PI: Robert S. McMillan, U. Ariz., firstname.lastname@example.org
Address: LPL, 1629 East University Blvd., Tucson, AZ 85721, USA
CoI: Jeff Larsen, U. S. Naval Academy
CoI: Jim Scotti, U. Ariz.
CoI: Terry Bressi, U. Ariz.
CoI: Tim Spahr, Harvard-Smithsonian CfA
CoI: Chet Maleszewski, U. Ariz.
Title: Astrometry and Photometry of Faint, High Priority Solar System Objects
Abstract: \raggedright We request MOSAIC 1.1 on the Mayall 4-meter telescope to improve knowledge of the orbits and magnitudes of high priority classes of Near Earth Objects (NEOs) and other small solar system bodies that cannot be reached with our Spacewatch telescopes. Targets include freshly discovered virtual impactors (VIs), other close approachers, and NEOs discovered by the NEOWISE spacecraft. It is better to follow objects longer during their discovery apparitions than to search tens of degrees of arc for them when they return years later, hence the need to reach fainter magnitudes on short notice. About half of our targets are therefore unknown at the time of this proposal. Other targets for recovery include future targets of radar, NEOs previously detected by WISE with orbits or albedos suggesting potential for cometary activity, potential destinations for spacecraft, and returning NEOs with hard-won albedos and diameters determined by WISE that need astrometry. Our past use of the Mayall telescope has been determined by Co-Investigator Tim Spahr of the Minor Planet Center to provide ``dramatic improvement'' to orbits.
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