Lightcurve Analysis of 1084 Tamariwa

Pedro V. Sada

Research output: Contribution to journalArticlepeer-review


Photometric observations of 1084 Tamariwa were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 6.1949 ± 0.0002 h and amplitude of ~0.32 mag.
Original languageEnglish
Pages (from-to)50
JournalThe Minor Planet Bulletin
Publication statusPublished - 1 Jun 2008


Dive into the research topics of 'Lightcurve Analysis of 1084 Tamariwa'. Together they form a unique fingerprint.

Cite this