Numerical Evidence that the Motion of Pluto is Chaotic

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

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