Physics – Optics
Scientific paper
Jul 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000hst..prop.8578m&link_type=abstract
HST Proposal ID #8578
Physics
Optics
Hst Proposal Id #8578 Solar System
Scientific paper
We recently made the first-ever discovery of a satellite of an asteroid from the Earth, using adaptive optics {Merline et al. 1999a, 1999b}. We propose here to acquire the first separate, comparative, and simultaneous spectra of an asteroid and its satellite. We will employ the UV-capabilities and high-spatial-resolution properties of STIS to study {45}Eugenia, and its satellite, S/1998{45}1, by obtaining medium-resolution spectra over the range 2900-10300 Angstrom, using only two grating settings, on a single HST orbit. We will determine whether the spectra, and hence surface compositions, are similar or different in a parent-satellite pair, and to test hypotheses concerning satellite production mechanisms. From the orbital parameters, determined using our ground-based adaptive-optics images, we have already determined that {45}Eugenia has a surprisingly low density of 1.2 g cm^-3. We know the spectrum of Eugenia is a {Tholen} FC-type, which is similar to the common C-types, but differs by the lack of a UV-band or UV-dropoff and by subtle, but measurable differences in the spectral slope. Both the UV-region and the existence of subtle absorption features in the near-IR { 0.9 micron} are diagnostic of the specific differences between F-, C-, and {Bus'} X-class. HST spectroscopy is the only way to separate the pair, because ground-based adaptive optics is not available in the UV and cannot yet provide adequate resolution in the visible.
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