Photometric Observations of the Near-Earth Asteroids 1999 AP10 2000 TO64, 2000 UJ1, 2000 XK44, 2001 MZ7, 2003 QO104, 2005 RQ6, 2005 WJ56, and 2009 UN3

Details Photometric Observations of the Near-Earth Asteroids 1999 AP10 2000 TO64, 2000 UJ1, 2000 XK44, 2001 MZ7, 2003 QO104, 2005 RQ6, 2005 WJ56, and 2009 UN3 Photometric Observations of the Near-Earth Asteroids 1999 AP10 2000 TO64, 2000 UJ1, 2000 XK44, 2001 MZ7, 2003 QO104, 2005 RQ6, 2005 WJ56, and 2009 UN3

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010mpbu...37...95b&link_type=abstract

The Minor Planet Bulletin (ISSN 1052-8091). Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Obse

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Scientific paper

The near-Earth asteroids 1999 AP10, 2000 TO64, 2000 UJ1, 2000 XK44, 2001 MZ7, 2003 QO104, 2005 RQ6, 2005 WJ56 and 2009 UN3 were observed by the authors between 2008 January and 2010 February at Salvador (Bahia, Brazil), Mayhill (New Mexico, USA) and Moorook (South Australia, Australia) to determine their Johnson-Cousins BVRI colors and from those, provide an estimate of the Tholen taxonomic classification. From our colors, we found that 1999 AP10, 2000 TO64, 2000 UJ1, 2000 XK44 and 2003 QO104 are probably S-complex members. We reanalysed our previous observations of 2005 WJ56 and confirmed a classification as an X type. The latter results agree with the classifications made by other research groups. We propose that 2001 MZ7 is a G type from its presented colors and G parameter. 2005 RQ6 and 2009 UN3 have colors more similar to Q-types.

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