A revised shape model of asteroid (216) Kleopatra
نویسندگان
چکیده
منابع مشابه
Adaptive optics observations of asteroid (216) Kleopatra
The large main-belt asteroid (216) Kleopatra has been for long suspected to be a binary object, mainly due to its large lightcurve amplitude. However, recent observations suggest that it is a single “bone-shaped” or bi-lobated body (Ostro et al. 2000; Tanga et al. 2001). We present results obtained from ground-based adaptive optics observations, and in agreement with the radar raw-observations,...
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Interferometric observations of asteroid (216) Kleopatra were performed in January 2000 using the Fine Guidance Sensors (FGS) aboard HST. The FGS data obtained clearly suggest that (216) Kleopatra is composed of two lobes in contact, in agreement with the radar data (Ostro et al. 2000, Science 288, 836–839), and provide more precise constraints on the absolute size of this peculiar object. c © ...
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ژورنال
عنوان ژورنال: Icarus
سال: 2018
ISSN: 0019-1035
DOI: 10.1016/j.icarus.2018.04.002