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NOAO > Observing Info > Approved Programs > 2006B-0413 |
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PI: Marc W. Buie, Lowell Observatory, buie@lowell.edu
Address: 1400 W. Mars Hill Road, Flagstaff, AZ 86001, USA
CoI: Lawrence H. Wasserman, Lowell Observatory
CoI: Robert L. Millis, Lowell Observatory
CoI: David E. Trilling, University of Arizona
CoI: James L. Elliot, Massachusetts Institute of Technology
CoI: Karen J. Meech, University of Hawaii
CoI: Susan D. Kern, Massachusetts Institute of Technology
CoI: Amanda A.S. Gulbis, Massachusetts Institute of Technology
CoI: Elisabeth Adams, Massachusetts Institute of Technology
Title: Dynamical Structure of the Kuiper Belt
Abstract:
The orbits and physical properties of Kuiper Belt Objects (KBOs)
provide valuable constraints on the dynamical and environmental
evolution of the outer Solar System. However, a full understanding of
this fossil record requires a large and well characterized sample of
objects with accurate orbits. Accurate orbits reveal important aspects
of the effects of planetary migration on the dynamical history of the
belt and provide ephemerides sufficiently accurate to enable physical
observations with giant groundbased and space telescopes. In May, 2005,
our team concluded the search phase of the Deep Ecliptic Survey - a
survey that has discovered approximately half of the known KBOs. It has
yielded important advances in understanding the belt, enabled
observational research by many other investigators, and stimulated
important theoretical investigations. In order to realize the full
value from the DES, we need to continue to make critical astrometric
observations of any of our survey objects whose orbit is not yet known
accurately enough to permit dynamical classification. This proposal
requests 4-meter time at KPNO and CTIO to continue these essential
observations.
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360
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NOAO > Observing Info > Approved Programs > 2006B-0413 |
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