The high frequency variations in the rotation of Eros - Archive ouverte HAL Access content directly
Journal Articles Astronomy and Astrophysics - A&A Year : 2005

The high frequency variations in the rotation of Eros

(1, 2) , (3, 1, 2)


We use very precise information concerning the physical properties of the asteroid Eros 433, obtained by the NEAR probe mission, to analytically compute the modifications of its rotation on a short time scale, with a precision never reached before for an asteroid. Two kinds of components are investigated here: the free rotation and the forced one, due to the gravitational torque exerted by the Sun. Coefficients of the short periodic part of Eros' forced nutation are rather large, due to the fact that the asteroid has a significant triaxial shape. They are calculated with the same relative accuracy as the moments of inertia of the asteroid. Our results are compared with those obtained through numerical integration (Miller et al. [CITE], Icarus, 155, 3), which show high frequency oscillations of the position of Eros' axis of figure in space. Some important differences are discussed.
Fichier principal
Vignette du fichier
aa0780.pdf (436.72 Ko) Télécharger le fichier
Origin : Publisher files allowed on an open archive

Dates and versions

hal-03732598 , version 1 (26-10-2022)



Jean Souchay, Sébastien Bouquillon. The high frequency variations in the rotation of Eros. Astronomy and Astrophysics - A&A, 2005, 433, pp.375-383. ⟨10.1051/0004-6361:20035780⟩. ⟨hal-03732598⟩
3 View
0 Download



Gmail Facebook Twitter LinkedIn More