Lightcurve Analysis of 669 Kypria

Craig S. Bennefeld, Pedro V. Sada

Research output: Contribution to journalArticlepeer-review


Photometric observations of 669 Kypria were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 14.283 ± 0.001 h and amplitude of ~0.60 mag.
Original languageEnglish
Pages (from-to)87-88
JournalThe Minor Planet Bulletin
Publication statusPublished - 1 Jun 2008


Dive into the research topics of 'Lightcurve Analysis of 669 Kypria'. Together they form a unique fingerprint.

Cite this