Lightcurves and Synodic Periods for Asteroids 1998 ST49, (13154) and (27529)

Details Lightcurves and Synodic Periods for Asteroids 1998 ST49, (13154) and (27529) Lightcurves and Synodic Periods for Asteroids 1998 ST49, (13154) and (27529)

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007em%26p..100...77g&link_type=abstract

Earth, Moon, and Planets, Volume 100, Issue 1-2, pp. 77-82

Physics

Minor Planets, Asteroids, Photometry

Scientific paper

The first photometric observations of the near-Earth asteroid 1998 ST49 and the main belt asteroids (13154) and (27529) are reported. The synodic rotation periods and amplitudes of the lightcurves are: - 2.3017 h, 0.11 mag for 1998 ST49; - 2.98502 h, 0.18 mag for (13154); - 4.1290 h, 0.51 mag for (27529). The periods for the first two asteroids are unambiguous, while the period of 4.1570 h is not ruled out for the third asteroid. Despite fast rotations, none of the presented asteroids exhibited any sign of binarity. Lightcurves were obtained at Modra Observatory.

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