Analysis of the lightcurve for 6249 Jennifer

Details Analysis of the lightcurve for 6249 Jennifer Analysis of the lightcurve for 6249 Jennifer

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006mpbu...33...23w&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

In 2002, the second author (Gross) observed the Hungaria group member, 6249 Jennifer, and derived a synodic period based on a bimodal curve of 4.950±0.003h with a 0.45±0.03 mag. amplitude. In mid-2005, the first author (Warner) observed the same asteroid and confirms the result with a 4.9535±0.0009h period and 0.14±0.02 mag. amplitude, based on a monomodal curve, likely indicating the 2005 apparition being nearly pole-on.

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