Origin of the Spacewatch Small Earth-Approaching Asteroids

التفاصيل البيبلوغرافية
العنوان: Origin of the Spacewatch Small Earth-Approaching Asteroids
المؤلفون: Bottke, William F., Nolan, Michael C., Melosh, H.J., Vickery, Ann M., Greenberg, Richard
المصدر: Icarus; August 1996, Vol. 122 Issue: 2 p406-427, 22p
مستخلص: Recent discoveries of small Earth-approaching asteroids by the 0.9 m Spacewatch telescope (referred to here as S-SEAs) reveal 16 objects which have diameters ∼50 m or smaller. Approximately half of these objects lie in a region where few large near-Earth asteroids are found, with perihelia (q) and aphelia (Q) near 1 AU,e< 0.35, andifrom 0° to ∼30°. Possible origins for these objects are examined by tracking the orbital evolution of test bodies from several possible source regions using an Öpik-type Monte Carlo dynamical evolution code, modified to include (a) impact disruption, based on a map in orbital (a,e,i) space of collision probabilities and mean impact velocities determined using actual main-belt and near-Earth asteroid orbits, (b) fragmentation, and (c) observational selection effects.
قاعدة البيانات: Supplemental Index
الوصف
تدمد:00191035
10902643
DOI:10.1006/icar.1996.0133