collaborators

6 papers

astro-ph.EP2026

Size Constraints for the Pre-atmospheric Parent Bodies of Ordinary Chondrites

Juan A. Sanchez, David C. Cantillo, Adam Battle +7

The study of S-complex near-Earth objects (NEOs), the parent bodies of ordinary chondrites, has shown that they are dominated by asteroids with LL chondrite-like compositions. This…

astro-ph.EP2026

Analysis of Karin and Koronis2 asteroid families: new findings and challenges

David Vokrouhlický, David Nesvorný, William F. Bottke

We use our home catalog of the asteroid proper elements to study the Karin family. The hierarchical clustering method provides formal identification with 3,863 members, but this se…

astro-ph.EP2025

Terrestrial Planet Formation from Two Source Reservoirs

David Nesvorny, Alessandro Morbidelli, William F. Bottke +2

This work describes new dynamical simulations of terrestrial planet formation. The simulations started at the protoplanetary disk stage, when planetesimals formed and accreted into…

astro-ph.EP2025

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

Rogerio Deienno, Andre Izidoro, David Nesvorny +3

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 a…

astro-ph.EP2025

A pre-flyby view on the origin of asteroid Donaldjohanson, a target of the NASA Lucy mission

Simone Marchi, David Vokrouhlický, David Nesvorný +3

The NASA Lucy mission is scheduled to fly-by the main belt asteroid (52246) Donaldjohanson on April 20, 2025. Donaldjohanson (DJ hereafter) is a member of the primitive (C-type cla…

astro-ph.EP2025

Orbital and absolute magnitude distribution of Hilda population

David Vokrouhlický, David Nesvorný, Miroslav Brož +4

The Hilda population of asteroids is located in a large orbital zone of long-term stability associated with the Jupiter J3/2 mean motion resonance. They are a sister population of…