Extended ring system of Uranus

Bhattacharyya, J. C; Bappu, M. K. V; Mohin, S; Mahra, H. S; Gupta, S. K

dc.contributor.author	Bhattacharyya, J. C
dc.contributor.author	Bappu, M. K. V
dc.contributor.author	Mohin, S
dc.contributor.author	Mahra, H. S
dc.contributor.author	Gupta, S. K
dc.date.accessioned	2007-11-29T09:21:35Z
dc.date.available	2007-11-29T09:21:35Z
dc.date.issued	1979-12
dc.identifier.citation	The Moon and the Planets, Vol. 21, Dec, pp. 393-404	en
dc.identifier.uri	http://hdl.handle.net/2248/1990
dc.description.abstract	Two photoelectric records of the occultation event on 10 March, 1977, obtained by two 102-cm-aperture telescopes, spaced 1500 km apart, are critically analyzed and indications of a complex structure of distribution of occulting material surrounding the planet are obtained. The results confirm the existence of a very shallow broad ring system with local condensation lanes of narrow and intermediate widths. A system of numerous thin rings are also present around the planet in the equatorial plane.	en
dc.format.extent	803505 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1979M%26P....21..393B	en
dc.subject	Astronomical Models	en
dc.subject	Electrophotometers	en
dc.subject	Planetary Structure	en
dc.subject	Uranus Rings	en
dc.subject	M.K.V. Bappu	en
dc.title	Extended ring system of Uranus	en
dc.type	Article	en