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. 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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Reply on the comments on “on the dynamics of non-rigid asteroid rotation”
Acta Astronautica, 2021Sergey Ershkov, Dmytro Leshchenko
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Asteroids: equilibrium shapes of rotating gravitational aggregates .
2011Many 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 ...
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Comments on “On the dynamics of non-rigid asteroid rotation”
Acta Astronautica, 2020Michael Ovtchinnikov, D S Roldugin
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The dynamics of asteroid rotation, governed by YORP effect: The kinematic ansatz
Acta Astronautica, 2018Sergey Ershkov, Roman V Shamin
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Averaged rotational dynamics of an asteroid in tumbling rotation under the YORP torque
Celestial Mechanics and Dynamical Astronomy, 2010D J Scheeres, Scheeres D J
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Asteroid rotation and orbit control via laser ablation
Advances in Space Research, 2016Massimiliano Vasile +2 more
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Acceleration of the rotation of asteroid 1862 Apollo by radiation torques
Nature, 2007Yurij Krugly +2 more
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