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The next decade of Solar System discovery with Pan-STARRS

Published online by Cambridge University Press:  01 August 2006

Robert Jedicke ,
E. A. Magnier ,
N. Kaiser  and
K. C. Chambers
Robert Jedicke
Affiliation:
Institute for Astronomy, University of Hawaii, Honolulu, HI, 96822 email: jedicke@ifa.hawaii.edu
E. A. Magnier
Affiliation:
Institute for Astronomy, University of Hawaii, Honolulu, HI, 96822 email: jedicke@ifa.hawaii.edu
N. Kaiser
Affiliation:
Institute for Astronomy, University of Hawaii, Honolulu, HI, 96822 email: jedicke@ifa.hawaii.edu
K. C. Chambers
Affiliation:
Institute for Astronomy, University of Hawaii, Honolulu, HI, 96822 email: jedicke@ifa.hawaii.edu
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Abstract

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The Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) at the University of Hawaii's Institute for Astronomy is a funded project to repeatedly survey the entire visible sky to faint limiting magnitudes (mR ~ 24). It will be composed of four 1.8m diameter apertures each outfitted with fast readout orthogonal transfer Giga-pixel CCD cameras. A single aperture prototype telescopes has achieved first-light in the second half of 2006 with the full system becoming available a few years later. Roughly 60% of the surveying will be suitable for discovery of new solar system objects and it will cover the ecliptic, opposition and low solar-elongation regions. In a single lunation Pan-STARRS will detect about five times more solar system objects than the entire currently known sample. Within its first year Pan-STARRS will have detected 20,000 Kuiper Belt Objects and by the end of its ten year operational lifetime we expect to have found 107 Main Belt objects and achieve ~90% observational completeness for all NEOs larger than ~300m diameter. With these data in hand Pan-STARRS will revolutionize our knowledge of the contents and dynamical structure of the solar system.

Keywords

Surveytelescopeinstrumentationastrometrydata analysisidentificationpopulation models

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