Volume 472, Number 2, September III 2007
|Page(s)||653 - 656|
|Section||Planets and planetary systems|
|Published online||26 June 2007|
Testing space weathering models on A-type asteroid (1951) Lick
Dipartimento di Fisica, Università del Salento, via Arnesano, 73100 Lecce, Italy
2 INAF – Osservatorio Astrofisico di Catania, via S. Sofia 78, 95123 Catania, Italy e-mail: firstname.lastname@example.org
3 Instituto de Astrofísica de Canarias, c/Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain
4 Isaac Newton Group, 38700, Santa Cruz de La Palma, Tenerife, Spain
Accepted: 15 June 2007
Aims.A-type asteroid (1951) Lick has a very red visible and near-infrared reflectance spectrum, and it is one of the reddest Near-Earth objects. Its surface is probably affected by heavy space weathering processes. Here we investigate the possibility of a weathering saturation regime.
Methods.We compare Lick's spectrum with those of silicate olivine after laser ablation experiments, reported by Brunetto et al. (2006a, Icarus, 180, 546; 2007, Icarus, in press). We apply scattering and space weathering models developed by Hapke (1981, J. Geophys. Res., 86, 3039; 2001, J. Geophys. Res., 106, 10039).
Results.We successfully fit the spectrum of Lick, in terms of slope, band profile, and albedo. Results confirm that Lick has olivine with Mg number higher than that of the Brachina meteorite. The use of metallic iron inclusions in the model yields a product of volume fraction of inclusions times effective optical path length of about 0.039 μm, similarly to what observed experimentally after UV laser ablation of Mg-rich olivine.
Conclusions.The surface of Lick is extremely weathered, indicating a saturation regime similar to what observed in the laboratory, and suggesting that the asteroid surface is probably older than about 107–108 years.
Key words: minor planets / asteroids / solar system: general
© ESO, 2007
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