CCD Photometry and Lightcurve Analysis of 1730 Marceline and 1996 Adams from Observatori Carmelita in Tiana

Details CCD Photometry and Lightcurve Analysis of 1730 Marceline and 1996 Adams from Observatori Carmelita in Tiana CCD Photometry and Lightcurve Analysis of 1730 Marceline and 1996 Adams from Observatori Carmelita in Tiana

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011mpbu...38...55a&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

Analysis of observations carried out during 2010 September and October determined the synodic periods of 1730 Marceline (1936 UA) and 1996 Adams (1961 UA). For main-belt asteroid 1730 Marceline, a period of 3.837 ± 0.001 h was found. For 1996 Adams, also an MBA, a period of 3.311 ± 0.001 h was determined. This differs from the period of 3.56 h found by Alvarez-Candal et al. (2004).

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