| dc.creator | Branham, Richard Lacy | |
| dc.date.accessioned | 2016-03-14T15:09:44Z | |
| dc.date.accessioned | 2018-11-06T12:27:08Z | |
| dc.date.available | 2016-03-14T15:09:44Z | |
| dc.date.available | 2018-11-06T12:27:08Z | |
| dc.date.created | 2016-03-14T15:09:44Z | |
| dc.date.issued | 2013-07-02 | |
| dc.identifier | Branham, Richard Lacy; Orbit of comet C/1854 L1 (Klinkerfues); Elsevier; Planetary And Space Science; 85; 2-7-2013; 289-292 | |
| dc.identifier | 0032-0633 | |
| dc.identifier | http://hdl.handle.net/11336/4765 | |
| dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/1866784 | |
| dc.description.abstract | Comet C/1854 L1 (Klinkerfues) is one of a large number of comets with parabolic orbits. Given that there are sufficient observations of the comet, 262 in right ascension and 260 in declination, it proves possible to calculate a better orbit. The calculations are based on a 12th order predictor–corrector method. The comet's orbit is highly elliptical, e=0.99866 and, from calculated mean errors, statistically different from a parabola. The comet will not return for at least 10,400 years and thus represents no immediate NEO threat. | |
| dc.language | eng | |
| dc.publisher | Elsevier | |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0032063313001645 | |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.pss.2013.06.023 | |
| dc.relation | info:eu-repo/semantics/altIdentifier/issn/0032-0633 | |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | |
| dc.rights | info:eu-repo/semantics/restrictedAccess | |
| dc.subject | CELESTIAL MECHANICS | |
| dc.subject | COMETS INDIVIDUAL | |
| dc.subject | METHODS-DATA ANALYSIS | |
| dc.title | Orbit of comet C/1854 L1 (Klinkerfues) | |
| dc.type | Artículos de revistas | |
| dc.type | Artículos de revistas | |
| dc.type | Artículos de revistas | |
