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Meteorites and Planet Formation

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arxiv 2404.15424 v1 pith:F6XFF5JW submitted 2024-04-23 astro-ph.EP astro-ph.SRphysics.geo-ph

Meteorites and Planet Formation

classification astro-ph.EP astro-ph.SRphysics.geo-ph
keywords formationplanetarymeteoritestheysolarsystemsystemsevolution
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Meteorites are a remarkable resource. They capture the imagination of people worldwide with their spectacular entry through Earth's atmosphere as fireballs, and their exotic character of being pieces of other worlds. Scientifically, they are critical to interpreting the early stages of formation of the Solar System, as well as the geological evolution of asteroids, the Moon, and Mars, and they are vital to understanding planetary formation processes. With the burgeoning exploration of extrasolar planetary systems, knowledge of the fundamental process of planetary growth from protoplanetary disks has taken on a new significance. Meteorites provide essential and detailed insight into the formation of planetary systems, although we must bear in mind that they only represent one reference point (our own Solar System) in what is clearly a wide spectrum of possible chemical and physical parameters governing the diverse realm of extrasolar planets. This chapter summarises the nature of our meteorite collections, and the ways in which meteorites contribute to our understanding of the formation and evolution of our own Solar System, with broader implications for planetary systems in general.

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  1. Chondrite Parent Bodies as Escaped Satellites of Proto-Planetary Embryos

    astro-ph.EP 2026-07 conditional novelty 7.0

    Embryo-embryo impacts create circum-embryo disks whose melted ejecta accrete into asteroid-sized satellites that are later scattered into heliocentric orbit, forming the parent bodies of ordinary chondrites.