Lightcurve Photometry and Analysis of 5167 Joeharms
Abstract
Photometric observations were made of the main-belt asteroid 5167 Joeharms from 2024 April 3 to April 16, at an observatory in Beryl Junction, Utah, on iTelescope's T21. Using MPO Canopus, the asteroid was determined to have a rotation period of 5.3204 ± 0.0025h and an amplitude of 0.14.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2024
- Bibcode:
- 2024MPBu...51..314H
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods