Lightcurve Analysis of Asteroid 2685 Masursky
Abstract
Photometric observations of the main-belt asteroid 2685 Masursky were conducted to determine the asteroid's synodic rotation period. Three telescopes based in Malta and Australia were used. The authors found a synodic rotation period of P = 59.531 ± 0.052 h with an amplitude of A = 1.26 mag.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- January 2023
- Bibcode:
- 2023MPBu...50...11H
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods