The continuous monitoring of meteor
and fireball provides information about the origin
and nature of meteoroids ablating in the Earth's atmosphere,
but also about the mechanisms that deliver these
materials to our planet. Thus, for instance, from the
analysis of meteor events simultaneously imaged from,
at least, two different locations it is possible to obtain
atmospheric trajectories, radiant, orbital and physicochemical
parameters such as the mass of the meteoroids
and the tensile strengths of these particles [1, 2,
3]. In addition, meteor spectroscopy provides helpful
information about the chemical nature of meteoroids
[5, 6, 7]. With this aim, the SPanish Meteor Network
(SPMN) is performing a continuous fireball monitoring
and meteor spectroscopy campaign over Spain and
neighbouring areas. Here we present orbital and
chemical information derived from the analysis of a
fireball imaged in 2012. This event was produced by a
meteoroid from a Jupiter Family Comet
