A fireball produced by a meteoroid belonging to the delta aquilids stream

Nieto, R.; Madiedo Gil, José María; Ortiz Moreno, José Luis; Castro Tirado, Alberto J.; Trigo Rodríguez, Josep María; Zamorano, J.; Izquierdo Gómez, Jaime; Ocaña Gónzalez, Francisco; Sánchez de Miguel, A.; Pastor, S.; Reyes, J. A. de los

Author

Nieto, R.; Madiedo Gil, José María ; Ortiz Moreno, José Luis; Castro Tirado, Alberto J.; Trigo Rodríguez, Josep María; [et al.]
Publication Date

2013
Citation

Nieto, R. ; Madiedo Gil, José María ; Ortiz Moreno, José Luis ; Castro Tirado, Alberto J. ; Trigo Rodríguez, J.M., Zamorano, J., Izquierdo Gómez, J., Ocaña Gónzalez, F., Sánchez de Miguel, A., Pastor, S., Reyes, J. A. de los: "A fireball produced by a meteoroid belonging to the delta aquilids stream". En: 44th Lunar and Planetary Science Conference (The Woolands, Texas, march 18-22, 2013)
Abstract

According to Jenniskens [1], the δ- Aquilids are active from April 10 to April 16, with a maximum peak around April 13. It is currently included in the IAU working list of meteor showers with code 131 DAL. The proposed parent body of the DAL stream is comet C/1984 S1 (Meier). The calculation of precise orbital elements can be very helpful to improve our knowledge about this poorly-known shower. Highsensitivity CCD devices can be very helpful for this purpose, as these provide information about different physico-chemical parameters of meteoroids ablating in the atmosphere [2, 3, 4]. We present here the analysis of a DAL bolide imaged in the framework of the continuous meteor and fireball monitoring campaign developed by the SPanish Meteor Network (SPMN).
URI

http://hdl.handle.net/10272/9045

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A fireball produced by a meteoroid belonging to the delta aquilids stream

Author

Nieto, R.; Madiedo Gil, José María UHU Authority

; Ortiz Moreno, José Luis; Castro Tirado, Alberto J.; Trigo Rodríguez, Josep María; [et al.]

Publication Date

2013

Citation

Nieto, R. ; Madiedo Gil, José María ; Ortiz Moreno, José Luis ; Castro Tirado, Alberto J. ; Trigo Rodríguez, J.M., Zamorano, J., Izquierdo Gómez, J., Ocaña Gónzalez, F., Sánchez de Miguel, A., Pastor, S., Reyes, J. A. de los: "A fireball produced by a meteoroid belonging to the delta aquilids stream". En: 44th Lunar and Planetary Science Conference (The Woolands, Texas, march 18-22, 2013)

Abstract

According to Jenniskens [1], the δ- Aquilids are active from April 10 to April 16, with a maximum peak around April 13. It is currently included in the IAU working list of meteor showers with code 131 DAL. The proposed parent body of the DAL stream is comet C/1984 S1 (Meier). The calculation of precise orbital elements can be very helpful to improve our knowledge about this poorly-known shower. Highsensitivity CCD devices can be very helpful for this purpose, as these provide information about different physico-chemical parameters of meteoroids ablating in the atmosphere [2, 3, 4]. We present here the analysis of a DAL bolide imaged in the framework of the continuous meteor and fireball monitoring campaign developed by the SPanish Meteor Network (SPMN).

URI

http://hdl.handle.net/10272/9045

Fichero	Tamaño	Formato	Ver	Description
A fireball_and_planetary.pdf	194.7Kb	PDF	View/Open	versión editor

Fichero	Tamaño	Formato	Ver	Description
A fireball_and_planetary.pdf	194.7Kb	PDF	View/Open	versión editor