RT Conference Proceedings
T1 Spectra of bolides produced by meteoroids from (3200) phaeton
A1 Moreno, A.
A1 Madiedo Gil, José María
A1 Trigo Rodríguez, Josep María
AB The Geminids is the densest annualmeteoroid stream whose parent body is asteroid (3200)Phaethon, which was considered by some researchersas an extinct cometary nucleus rather than a regularasteroid [1]. On the basis of spectral and dynamicalsimilarities, it has been recently proposed that asteroid2 Pallas is the likely parent body of asteroid (3200)Phaeton [2, 3]. The asteroidal origin of the Geminidssuggests that this stream could be a potential meteoriteproducer. The analysis of several Geminid fireballsobserved between 2009 and 2010 from Spain supportsthis idea [4]. In this work we present the preliminaryanalysis of four emission spectra produced by meteoroidsfrom the Geminids stream. These were obtainedin the framework of the continuous spectroscopic campaigndeveloped by the SPanish Meteor Network(SPMN).
YR 2013
FD 2013
LK http://hdl.handle.net/10272/9389
UL http://hdl.handle.net/10272/9389
LA eng
NO Moreno, A., Madiedo Gil, J.M., Trigo Rodríguez, J.M.: "Spectra of bolides produced by meteoroids from (3200) phaeton". 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