Abstract
CCD photometry of asteroids 970 Primula and 1631 Kopff obtained remotely
at Tenagra Observatories during October and November 2003 is reported. A
synodic rotation period of 2.777±0.001 hours is determined from
four nights of observations for Primula. The resulting rotation period
for Kopff is 6.683±0.001 hours from five nights of observations.
Both observed lightcurves were nearly symmtrical with amplitudes of
0.18±0.02 magnitudes for Primula and 0.41±0.04 for Kopff.
| Original language | English |
|---|---|
| Pages (from-to) | 49-50 |
| Journal | The Minor Planet Bulletin |
| Volume | 31 |
| Publication status | Published - 1 Sept 2004 |