Exogenic basalt on asteroid (101955) Bennu
Résumé
When rubble-pile asteroid 2008 TC3 impacted Earth on October 7, 2008, the recovered rock
fragments indicated that such asteroids can contain exogenic material [1,2]. However,
spacecraft missions to date have only observed exogenous contamination on large,
monolithic asteroids that are impervious to collisional disruption [3, 4]. Here we report the
presence of meter-scale exogenic boulders on the surface of near-Earth asteroid (101955)
Bennu—the 0.5-km, rubble-pile target of the OSIRIS-REx mission [5] which has been
spectroscopically linked to the CM carbonaceous chondrite meteorites [6]. Hyperspectral
data indicate that the exogenic boulders have the same distinctive pyroxene composition as
the howardite–eucrite–diogenite (HED) meteorites that come from (4) Vesta, a 525-km-
diameter asteroid that has undergone differentiation and extensive igneous processing [7,
8, 9]. Delivery scenarios include the infall of Vesta fragments directly onto Bennu or
indirectly onto Bennu’s parent body, where the latter’s disruption created Bennu from a
mixture of endogenous and exogenic debris. Our findings demonstrate that rubble-pile
asteroids can preserve evidence of inter-asteroid mixing that took place at macroscopic
scales well after planetesimal formation ended. Accordingly, the presence of HED-like
material on the surface of Bennu provides previously unrecognized constraints on the
collisional and dynamical evolution of the inner main belt.
Domaines
Planète et Univers [physics]
Origine : Fichiers produits par l'(les) auteur(s)