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Hubble Space Telescope Images of Asteroid 4 Vesta in 1994

โœ Scribed by Benjamin H. Zellner; Rudolph Albrecht; Richard P. Binzel; Michael J. Gaffey; Peter C. Thomas; Alex D. Storrs; Eddie N. Wells


Publisher
Elsevier Science
Year
1997
Tongue
English
Weight
308 KB
Volume
128
Category
Article
ISSN
0019-1035

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โœฆ Synopsis


The Planetary Camera of the WFPC2 on board the Hubble Space Telescope was used in late 1994 to record 56 images of demonstrated that the photometric lightcurve of Vesta is Asteroid 4 Vesta in four compositionally diagnostic wavelength not due to shape and shadowing, as is the case for almost bands. The images were taken at eight epochs to give global all other asteroids, but is due to hemispheric albedo differcoverage of Vesta at an aspect of approximately 16ุ‡ north ences of about 10%. Conspicuous albedo markings from latitude. The prograde rotation of Vesta is clearly revealed groundbased speckle interferometry have been reported by surface markings contributing to a hemispherical albedo by Drummond et al. (1988) and Drummond and Hege difference.


๐Ÿ“œ SIMILAR VOLUMES


Imaging of Asteroid 4179 Toutatis with t
โœ Keith S. Noll; H.A. Weaver; A.D. Storrs; B. Zellner ๐Ÿ“‚ Article ๐Ÿ“… 1995 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 572 KB

We obtained four images of the asteroid 4179 Toutatis during its close approach to the Earth on 10 December 1992 with the planetary camera of the Hubble Space Telescope. The distance between the Earth and Toutatis at the time of our observations was \(0.0291 \mathrm{AU}\left(4.35 \times 10^{6} \math