Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1776117 | Icarus | 2006 | 8 Pages |
Abstract
Arecibo (2380 MHz, 13 cm) radar observations of 2005 CR37 provide detailed images of a candidate contact binary: a 1.8-km-long, extremely bifurcated object. Although the asteroid's two lobes are round, there are regions of modest topographic relief, such as an elevated, 200-m-wide facet, that suggest that the lobes are geologically more complex than either coherent fragments or homogeneous rubble piles. Since January 1999, about 9% of NEAs larger than ∼200 m imaged by radar can be described as candidate contact binaries.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Lance A.M. Benner, Michael C. Nolan, Steven J. Ostro, Jon D. Giorgini, Donald P. Pray, Alan W. Harris, Christopher Magri, Jean-Luc Margot,