Lightcurve Analysis for Sixteen Main-Belt Asteroids
Abstract
Photometric observations of sixteen main-belt asteroids were obtained on the nights from 2022 August - December. We derived the following rotational periods: 1055 Tynca 11.893 ± 0.001 h, 1417 Walinskia, 1500 Jyvaskyla 8.827 ± 0.0002 h, 2003 Harding 4.453 ± 0.001 h, 2695 Christabel 5.623 ± 0.004 h, 3686 Antoku 6.744 ± 0.006 h, 4528 Berg 3.564 ± 0.001 h, 5501 1982 FF2 2.464 ± 0.002 h, 5643 Roques 7.490 ± 0.03 h, 7195 Danboice 8.689 ± 0.007 h, 7317 Cabot 2.345 ± 0.002 h, 12999 Torun 4.020 ± 0.002 h, 15476 Narendra, 19750 2000 CM62 6.518 ± 0.001 h, 23892 1998 SH49 3.722 ± 0.001 h, 33697 1999 KJ11 4.876 ± 0.003 h.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- July 2023
- Bibcode:
- 2023MPBu...50..183F
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods