Photometric Observations and Analysis of 604 Tekmessa

Details Photometric Observations and Analysis of 604 Tekmessa Photometric Observations and Analysis of 604 Tekmessa

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011mpbu...38..195b&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

CCD observations of the main-belt asteroid 604 Tekmessa were recorded during the period 2010 September to December. Analysis of the lightcurve found a synodic period of P = 5.5596 ± 0.0001 h and amplitude A = 0.49 ± 0.01 mag. The phase curve referenced to mean magnitude suggests the absolute magnitude and phase slope parameter H = 9.435 ± 0.014 and G = 0.112 ± 0.013. The phase curve referenced to maximum light suggests H = 9.279 ± 0.018 and G = 0.165 ± 0.017.

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