activity
20242026
collaborators

7 papers

astro-ph.EP2026

Unmasking (44) Nysa: Evidence for a trilobate structure

Kate Minker, Anthony Berdeu, Gianluca Li Causi +16

Context. (44) Nysa is one of the largest known E-type asteroids. Light curve inversion models have indicated that it may have an elongated shape commonly found in large binary syst…

astro-ph.EP2026

The spin state of asteroid Apophis and a prediction of its change during the 2029 close encounter with Earth

J. Durech, D. Vokrouhlicky, P. Pravec +23

On April 13, 2029, the asteroid Apophis will pass near Earth at a geocentric distance of about 38,000 km. Numerical models have suggested that the post-encounter spin state will cr…

astro-ph.EP2025

Catastrophic disruption of asteroid 2023 CX1 and implications for planetary defense

Auriane Egal, Denis Vida, François Colas +94

Mitigation of the threat from airbursting asteroids requires an understanding of the potential risk they pose for the ground. How asteroids release their kinetic energy in the atmo…

astro-ph.EP2025

Satellite formation around the largest asteroids

Kevin J. Walsh, Ronald-Louis Ballouz, Harrison F. Agrusa +3

Satellites around large asteroids are preferentially found among those with the most rapid rotation and elongated shape. The taxonomic statistics are similarly skewed; in total, 13…

astro-ph.EP2025

The discovery and characterization of Earth-crossing asteroid 2024 YR

Bryce T. Bolin, Josef Hanuš, Larry Denneau +9

We describe observations and physical characteristics of Earth-crossing asteroid 2024 YR, discovered on 2024 December 27 by the Asteroid Terrestrial-impact Last Alert System. T…

astro-ph.EP2025

Confined tumbling state as the origin of the excess of slowly rotating asteroids

Wen-Han Zhou, Patrick Michel, Marco Delbo +4

The rotational distribution of asteroids as a function of their size is used {as a diagnostic of} their physical properties and evolution. Recent photometric surveys from the Gaia…