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dc.contributor.author
Gritsevich, Maria
dc.contributor.author
Moilanen, Jarmo
dc.contributor.author
Visuri, Jaakko
dc.contributor.author
Meier, Matthias M.M.
dc.contributor.author
Maden, Colin
dc.contributor.author
Oberst, Jürgen
dc.contributor.author
Heinlein, Dieter
dc.contributor.author
Flohrer, Joachim
dc.contributor.author
Castro-Tirado, Alberto J.
dc.contributor.author
Delgado-García, Jorge
dc.contributor.author
Koeberl, Christian
dc.contributor.author
Ferrière, Ludovic
dc.contributor.author
Brandstätter, Franz
dc.contributor.author
Povinec, Pavel P.
dc.contributor.author
Schweidler, Florian
dc.date.accessioned
2024-06-04T08:13:56Z
dc.date.available
2024-06-04T06:16:54Z
dc.date.available
2024-06-04T08:13:56Z
dc.date.issued
2024
dc.identifier.issn
1086-9379
dc.identifier.issn
0026-1114
dc.identifier.issn
1945-5100
dc.identifier.other
10.1111/maps.14173
en_US
dc.identifier.uri
http://hdl.handle.net/20.500.11850/676401
dc.identifier.doi
10.3929/ethz-b-000676401
dc.description.abstract
The discovery of the Ischgl meteorite unfolded in a captivating manner. 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 the town of Ischgl in Austria. Subsequent to its retrieval, the specimen remained tucked away in the finder's private residence without undergoing any scientific examination or identification until 2008, when it was brought to the University of Innsbruck. Upon evaluation, 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 10 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.
en_US
dc.format
application/pdf
en_US
dc.language.iso
en
en_US
dc.publisher
Wiley-Blackwell
en_US
dc.rights.uri
http://creativecommons.org/licenses/by/4.0/
dc.title
The fireball of November 24, 1970, as the most probable source of the Ischgl meteorite
en_US
dc.type
Journal Article
dc.rights.license
Creative Commons Attribution 4.0 International
dc.date.published
2024-05-25
ethz.journal.title
Meteoritics & Planetary Science
ethz.journal.abbreviated
Meteorit Planet Sci.
ethz.version.deposit
publishedVersion
en_US
ethz.identifier.wos
ethz.publication.status
published
en_US
ethz.date.deposited
2024-06-04T06:17:20Z
ethz.source
WOS
ethz.eth
yes
en_US
ethz.availability
Open access
en_US
ethz.rosetta.exportRequired
true
ethz.COinS
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