activity
20242026
collaborators

5 papers

astro-ph.SR2026

Lithium Enrichment in a Subgiant Star with a Brown Dwarf Companion: A Planetary Engulfment Candidate

Brooke Kotten, Melinda Soares-Furtado, Ricardo Yarza +11

Theoretical models predict that subgiants within a narrow mass regime can retain detectable lithium enrichment signatures from planetary engulfment. We test this prediction using T…

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…