The synodic rotational period of asteroid 4332 Milton


ICARUS, cilt.271, ss.279-282, 2016 (SCI İndekslerine Giren Dergi) identifier identifier


The results of our new photometric observations of the main-belt asteroid 4332 Milton are presented. These observations were obtained on two successive nights in August 2012 at Canakkale University Observatory. The bimodal light curve amplitude and period were determined to be 0.16 +/- 0.01 mag and 3.295 +/- 0.005 h, respectively. (C) 2016 Elsevier Inc. All rights reserved.