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astro-ph.EP2026

Direct contact binary planetesimal formation from gravitational collapse

Jackson T. Barnes, Stephen R. Schwartz, Seth A. Jacobson

Bilobate contact binaries comprise a significant fraction of the relict Kuiper Belt, which includes the exemplary contact binary (486958) Arrokoth. The surfaces of its lobes contai…

astro-ph.EP2025

Formation of Planetesimals in the Outer Solar System

Anders Johansen, Michele T. Bannister, Luke Dones +4

The Solar System hosts the most studied and best understood major and minor planetary bodies - and the only extraterrestrial bodies to have been visited by spacecraft. The Solar Sy…

astro-ph.EP2025

Orbits of very distant asteroid satellites

K. Minker, B. Carry, F. Vachier +36

The very wide binary asteroid (VWBA) population is a small subset of the population of known binary and multiple asteroids made of systems with very widely orbiting satellites and…

astro-ph.EP2024

Tungsten isotope evolution during Earth's formation and new constraints on the viability of accretion simulations

D. C. Rubie, K. I. Dale, G. Nathan +5

The Hf-W isotopic system is the reference chronometer for determining the chronology of Earth's accretion and differentiation. However, its results depend strongly on uncertain par…

astro-ph.EP2024

BYORP and Dissipation in Binary Asteroids: Lessons from DART

Matija Ćuk, Harrison Agrusa, Rachel H. Cueva +10

The Near-Earth binary asteroid Didymos was the target of a planetary defense demonstration mission DART in September 2022. The smaller binary component, Dimorphos, was impacted by…

astro-ph.EP2024

Forming Mercury from excited initial conditions

Jennifer Scora, Diana Valencia, Alessandro Morbidelli +1

Mercury is notoriously difficult to form in solar system simulations, due to its small mass and iron-rich composition. Smooth particle hydrodynamics simulations of collisions have…