The lightcurve for the Hungaria asteroid 4232 Aparicio

Details The lightcurve for the Hungaria asteroid 4232 Aparicio The lightcurve for the Hungaria asteroid 4232 Aparicio

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006mpbu...33...24w&link_type=abstract

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

Physics

Minor Planets, Light Curves

Scientific paper

Photometric observations of 4232 Aparicio, a member of the Hungaria class, were made from late August to late September 2005. The majority of the data revealed a likely synodic period of 54.4±0.1h and amplitude of 0.82±0.02m. However, a small subset of the data do not fit with this solution. Given the approximate size and period of the object, there remains the possibility that it may have non-principal axis rotation, i.e., it is a tumbler.

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