Orbits of comets C/1848 P1 (Petersen) and C/1848 U1 (Petersen)

dc.creatorBranham, Richard Lacy
dc.date.accessioned2017-12-29T17:59:00Z
dc.date.accessioned2018-11-06T15:47:53Z
dc.date.available2017-12-29T17:59:00Z
dc.date.available2018-11-06T15:47:53Z
dc.date.created2017-12-29T17:59:00Z
dc.date.issued2014-08
dc.identifierOrbits of comets C/1848 P1 (Petersen) and C/1848 U1 (Petersen); Pergamon-Elsevier Science Ltd.; Planetary and Space Science; 103; 103; 8-2014; 286-290
dc.identifier0032-0633
dc.identifierhttp://hdl.handle.net/11336/31928
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1901177
dc.description.abstractComets C/1848 P1 (Petersen) and C/1848 U1 (Petersen) are ones of a large number of comets with parabolic orbits. Given that there are sufficient observations, 67 in right ascencion and 61 in declination for the former and 144 in right ascension and 144 in declination for the latter, it proves to be possible to calculate better orbits. The C/1848 P1's orbit is hyperbolic, although statistically indistinguishable from a parabola. This object, therefore, cannot be considered as an NEO. C/1848 U1's orbit is also hyperbolic, but with no indication of a possible extrasolar origin.
dc.languageeng
dc.publisherPergamon-Elsevier Science Ltd.
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0032063314002645
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.pss.2014.08.014
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectCELESTIAL MECHANICS
dc.subjectCOMETS: INDIVIDUAL
dc.subjectMETHODS: DATA ANALYSIS
dc.subjectComets
dc.subjectIndividual Methods
dc.subjectData analysis
dc.titleOrbits of comets C/1848 P1 (Petersen) and C/1848 U1 (Petersen)
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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