Solar system objects observed in the Sloan Digital Sky Survey commissioning data

We discuss measurements of the properties of D13,000 asteroids detected in 500 deg2 of sky in the Sloan Digital Sky Survey (SDSS) commissioning data. The moving objects are detected in the magnitude range 14 \ r* \ 21.5, with a baseline of D5 minutes, resulting in typical velocity errors of D3%. Extensive tests show that the sample is at least 98% complete, with a contamination rate of less than 3%. We —nd that the size distribution of asteroids resembles a broken power law, independent of the heliocentric distance: D~2.3 for 0.4 km, and D~4 for 5

[1]  Harold F. Levison,et al.  A Search for Proto-Comets in the Outer Regions of the Solar System , 1990 .

[2]  Robert Jedicke,et al.  Detection of Near Earth Asteroids Based Upon Their Rates of Motion , 1996 .

[3]  Baryonic dark matter , 1996, astro-ph/9708222.

[4]  et al,et al.  The Sloan Digital Sky Survey Photometric Camera , 1998, astro-ph/9809085.

[5]  Alberto Cellino,et al.  The size distribution of main-belt asteroids from IRAS data , 1991 .

[6]  S. Dermott,et al.  The Collisional Evolution of the Asteroid Belt and Its Contribution to the Zodiacal Cloud , 1997 .

[7]  Xiaohui Fan Simulation of Stellar Objects in SDSS Color Space , 1999 .

[8]  S. Tremaine,et al.  Dark Matter in the Solar System , 1990 .

[9]  D. Lynden-Bell,et al.  A Method of Allowing for Known Observational Selection in Small Samples Applied to 3CR Quasars , 1971 .

[10]  Karri Muinonen,et al.  A Public-Domain Asteroid Orbit Database , 1994 .

[11]  Robert C. Nichol,et al.  Optical and Infrared Colors of Stars Observed by the Two Micron All Sky Survey and the Sloan Digital Sky Survey , 2000 .

[12]  J. Williams,et al.  A Three-Parameter Asteroid Taxonomy , 1989 .

[13]  T. Owen Planets and satellites. , 1981, Science.

[14]  David Morrison,et al.  Surface properties of asteroids - A synthesis of polarimetry, radiometry, and spectrophotometry , 1975 .

[15]  D. L. Rabinowitz,et al.  Detection of earth-approaching asteroids in near real time , 1991 .

[16]  Elitzur,et al.  Infrared Classification of Galactic Objects , 2000, The Astrophysical journal.

[17]  D. Williams,et al.  Size Distribution of Collisionally Evolved Asteroidal Populations: Analytical Solution for Self-Similar Collision Cascades , 1994 .

[18]  R. Jedicke,et al.  The Orbital and Absolute Magnitude Distributions of Main Belt Asteroids , 1998 .

[19]  D. Jewitt KUIPER BELT OBJECTS , 1999 .

[20]  C. Murray,et al.  Variation of the UBV colors of S-class asteroids with semimajor axis and diameter , 1985 .

[21]  D. Rabinowitz,et al.  A reduced estimate of the number of kilometre-sized near-Earth asteroids , 2000, Nature.

[22]  D. J. Tholen,et al.  The Eight-Color Asteroid Survey: Results for 589 Minor Planets , 1985 .

[23]  L. W. Alvarez,et al.  Extraterrestrial Cause for the Cretaceous-Tertiary Extinction , 1980, Science.

[24]  Petr Pravec,et al.  Fast and Slow Rotation of Asteroids , 2000 .

[25]  E. al.,et al.  The Sloan Digital Sky Survey: Technical summary , 2000, astro-ph/0006396.

[26]  Jack Wisdom,et al.  Meteorites may follow a chaotic route to Earth , 1985, Nature.

[27]  Stephan D. Price,et al.  The 2MASS Asteroid and Comet Survey , 1999 .

[28]  J. S. Dohnanyi Collisional model of asteroids and their debris , 1969 .

[29]  Bradley Efron,et al.  A simple test of independence for truncated data with applications to redshift surveys , 1992 .

[30]  Joseph M. Hahn,et al.  Completing the inventory of the solar system , 1996 .

[31]  High-redshift quasars found in sloan digital sky survey commissioning data. IV. Luminosity function from the fall equatorial stripe sample , 2000, astro-ph/0008123.

[32]  Kevin Krisciunas,et al.  The Recognition of Unusual Objects in the Sloan Digital Sky Survey Color System , 1998, astro-ph/9808093.

[33]  D. Bender,et al.  The large-scale structure of the asteroid belt , 1985 .

[34]  S. Bergh Astronomical Catastrophes in Earth History , 1994 .

[35]  Douglas O. ReVelle,et al.  Meteor Phenomena and Bodies , 1998 .

[36]  David Jewitt,et al.  Color Diversity Among the Centaurs and Kuiper Belt Objects , 1996 .

[37]  David L. Rabinowitz,et al.  The size distribution of the earth-approaching asteroids , 1993 .

[38]  S. Tegler,et al.  Two distinct populations of Kuiper-belt objects , 1998, Nature.

[39]  E. Tedesco,et al.  Compositional Structure of the Asteroid Belt , 1982, Science.

[40]  C. J. van Houten,et al.  Survey of Asteroids. , 1958 .

[41]  D. Jewitt,et al.  Discovery of the candidate Kuiper belt object 1992 QB1 , 1993, Nature.

[42]  W J Boyne AIR AND SPACE , 1985 .

[43]  Richard P. Binzel,et al.  Small main-belt asteroid spectroscopic survey: Initial results , 1995 .

[44]  Alberto Cellino,et al.  Asteroid Families. I. Identification by Hierarchical Clustering and Reliability Assessment , 1990 .

[45]  S. Tremaine,et al.  The Origin of Short-Period Comets , 1988 .

[46]  Robert Jedicke,et al.  Collisional Models and Scaling Laws: A New Interpretation of the Shape of the Main-Belt Asteroid Size Distribution☆ , 1998 .

[47]  M. Fukugita,et al.  The Sloan Digital Sky Survey Photometric System , 1996 .

[48]  High-redshift quasars found in sloan digital sky survey commissioning data. III. A color-selected sample at i* <20 in the fall equatorial stripe , 2000, astro-ph/0008122.

[49]  J. B. Oke,et al.  Secondary standard stars for absolute spectrophotometry , 1983 .

[50]  C. Kowal,et al.  A solar system survey , 1989 .

[51]  Julio A. Fernández On the existence of a comet belt beyond Neptune , 1980 .

[52]  Z. Ivezic,et al.  Candidate RR Lyrae Stars Found in Sloan Digital Sky Survey Commissioning Data , 2000, astro-ph/0004130.

[53]  Paolo Persi,et al.  The Impact of Large Scale Near-IR Sky Surveys , 1997 .