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HST Snapshot Images of Asteroids. Alex Storrs Khaldoun Makhoul Mike Gaffey, U. of N. Dakota Rob Landis, JPL Faith Vilas, JSC and NASA HQ Ed Wells, CSC/STScI Chuck Wood Ben Zellner, Ga. Southern Univ. 1 Ceres, F439W. 0.5 arcsec.
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HST Snapshot Images of Asteroids Alex Storrs Khaldoun Makhoul Mike Gaffey, U. of N. Dakota Rob Landis, JPL Faith Vilas, JSC and NASA HQ Ed Wells, CSC/STScI Chuck Wood Ben Zellner, Ga. Southern Univ.
1 Ceres, F439W 0.5 arcsec
F673N ratio F791W 0.5 arcsec
45 Eugenia, F439W 0.5 arcsec
87 Sylvia, F439W 0.5 arcsec
107 Camilla, F439W 0.5 arcsec
Conclusions • Resolve the disks of large main belt asteroids • Easily detect companions • Compare colors to primaries– • some significant differences • Restore images at high resolution • 1 Ceres is noticeably oblate • Map distribution of volatiles, minerals on surface • 1 Ceres has a region with depressed 0.7 mm reflection