activity
20162026
most citedCol-OSSOS: Colors of the Interstellar Planetesimal 1I/`Oumuamua

87 citations · 610 across the 26 of their papers we have counts for

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Showing astro-ph.EPShow all

39 papers · 1 filter

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.EP2026

Tianwen-2 target asteroid (469219) Kamo'oalewa probably develops an Itokawa-compositional but ultra-highly space-weathered surface

Pengfei Zhang, Guozheng Zhang, Zichen Wei +45

China's Tianwen-2 mission plans to return samples from a small, rapidly spinning Earth quasi-satellite (469219) Kamo'oalewa. Previous studies linked Kamo'oalewa to lunar compositio…

astro-ph.EP2026

Apophis source population and Earth encounter frequency of Apophis-like bodies

M. Brož, R. P. Binzel, P. Vernazza +4

We provide context for Apophis' 2029 Earth passage by analyzing its possible source populations, in particular, the Flora family, which has a similar composition, corresponding to…

astro-ph.EP2026

Col-OSSOS: Investigating the Origins of Different Surfaces in the Primordial Kuiper Belt

Laura E. Buchanan, Megan E. Schwamb, Wesley C. Fraser +12

The Colours of the Outer Solar System Origins Survey (Col-OSSOS) measured the optical/NIR colours of a brightness-complete sample of Trans-Neptunian Objects (TNOs). Like previous s…

astro-ph.EP202514 cited

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

A dynamical dichotomy in large binary asteroids

K. Minker, B. Carry, F. Vachier +20

No less than 15% of large (diameter greater than 140 km) asteroids have satellites. The commonly accepted mechanism for their formation is post-impact reaccumulation. However, the…