A catalog of slow-moving objects extracted from the Sloan Digital Sky Survey: Compilation and applications

Details A catalog of slow-moving objects extracted from the Sloan Digital Sky Survey: Compilation and applications A catalog of slow-moving objects extracted from the Sloan Digital Sky Survey: Compilation and applications

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007phdt........14p&link_type=abstract

Proquest Dissertations And Theses 2007. Section 0330, Part 0606 153 pages; [Ph.D. dissertation].United States -- Illinois: The

Statistics

Applications

Slow-Moving Objects, Sloan Digital Sky Survey, Minor Planets, Comets, Photometry, Astrometry, Transneptunian Objects, Centaurs

Scientific paper

I have compiled the Slow-Moving Object Catalog of Known minor planets and comets ("the SMOCK") by comparing the predicted positions of known bodies with those of sources detected by the Sloan Digital Sky Survey (SDSS) that lack positional counterparts at other survey epochs. For the ~50% of the SDSS footprint that has been imaged only once, I have used the Astrophysical Research Consortium's 3.5-meter telescope to obtain reference images for confirmation of Solar System membership.
The SMOCK search effort includes all known objects with orbital semimajor axes a > 4.7 AU, as well as a comparison sample of inherently bright Main Belt asteroids. In fact, objects of all proper motions are included, resulting in substantial overlap with the SDSS Moving Object Catalog (MOC) and providing an important check on the inclusion criteria of both catalogs. The MOC does not contain any correctly-identified known objects with a > 12 AU, and also excludes a number of detections of Main Belt and Trojan asteroids that happen to be moving slowly as they enter or leave retrograde motion.
The SMOCK catalog is a publicly-available product of this investigation. Having created this new database, I demonstrate some of its applications. The broad dispersion of color indices for transneptunian objects (TNOs) and Centaurs is confirmed, and their tight correlation in ( g - r ) vs ( r - i ) is explored. Repeat observations for more than 30 of these objects allow me to reject the collisional resurfacing scenario as the primary explanation for this broad variety of colors. Trojans with large orbital inclinations are found to have systematically redder colors than their low-inclination counterparts, but an excess of reddish low-inclination objects at L5 is identified. Next, I confirm that non-Plutino TNOs are redder with increasing perihelion distance, and that this effect is even more pronounced among the Classical TNOs. Finally, I take advantage of the byproducts of my search technique and attempt to recover objects with poorly-known orbits. I have drastically improved the current and future ephemeris uncertainties of 3 Trojan asteroids, and have increased by 20%-450% the observed arcs of 10 additional bodies.

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