Lightcurve Analysis of 1565 Lemaitre

Details Lightcurve Analysis of 1565 Lemaitre Lightcurve Analysis of 1565 Lemaitre

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mpbu...35...52w&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

Scientific paper

The authors observed 1565 Lemaitre independently in August and September 2007. The combined data set was used to determine the synodic period. This proved difficult due to the small amplitude of the lightcurve. We propose a synodic period of either 11.403 ± 0.003 hr (monomodal) with the possibility of 22.805 ± 0.007 hr (bimodal) with an amplitude of 0.04 ± 0.01 mag for either. Given the low amplitude, curves with three or more maxima and minima could not be rejected automatically, however period searches for such possibilities were not convincing.

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