The Fireball of November 24, 1970, as the Most Probable Source of the Ischgl Meteorite
Fuente:
arXiv
Guardado en:
| Autores principales: | , , , , , , , , , , , , , , , |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
| _version_ | 1866910414513635328 |
|---|---|
| author | Gritsevich, Maria Moilanen, Jarmo Visuri, Jaakko Meier, Matthias M. M. Maden, Colin Oberst, Jürgen Heinlein, Dieter Flohrer, Joachim Castro-Tirado, Alberto J. Delgado-García, Jorge Koeberl, Christian Ferrière, Ludovic Brandstätter, Franz Povinec, Pavel P. Sýkora, Ivan Schweidler, Florian |
| author_facet | Gritsevich, Maria Moilanen, Jarmo Visuri, Jaakko Meier, Matthias M. M. Maden, Colin Oberst, Jürgen Heinlein, Dieter Flohrer, Joachim Castro-Tirado, Alberto J. Delgado-García, Jorge Koeberl, Christian Ferrière, Ludovic Brandstätter, Franz Povinec, Pavel P. Sýkora, Ivan Schweidler, Florian |
| contents | In June 1976, a pristine meteorite stone weighing approximately 1 kg, fully covered with a fresh black fusion crust, was collected on a mountain road in the high-altitude Alpine environment. The recovery took place while clearing the remnants of a snow avalanche, 2 km northwest of Ischgl in Austria. Subsequent to its retrieval, the specimen remained in the finder's private residence without undergoing any scientific examination or identification until 2008, when it was brought to the University of Innsbruck. The sample was classified as a well-preserved LL6 chondrite, with a W0 weathering grade, implying a relatively short time between the meteorite fall and its retrieval. To investigate the potential connection between the Ischgl meteorite and a recorded fireball event, we have reviewed all documented fireballs ever photographed by German fireball camera stations. This examination led us to identify the fireball EN241170 observed in Germany by ten different European Network stations on the night of November 23/24, 1970, as the most likely candidate. We employed state-of-the-art techniques to reconstruct the fireball's trajectory, and to reproduce both its luminous and dark flight phases in detail. We find that the determined strewn field and the generated heat map closely align with the recovery location of the Ischgl meteorite. Furthermore, the measured radionuclide data reported here indicate that the pre-atmospheric size of the Ischgl meteoroid is consistent with the mass estimate inferred from our deceleration analysis along the trajectory. Our findings strongly support the conclusion that the Ischgl meteorite originated from the EN241170 fireball, effectively establishing it as a confirmed meteorite fall. This discovery enables to determine, along with the physical properties, also the heliocentric orbit and cosmic history of the Ischgl meteorite. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2404_11989 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The Fireball of November 24, 1970, as the Most Probable Source of the Ischgl Meteorite Gritsevich, Maria Moilanen, Jarmo Visuri, Jaakko Meier, Matthias M. M. Maden, Colin Oberst, Jürgen Heinlein, Dieter Flohrer, Joachim Castro-Tirado, Alberto J. Delgado-García, Jorge Koeberl, Christian Ferrière, Ludovic Brandstätter, Franz Povinec, Pavel P. Sýkora, Ivan Schweidler, Florian Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics In June 1976, a pristine meteorite stone weighing approximately 1 kg, fully covered with a fresh black fusion crust, was collected on a mountain road in the high-altitude Alpine environment. The recovery took place while clearing the remnants of a snow avalanche, 2 km northwest of Ischgl in Austria. Subsequent to its retrieval, the specimen remained in the finder's private residence without undergoing any scientific examination or identification until 2008, when it was brought to the University of Innsbruck. The sample was classified as a well-preserved LL6 chondrite, with a W0 weathering grade, implying a relatively short time between the meteorite fall and its retrieval. To investigate the potential connection between the Ischgl meteorite and a recorded fireball event, we have reviewed all documented fireballs ever photographed by German fireball camera stations. This examination led us to identify the fireball EN241170 observed in Germany by ten different European Network stations on the night of November 23/24, 1970, as the most likely candidate. We employed state-of-the-art techniques to reconstruct the fireball's trajectory, and to reproduce both its luminous and dark flight phases in detail. We find that the determined strewn field and the generated heat map closely align with the recovery location of the Ischgl meteorite. Furthermore, the measured radionuclide data reported here indicate that the pre-atmospheric size of the Ischgl meteoroid is consistent with the mass estimate inferred from our deceleration analysis along the trajectory. Our findings strongly support the conclusion that the Ischgl meteorite originated from the EN241170 fireball, effectively establishing it as a confirmed meteorite fall. This discovery enables to determine, along with the physical properties, also the heliocentric orbit and cosmic history of the Ischgl meteorite. |
| title | The Fireball of November 24, 1970, as the Most Probable Source of the Ischgl Meteorite |
| topic | Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2404.11989 |