Extended ring system of Uranus

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	2011-01-11T06:15:13Z
dc.date.available	2011-01-11T06:15:13Z
dc.date.issued	1979
dc.identifier.citation	This article is taken from ADS database	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/775
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 analysed 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 alos present around the planet in the equatorial plane.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	emp21-393
dc.subject	Solar System, Uranus - Planet	en_US
dc.title	Extended ring system of Uranus	en_US
dc.type	Article	en_US