Other
Scientific paper
Jul 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..248..130s&link_type=abstract
A Giant Step: from Milli- to Micro-arcsecond Astrometry, Proceedings of the International Astronomical Union, IAU Symposium, Vol
Other
Occultations, Minor Planets, Asteroids, Binaries: Close
Scientific paper
The occultation of a 9.1 magnitude star by asteroid (22) Kalliope and its satellite Linus was successfully observed in Japan in 2006 November 7.826 UT. This was the first definite observation of an occultation of a satellite of an asteroid that was discovered previously by other means. As a result the position of the satellite relative to Kalliope was obtained to be d = 0.246 ± 0.011 (arcsec), and P = 313.8 ± 2.7 (deg), where d is the angular distance and P is the position angle. The derived size for Kalliope is (209 ± 40)km × (136 ± 26)km (with the major axis in position angle of (8 ± 17) deg), and that for Linus is (33 ± 3) km. From the observations, the occulted star is also found to be a close double star whose separation is about 0.7 mas in position angle of about 300 deg, and the magnitudes of the components are found to be almost the same (~9.9 mag).
Hayamizu Tsutomu
Hirose Tachishige
Miyashita Kazuhisa
Setoguchi T.
Soma Makoto
No associations
LandOfFree
Occultation by (22) Kalliope and its satellite Linus does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Occultation by (22) Kalliope and its satellite Linus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Occultation by (22) Kalliope and its satellite Linus will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1322041