Physics – Optics
Scientific paper
Jan 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996eiaf.conf....7d&link_type=abstract
Workshop on Evolution of Igneous Asteroids: Focus on Vesta and the HED Meterorites, p. 7
Physics
Optics
Vesta Asteroid, Adaptive Optics, Mapping, Hubble Space Telescope, Infrared Telescopes, Pyroxenes, Albedo, Galileo Spacecraft, Imaging Techniques, Mineralogy
Scientific paper
Until recently it was not possible to directly image and resolve any asteroids from the ground.This situation was mainly due to the limitation imposed by the atmospheric turbulences to resolve any subarcsecond object. High-resolution observations of asteroid surfaces were then obtained from speckle interferometry and radar imaging as well as direct imaging from space: The Galileo spacecraft made two successful flybys of asteroids 951 Gaspra and 243 Ida and Hubble Space Telescope observed 4 Vesta during the 1994 opposition. Adaptive optics (AO) is radically changing this situation: Correcting the effects of the atmospheric turbulences, it restores the full theoretical resolving power of a telescope. Details on the surface of the largest asteroids can be imaged from the ground in the near-infrared and visible; these are the optimal wavelength ranges because the gain in resolution obtained with AO is maximal and they contain most of the spectral signatures of the minerals. Vesta is certainly the most interesting asteroid to be observed with AO since it is the only large minor planet showing substantial hemispherical albedo variations We will present the results of the two last Vesta oppositions observed using telescopes equipped with AO.
Dumas Cédric
Hainaut Olivier R.
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