Differential Photometry And Lightcurve Analysis For Numbered Asteroids 229, 275, 426, 557, 613, 741, 788, 872, 907, And 5010

Details Differential Photometry And Lightcurve Analysis For Numbered Asteroids 229, 275, 426, 557, 613, 741, 788, 872, 907, And 5010 Differential Photometry And Lightcurve Analysis For Numbered Asteroids 229, 275, 426, 557, 613, 741, 788, 872, 907, And 5010

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21340112p&link_type=abstract

American Astronomical Society, AAS Meeting #213, #401.12; Bulletin of the American Astronomical Society, Vol. 41, p.190

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Partial lightcurves for asteroids 229 Adelinda, 275 Sapientia, 426 Hippo, 613 Ginevra, 741 Botolphia, 788 Hohensteina, 872 Holda, and 907 Rhoda are presented within this paper. Approximate rotation periods are suggested for 275 Sapientia, 613 Ginevra, and 872 Holda. Complete lightcurves for asteroids 557 Violetta and 5010 Amenemhet are presented within this paper. 557 Violetta was found to have a rotation period of 5.1 ± 0.1 hrs with an amplitude of 0.215 ± 0.044 magnitude (mag). No alternate rotation period or confirmation of the published period is suggested for 5010 Amenemhet. 613 Ginevra was observed during November and December, 2006. Numbered asteroids 741 and 872 were observed during March, 2007. 275 Sapientia was observed during January, 2008. Numbered asteroids 426, 557, and 907 were observed during April, 2008; 229, 788, and 5010 were observed during June, 2008. All observations were taken using the SARA 0.9 meter telescope at the Kitt Peak National Observatory.

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