Broad-band photometry of the near-Earth asteroid 154029 (2002 CY46): An unusually steep solar phase curve and evidence for complex rotation.

Details Broad-band photometry of the near-Earth asteroid 154029 (2002 CY46): An unusually steep solar phase curve and evidence for complex rotation. Broad-band photometry of the near-Earth asteroid 154029 (2002 CY46): An unusually steep solar phase curve and evidence for complex rotation.

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2859....1h&link_type=abstract

The Astronomer's Telegram, #2859

Astronomy and Astrophysics

Astronomy

Optical, Asteroids, Planets, Planets (Minor), Solar System Objects

Scientific paper

The near-Earth asteroid 154029 (2002 CY46) was discovered on 1998 February 11 by the LINEAR survey (MPEC 2002-C89). In anticipation of planned radar observations by the JPL planetary radar group, we obtained four nights of Bessel BVRI observations and two nights of R photometry at the JPL Table Mountain Observatory (TMO) 0.6-m telescope [Figure 1].

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