Lightcurve Analysis of 1654 Bojeva
Abstract
Photometric observations of main-belt asteroid 1654 Bojeva were made over six nights during 2015 October and November. Remote observations were made using iTelescope Observatory (MPC H06) in Mayhill, New Mexico. Lightcurve analysis using MPO Canopus found a possible rotation period of 10.5559 ± 0.0137 h with an amplitude of 0.27 mag.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- April 2016
- Bibcode:
- 2016MPBu...43..122H