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A SEARCH FOR DISTANT SOLAR SYSTEM BODIES IN THE REGION OF SEDNA

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Megan E. Schwamb1, Michael E. Brown1 and David L. Rabinowitz2

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We present the results of a wide-field survey for distant Sedna-like bodies in the outer solar system using the 1.2 m Samuel Oschin Telescope at Palomar Observatory. We searched ~12,000 deg2 down to a mean limiting magnitude of 21.3 in R. A total number of 53 Kuiper Belt objects and Centaurs have been detected, 25 of which were discovered in this survey. No additional Sedna-like bodies with perihelia beyond 70 AU were found despite a sensitivity to motions out to ~1000 AU. We place constraints on the size and distribution of objects on Sedna orbits.


Keywords

Kuiper Belt; Oort Cloud; solar system: formation


PACS

96.30.Xa 

96.30.Ys Asteroids (minor planets)

96.12.Bc Origin and evolution

96.12.De Orbital and rotational dynamics

95.55.Ev Solar instruments

Subjects

Instrumentation and measurement

Astrophysics and astroparticles

Dates

Issue 1 (2009 March 20)

Received 2009 January 7, accepted for publication 2009 January 27

Published 2009 February 26



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