Lightcurve Analysis for Eight Main-belt and Three Near-Earth Asteroids
Abstract
Photometric observations of eight main-belt asteroids and three NEAs were obtained between 2023/8 - 2023/12. We derived the following rotational synodic periods: 353 Ruperto-Carola, 2.7389 ± 0.000016 h; 452 Hamiltonia, 2.88119 ± 0.00007 h; 914 Palisana, 8.68062 ± 0.00017 h; 1554 Yugoslavia, 3.8873 ± 0.0002 h; 2729 Urumqi, 3.127840 ± 0.000024 h; 4917 Yurilvovia, 10.169 ± 0.018 h; 8142 Zolotov, 4.32388 ± 0.00005 h; (6037) 1988 EG, 2.75724 ± 0.00036 h; 15817 Lucianotesi, 12.687 ± 0.005 h; (41437) 2000 GT122, 2.99011 ± 0.00035 h; (154244) 2002 KL6, 4.60721 ± 0.00002 h. And the following sidereal periods: 452 Hamiltonia: 2.881314 ± 0.000002 h; 1554 Yugoslavia: 3.88762 ± 0.000003; 8142 Zolotov: 4.323410 ± 0.000003 h.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- April 2024
- Bibcode:
- 2024MPBu...51..169F
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods