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Rotational Evolution of Asteroids: The Confined Tumbling State as the Origin of the Excess of Slowly Rotating Asteroids

. IntroductionIt was initially assumed that asteroid rotation distribution had to take a Maxwellian form, peaking at about four revolutions per day as the result of the collision-induced random distribution of their spin vectors in three-dimensional velocity space (Harris & Burns, 1979).
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Asteroid Rotations

2002
P. Pravec, A. W. Harris, T. Michalowski
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Asteroids: equilibrium shapes of rotating gravitational aggregates .

2011
Many evidences lead us to think that a significant portion of asteroids are aggregates of boulders kept together by gravity, with little or no contribution from cohesive forces. The standard hydrodynamics results for a self-gravitating and rotating cohesionless body would impose it to stay close to one of the well-known equilibrium sequences of ...
Comito, C. +6 more
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Asteroid rotation rates

Icarus, 1979
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Comments on “On the dynamics of non-rigid asteroid rotation”

Acta Astronautica, 2020
M Yu Ovchinnikov, D S Roldugin
exaly

The dynamics of asteroid rotation, governed by YORP effect: The kinematic ansatz

Acta Astronautica, 2018
Sergey V Ershkov, Roman V Shamin
exaly

Asteroid rotation and orbit control via laser ablation

Advances in Space Research, 2016
Massimo Vetrisano +2 more
exaly

Acceleration of the rotation of asteroid 1862 Apollo by radiation torques

Nature, 2007
J Ďurech, Brian D Warner, Yu N Krugly
exaly

On the rotation rates and axis ratios of the smallest known near-Earth asteroids—The archetypes of the Asteroid Redirect Mission targets

Planetary and Space Science, 2015
Paul Wiegert
exaly