Lightcurves for 91 Aegina, 235 Carolina, 1117 Reginita, and (505657) 2014 SR339
Abstract
Photometric observations of three main-belt and one near-Earth asteroids were made in order to acquire lightcurves for shape/spin axis models. For 91 Aegina, the synodic rotation period is 6.029 ± 0.001 h, amplitude 0.19 mag. For 235 Carolina, the synodic rotation period is 17.61 ± 0.01 h, amplitude 0.31 mag. For 1117 Reginita, the synodic rotation period is 2.9467 ± 0.0001 h, amplitude 0.19 mag. For (505657) 2014 SR339, the synodic rotation period is 8.71 ± 0.01 h, amplitude 0.75 mag.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2018
- Bibcode:
- 2018MPBu...45..399F
- Keywords:
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- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods