Calculation of the rotational period of the "Mars crosser" asteroid (32910) 1994TE15

Details Calculation of the rotational period of the "Mars crosser" asteroid (32910) 1994TE15 Calculation of the rotational period of the "Mars crosser" asteroid (32910) 1994TE15

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012hell.conf...10a&link_type=abstract

10th Hellenic Astronomical Conference, Proceedings of the conference held at Ioannina, Greece, 5-8 September 2011. Edited by Io

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the lightcurves and the derived rotational period of the inner main belt asteroid (32910) 1994TE15. The asteroid was selected because it seems to have close encounters with the orbit of Mars (Mars crosser). The observations were undertaken during August 2010 at Skinakas Observatory, Crete, using the 1.3m Telescope with an Andor DZ436 CCD camera and a Johnson-Cousins Rlter. The magnitude of the target was 15.3 during the observations and the amplitude of the lightcurve was 0.13 mag.

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