Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000dps....32.0308d&link_type=abstract
American Astronomical Society, DPS Meeting #32, #03.08; Bulletin of the American Astronomical Society, Vol. 32, p.996
Astronomy and Astrophysics
Astronomy
Scientific paper
Hapke modeling of 433 Eros' disk-integrated solar phase curve from ground-based telescopic observations and NEAR-Shoemaker spacecraft measurements show that Eros' surface photometric properties are typical of average S-class asteroids. Eros displays the same single particle scattering characteristics and porosity versus grain size relationships as typical S-asteroids. Eros' single scattering albedo is similar in value to that of 951 Gaspra. The physical albedo derived for Eros is higher than either 243 Ida or it's satellite Dactyl, but is equivalent to Gaspra's within the error bars. The phase integral and Bond albedo for Eros is significantly lower than for either Gaspra, Ida, or average S-asteroids. Results are commensurate with the photometric analysis of the NIS low-phase fly-by observations.
Carcich Brian
Clark Beth Ellen
Domingue Donovan L.
Joseph James
Robinson Michael
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