RT Conference Proceedings
T1 A meteoroid from a Jupiter family comet recorded as a bright  bolide in 2012
A1 Romero, A.
A1 Madiedo Gil, José María
A1 Trigo Rodríguez, Josep María
AB The continuous monitoring of meteorand fireball provides information about the originand nature of meteoroids ablating in the Earth's atmosphere,but also about the mechanisms that deliver thesematerials to our planet. Thus, for instance, from theanalysis of meteor events simultaneously imaged from,at least, two different locations it is possible to obtainatmospheric trajectories, radiant, orbital and physicochemicalparameters such as the mass of the meteoroidsand the tensile strengths of these particles [1, 2,3]. In addition, meteor spectroscopy provides helpfulinformation about the chemical nature of meteoroids[5, 6, 7]. With this aim, the SPanish Meteor Network(SPMN) is performing a continuous fireball monitoringand meteor spectroscopy campaign over Spain andneighbouring areas. Here we present orbital andchemical information derived from the analysis of afireball imaged in 2012. This event was produced by ameteoroid from a Jupiter Family Comet.
YR 2013
FD 2013
LK http://hdl.handle.net/10272/9067
UL http://hdl.handle.net/10272/9067
LA eng
NO Romero, A., Madideo Gil, J.M., Trigo Rodriguez, J. M.: "A meteoroid from a Jupiter family comet recorded as a bright  bolide in 2012". En: 44th Lunar and Planetary Science Conference (The Woolands, Texas, march 18-22, 2013)
DS Repositorio Institucional de la Universidad de Huelva
RD 30 may 2026