The first near-infrared (0.9 m) photometric observations of Saturn's five medium-sized satellites were obtained during the In this paper we report on the analysis of nearly 300 August 1995 ring plane crossing with Palomar Observatory's images obtained in the near infrared during the RPX of 60-in. te
HST Observations of Saturnian Satellites during the 1995 Ring Plane Crossings
β Scribed by Colleen A. McGhee; Philip D. Nicholson; Richard G. French; Katherine J. Hall
- Publisher
- Elsevier Science
- Year
- 2001
- Tongue
- English
- Weight
- 889 KB
- Volume
- 152
- Category
- Article
- ISSN
- 0019-1035
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β¦ Synopsis
Hubble Space Telescope (HST) observations during Saturn's ring-plane crossings allowed us to view saturnian satellites normally hidden to Earth-based observers in the glare of the rings. New measurements of Janus, Epimetheus, Prometheus, and Pandora have been combined to form revised orbital solutions using all three HST data sets. These measurements and orbit fits are presented, as well as similar fits for the brighter satellites Mimas, Tethys, Enceladus, Dione, and Rhea. Observations of the Lagrangian satellites Telesto, Calypso, and Helene are also reported. While most satellites were found to be close to their expected positions based on previous orbital solutions (Nicholson
π SIMILAR VOLUMES
We report the first absolutely calibrated photometry of nine saturnian satellites beyond 1.0 Β΅m, in canonical near-infrared filters, including the first such spectrum of the leading side of Enceladus. The satellites were observed during Ring Plane Crossing in August and September of 1995 with the NS
main rings are viewed edge-on and so reflect very little sunlight toward Earth. In this note, we discuss the first ground-based detection of Saturn's We report the first ground-based detection of Saturn's G G ring and the first infrared images of the E ring. ring, together with the first infrared im
The crossings of Saturn's ring plane by Earth were observed in the near infrared on May 22 and August 10, 1995, from the 2.2-m telescope of the University of Hawaii, the 2-m telescope at Pic du Midi, France, and with the Adonis adaptive optics camera at the 3.6-m telescope of the European Southern O