2006 SQ372: A Likely Long-Period Comet from the Inner Oort Cloud

We report the discovery of a minor planet (2006 SQ372) on an orbit with a perihelion of 24 AU and a semimajor axis of 796 AU. Dynamical simulations show that this is a transient orbit and is unstable on a timescale of ~200 Myr. Falling near the upper semimajor axis range of the scattered disk and th...

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Bibliographic Details
Published in:	The Astrophysical journal 2009-04, Vol.695 (1), p.268-275
Main Authors:	Kaib, Nathan A, Becker, Andrew C, Jones, R. Lynne, Puckett, Andrew W, Bizyaev, Dmitry, Dilday, Benjamin, Frieman, Joshua A, Oravetz, Daniel J, Pan, Kaike, Quinn, Thomas, Schneider, Donald P, Watters, Shannon
Format:	Article
Language:	eng
Subjects:	Astronomy Astrophysics CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS CLOUDS COMETS Earth, ocean, space Exact sciences and technology PLANETS PRODUCTION SIMULATION TRANSIENTS
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Summary:	We report the discovery of a minor planet (2006 SQ372) on an orbit with a perihelion of 24 AU and a semimajor axis of 796 AU. Dynamical simulations show that this is a transient orbit and is unstable on a timescale of ~200 Myr. Falling near the upper semimajor axis range of the scattered disk and the lower semimajor axis range of the Oort Cloud, previous membership in either class is possible. By modeling the production of similar orbits from the Oort Cloud as well as from the scattered disk, we find that the Oort Cloud produces 16 times as many objects on SQ372-like orbits as the scattered disk. Given this result, we believe this to be the most distant long-period comet (LPC) ever discovered. Furthermore, our simulation results also indicate that 2000 OO67 has had a similar dynamical history. Unaffected by the 'Jupiter-Saturn Barrier,' these two objects are most likely LPCs from the inner Oort Cloud.
ISSN:	0004-637X 1538-4357