Analysis of the Lightcurves of 198 Ampella and 2008 SV11

Details Analysis of the Lightcurves of 198 Ampella and 2008 SV11 Analysis of the Lightcurves of 198 Ampella and 2008 SV11

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009mpbu...36..164w&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

We report on our collaborations to obtain photometric data on two asteroids. 198 Ampella, a main-belt object, was observed to check previously reported periods. We found a synodic period of 20.778 ± 0.003 h, which is double that of the most reliable of those previous results. The near-Earth asteroid 2008 SV11 was observed in support of radar observations. We found a period of 32.4 ± 0.1 h. However, the shape of the lightcurve was very unusual and so the period remains in some doubt. Radar observations indicate a strongly bifurcated body.

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