Abstract
CCD photometry of six asteroids was obtained at the Universidad de
Monterrey Observatory during January and February 2008. The resulting
synodic rotation periods and amplitudes are as follows: 1292 Luce,
6.9541 ± 0.0002 h, 0.20 ± 0.01 mag; 1303 Luthera, 5.878
± 0.003 h, 0.08 ± 0.01 mag; 1900 Katyusha, 9.4999
± 0.0001 h, 0.72 ± 0.02 mag, 2807 Karl Marx, 8.842
± 0.001 h, 0.40 ± 0.05 mag; 3409 Abramov, 7.791 ±
0.002 h, 0.55 ± 0.02 mag; and 9117 Aude, 2.8156 ± 0.0001
h, 0.20 ± 0.01 mag.
| Original language | English |
|---|---|
| Pages (from-to) | 105-107 |
| Journal | The Minor Planet Bulletin |
| Volume | 35 |
| Publication status | Published - 1 Sept 2008 |