JOURNAL OF OCCULTATION AND ECLIPSE (JOE); ISSN 2522-7955; No. 1, 2014
Paul D. Maley1
1International Occultation Timing Association, Houston, Texas, USA; pdmaley@yahoo.com
Abstract
Physical models of minor planets depend on their pole of rotation and spin rate. Observations of occultations provide useful information that can, with additional types of information, assist in determination of physical characteristics of asteroids.
Keywords: Asteroid, Rotation, Occultation