The 2019 Mexican Asteroid Photometry Campaign
Abstract
We present photometric optical lightcurves and derived rotation periods for a sample of five asteroids: 722 Frieda (30.06 ± 0.02 h), 1239 Queteleta (10.278 ± 0.003 h), 2162 Anhui (8.101 ± 0.001 h), 4148 McCartney (20.756 ± 0.0006 h), and 4408 Zlata Koruna (4.392 ± 0.001 h). These observations were carried out at the Observatorio Astronómico Nacional at Sierra San Pedro Mártir (OAN-SPM), Baja California, Mexico, the Carl Sagan Observatory (OCS) of the Universidad de Sonora, México, and at the INAOE Tonantzintla Observatory (TONA), Puebla, México.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2020
- Bibcode:
- 2020MPBu...47..340O
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods