CCD Photometry and Lightcurve Analysis of Main Belt Asteroids 1077 Campanula and 1151 Ithaka from Observatori Carmelita
Abstract
Observations carried out in 2011 August and September allowed us to determine the synodic periods of 1077 Campanula and 1151 Ithaka. For 1077 Campanula, a period of 3.850 ± 0.001 h and amplitude of 0.36 mag were found. 1151 Ithaka exhibited an irregularly-shaped lightcurve with a period of 4.932 ± 0.001 h and amplitude of 0.15 mag.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- January 2012
- Bibcode:
- 2012MPBu...39...29A