Computer Science
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1531t&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1531
Computer Science
Scientific paper
Understanding the albedo distribution of the Near- Earth Object (NEO) population allows for a better understanding of the relationship between absolute magnitude and size, which impacts calculations of size frequency distribution and impact hazards. Examining NEO albedos also sheds light on the differences between the NEO and Main Belt populations. We combine albedo results from the ExploreNEOs Warm Spitzer Exploration Science program [17] with taxonomic classifications from the literature, publicly available datasets, and new observations from our concurrent spectral survey to derive the average albedos for C-, D-, Q-, S-, V- and X-complex NEOs.
Benner Lance A. M.
Bhattacharya Bhubanjyoti
Bottke William F.
Chesley Steve
Delbo' Marco
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