Size–Frequency Distribution of Terrestrial Leftover Planetesimals and S-complex Implanted Asteroids

The isotopic composition of meteorites linked to S-complex asteroids has been used to suggest that these asteroids originated in the terrestrial planet’s region, i.e., within 1.5 au, and later got implanted into the main asteroid belt (MAB). Dynamical models of planet formation support this view. Ye...

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Hlavní autoři:	Rogerio Deienno, André Izidoro, David Nesvorný, William F. Bottke, Fernando Roig, Simone Marchi
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2025-01-01
Edice:	The Astrophysical Journal
Témata:	Asteroid belt Asteroid dynamics Solar system formation Solar system terrestrial planets
On-line přístup:	https://doi.org/10.3847/1538-4357/adccbb
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