magma ocean degassed silicate atmospheres or thin gaseous envelopes from planetary building blocks, airless bodies in the inner Solar System, and close-in magmatic rocky exoplanets such as CoRot-7b, HD 219134 b and 55 Cnc e are addressed. The depletion and fractionation of elements from planetary embryos, which act as the building blocks for proto-planets are also discussed. In this context the formation processes of the Moon and Mercury are briefly reviewed. The Lunar surface modification since its origin by micrometeoroids, plasma sputtering, plasma impingement as well as chemical surface alteration and the search of particles from the early Earth’s atmosphere that were collected by the Moon on its surface are also discussed. Finally, we address important questions on what can be learned from the study of Mercury’s environment and its solar wind interaction by MESSENGER and BepiColombo in comparison with the expected observations at exo-Mercurys by future space-observatories such as the JWST or ARIEL and ground-based telescopes and instruments like SPHERE and ESPRESSO on the VLT, and vice versa.