Rotation Period Determination for the Mars-Crossing Asteroid (97514) 2000 Dl1
Abstract
Photometric observations of the Mars-crossing asteroid (97514) 2000 DL1 were conducted in order to determine its synodic rotation period. The asteroid is certainly a slow rotator and the period has not been completely covered by our observations. We present the most likely bimodal solution with a period of P = 163.6 ± 0.3 h, A = 0.47 ± 0.09 mag.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- July 2023
- Bibcode:
- 2023MPBu...50..195M
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods