Lightcurve Analysis of 27810 Daveturner: A Long Period Hungaria

Details Lightcurve Analysis of 27810 Daveturner: A Long Period Hungaria Lightcurve Analysis of 27810 Daveturner: A Long Period Hungaria

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011mpbu...38..150w&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 photometric observations of the Hungaria asteroid 27810 Daveturner were made by a collaboration of three observatories. Analysis of the final data set found a synodic rotation period of P = 540 ± 20 h with a lightcurve amplitude of 0.43 ± 0.03 mag. While the long period makes the asteroid a candidate for being in nonprincipal axis rotation (NPAR or "tumbling"), the data show no signs of such. The long period is hardly unusual since slow rotators are common among the Hungarias, accounting for approximately 30% of those with established rotation rates.

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