titre : The solar wind is the cause of rapid ageing of the asteroids

Why the materials constituting the surface of the asteroids reflect in a different way the light when they are in space or in laboratory, appearing thus redder and darker in space ? This different behavior is mainly due to the interaction of the interplanetary medium with the surface of the asteroids. This surface is deteriorated by the solar wind and the micrometeorites present in the interplanetary medium.

This team studied young families of asteroids formed from violent collisions and having thus a young surface. These asteroids submitted to the impacts of the interplanetary medium see their surface evolving very quickly, in approximately 1 million years, to arrive at surfaces having average colors identical to those of old asteroids. This rapid evolution supports the role of the solar wind as principal element in the transformation of their surfaces. The composition plays also a part, the asteroids including olivine evolving more quickly.

Figure 1 : Evolution de la couleur des astéroïdes en fonction de leur âge en supposant que ces objets ont la même composition. La couleur initiale d’un astéroïde lorsqu’il vient de subir une collision catastrophique (qui le décompose en divers fragments) devrait être semblable à la couleur des météorites mesurées en laboratoire. L’observation de jeunes astéroïdes (âge < 1 million d’année) révèle que leur couleur a été fortement modifiée en ce temps très court leur donnant l’apparence de surfaces âgées. Seul le vent solaire (flèche rouge) peut agir aussi rapidement sur la couleur de ces objets comme l’ont démontré des expériences en laboratoire. Dans un deuxième temps, les impacts de micrométéorites pourraient vieillir les surfaces avec une échelle de temps plus longue. © Nature. Cliquer sur l’image pour l’agrandir

This team was also interested in the asteroids crossing the orbit of the Earth (NEA : Near-Earth Asteroids) which for some have a color which reveals a surface virgin of any deterioration. All these objects were formed by collisions since more than 100 million years. Thus, recent collisions cannot explain their apparent youth and it is necessary to find another process being able to renovate the matter on the surface. These asteroids could undergo gravitational effects with the approach of the Earth or another telluric planet (tidal effects) tending to dredge up on the surface the internal material, which was not exposed to the solar wind, and thus to give this effect of "renovation". It will be necessary to confirm this hypothesis in observing the spectral color of the asteroids of the same type present in the principal belt, between Mars and Jupiter, which should then be redder.

Communiqué de presse

INSU-CNRS

Reference

Â Solar wind as the origin of rapid reddening of asteroid surfaces P. Vernazza, R. P. Binzel, A. Rossi, M. Fulchignoni & M. Birlan Nature 23/04/2009.

Contact

Pierre Vernazza
(ESA, et Observatoire de Paris, LESIA)
Marcello Fulchignoni
(Observatoire de Paris, LESIA, et CNRS)
Mirel Birlan

Dernière modification le 21 décembre 2021