10132 Lummelunda: A New Biary Asteroid System
Abstract
CCD photometric observations carried out at several observatories over a wide range of longitudes in 2017 August-September revealed that the main-belt asteroid 10132 Lummelunda is a binary asteroid system with a primary rotational period of 2.5099 ± 0.0001 h and a secondary orbital period of 22.44 ± 0.01 h.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- July 2018
- Bibcode:
- 2018MPBu...45..295B
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods