Keck Observations of Solar System Objects: Perspectives for Extremely Large Telescopes

From differential tracking techniques, required for appulse observations of KBOs with Laser Guide Star Adaptive Optics (LGSAO), to developing methods for collecting spectra at the precise moment of a predicted impact, each Solar System observation conducted on a large telescope presents a unique set...

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Published inEarth, moon, and planets Vol. 105; no. 2-4; pp. 115 - 122
Main Authors Conrad, A. R., Goodrich, R. W., Campbell, R. D., Merline, W. J., Drummond, J. D., Dumas, C., Carry, B.
Format Journal Article
LanguageEnglish
Published Dordrecht Springer Netherlands 01.09.2009
Springer Nature B.V
Springer Verlag
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Summary:From differential tracking techniques, required for appulse observations of KBOs with Laser Guide Star Adaptive Optics (LGSAO), to developing methods for collecting spectra at the precise moment of a predicted impact, each Solar System observation conducted on a large telescope presents a unique set of challenges. We present operational details and some key science results from our science program, adaptive optics observations of main belt asteroids and near earth objects ; as well as the technical and operational details of several Keck Solar System observations conducted by other teams: the impact of Shoemaker-Levy 9 on Jupiter, volcanoes on Io, the Deep Impact mission to Comet 9P/Tempel 1, and recent observations of Pluto’s moons Nix and Hydra. For each of these observations, we draw from our Keck experience to predict what challenges may lie ahead when similar observations are conducted on next generation telescopes.
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ISSN:0167-9295
1573-0794
DOI:10.1007/s11038-009-9320-0