Numerical Evidence that the Motion of Pluto is Chaotic

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/1721.1/6038

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DC Field	Value	Language
dc.creator	Sussman, Gerald Jay	-
dc.creator	Wisdom, Jack	-
dc.date	2004-10-04T14:36:38Z	-
dc.date	2004-10-04T14:36:38Z	-
dc.date	1988-04-01	-
dc.date.accessioned	2013-10-09T02:42:30Z	-
dc.date.available	2013-10-09T02:42:30Z	-
dc.date.issued	2013-10-09	-
dc.identifier	AIM-1039	-
dc.identifier	http://hdl.handle.net/1721.1/6038	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/xmlui/handle/1721	-
dc.description	The Digital Orrery has been used to perform an integration of the motion of the outer planets for 845 million years. This integration indicates that the long-term motion of the planet Pluto is chaotic. Nearby trajectories diverge exponentially with an e-folding time of only about 20 million years.	-
dc.format	18 p.	-
dc.format	2648967 bytes	-
dc.format	1066764 bytes	-
dc.format	application/postscript	-
dc.format	application/pdf	-
dc.language	en_US	-
dc.relation	AIM-1039	-
dc.subject	dynamics	-
dc.subject	orrery	-
dc.subject	chaos	-
dc.subject	numerical methods	-
dc.subject	Pluto	-
dc.subject	solarssystem	-
dc.title	Numerical Evidence that the Motion of Pluto is Chaotic	-
Appears in Collections:	MIT Items

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