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Orbital Elements of 2004 Perseid Meteoroids Perturbed by Jupiter
Authors:Josep Maria Trigo-Rodriguez  Jeremie Vaubaillon  José Luís Ortiz  Alberto Castro-Tirado  Jordi Llorca  Esko Lyytinen  Martin Jelínek  Antonio de Ugarte Postigo  Pablo Santos Sanz  Francisco J Aceituno Castro  Albert Sánchez Caso  Antonio Bernal González  Juan Pastor Erades  Francisco Ocaña
Institution:(1) Institut Ciències de l’Espai – CSIC, Campus UAB, Facultat de Ciències, Torre C5-parell-2a, 08193 Bellaterra, Barcelona, Spain;(2) Institut d’Estudis Espacials de Catalunya (IEEC), Edif. Nexus, c/Gran Capità, 2-4, 08034 Barcelona, Spain;(3) University of Western Ontario, London, Ontario, Canada;(4) Instituto de Astrofísica de Andalucía (IAA-CSIC), PO Box 3004, 18080 Granada, Spain;(5) Universitat Politècnica de Catalunya, Barcelona, Spain;(6) Kehakukantie 3 B, 00720 Helsinki, Finland;(7) Gualba Observatory, MPC 442, Barcelona, Spain;(8) Asociación Astronómica de Castelldefels, Barcelona, Spain;(9) Agrupació Astronòmica de Sabadell, Barcelona, Spain;(10) Agrupación Astronómica de Madrid, Madrid, Spain
Abstract:Jupiter and Saturn produce important gravitational impulses on meteoroids released by comet 109P/Swift-Tuttle. The meteoroids from this comet once released follow retrograde orbits that during their periodic approaches to these planets (within 1.6 and 0.9 A.U., respectively) are impulsed gaining orbital energy. This perturbation effect is translated into a net inward shift in the node of the perturbed meteoroids. Such geometry with Jupiter occurred in 2004 over a meteoroid trail ejected by this comet during the 1862 A.D. return of the comet to perihelion. In order to study the predicted outburst produced by one-revolution meteoroids, the Spanish Photographic Meteor Network (SPMN) performed an extensive campaign. As a part of this observational effort here are presented 10 accurate meteoroid orbits. We discuss their origin by comparing them with the theoretical orbital elements of the dust trails intercepting the Earth during the 2004 Perseid return.
Keywords:109P/Swift-Tuttle  perseids  meteors  meteor outburst  dust trail
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