Rotation Period Determination for (13832) 1999 XR13
Abstract
Photometric observations of the outer main belt asteroid (13832) 1999 XR13 were conducted in order to determine its synodic rotation period. It revealed to be a very slow rotator with P = 98.53 ± 0.04 h, A = 0.31 ± 0.03 mag.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2021
- Bibcode:
- 2021MPBu...48..330M
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods