The Rotation Period of 1117 Reginita
Abstract
The lightcurve of main-belt asteroid 1117 Reginita was determined using images taken at Xingming Observatory (C42) on four nights in 2017 Jan. Analysis of the observations shows a bimodal solution with a synodic rotation period of 2.946 ± 0.001 h and an amplitude of 0.15 mag.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2017
- Bibcode:
- 2017MPBu...44..307T
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods