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Astrometry of Outer Solar System Bodies with Small Telescopes
Published online by Cambridge University Press: 30 March 2016
Abstract
Astrometry for an accurate orbit determination of distant objects is usually made with large telescopes ranging from 2 to 10 meters. In selected cases the bright(er) part of their population has been effectively observed with small 0.6 to 1 meter class telescopes. We point out here methods and techniques used at the Kle Observatory including our results. The extension of this programme using a new larger telescope is in preparation. We also mention a possibility of using some web tools for call for follow-up.
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- II. Joint Discussions
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- Copyright © Astronomical Society of Pacific 2002