Inner Solar System Studies in the Era of the Next Generation Wide Field Sky Surveys

Details Inner Solar System Studies in the Era of the Next Generation Wide Field Sky Surveys Inner Solar System Studies in the Era of the Next Generation Wide Field Sky Surveys

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.5604j&link_type=abstract

American Astronomical Society Meeting 210, #56.04; Bulletin of the American Astronomical Society, Vol. 39, p.167

Astronomy and Astrophysics

Astronomy

Scientific paper

The Next Generation Wide Field Sky Surveys (e.g. Pan-STARRS, LSST, SkyMapper) will provide more than an order of magnitude increase in the number of known asteroids and comets in the inner solar system along with significantly better astrometric positions, consistent and accurate multi-color photometry, and regular recovery for light-curve analysis and orbit determination. I will discuss the challenges and solutions associated with processing the high detection rates in the Pan-STARRS and LSST Moving Object Processing Systems (MOPS) as well as new inner solar system asteroid and comet science enabled by these remarkable data sets.

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