The fireball of November 24, 1970, as the most probable source of the Ischgl meteorite

被引:2
|
作者
Gritsevich, Maria [1 ,2 ,3 ,4 ]
Moilanen, Jarmo [1 ,3 ]
Visuri, Jaakko [3 ]
Meier, Matthias M. M. [5 ,6 ]
Maden, Colin [5 ]
Oberst, Juergen [7 ]
Heinlein, Dieter [8 ]
Flohrer, Joachim [9 ]
Castro-Tirado, Alberto J. [10 ,11 ]
Delgado-Garcia, Jorge [12 ]
Koeberl, Christian [13 ]
Ferriere, Ludovic [14 ,15 ]
Brandstatter, Franz [14 ]
Povinec, Pavel P. [16 ]
Sykora, Ivan [16 ]
Schweidler, Florian [17 ]
机构
[1] Univ Helsinki, Fac Sci, Gustaf Hallstromin Katu 2, FI-00014 Helsinki, Finland
[2] Swedish Inst Space Phys IRF, Kiruna, Sweden
[3] Finnish Fireball Network, Ursa Astron Assoc, Helsinki, Finland
[4] Ural Fed Univ, Inst Phys & Technol, Ekaterinburg, Russia
[5] Swiss Fed Inst Technol, Inst Geochem & Petrol, Zurich, Switzerland
[6] Naturmuseum St Gallen, St Gallen, Switzerland
[7] Tech Univ Berlin, Inst Geodesy & Geoinformat Sci, Berlin, Germany
[8] German Fireball Network, Augsburg, Germany
[9] Inst Planetary Res, German Aerosp Ctr DLR, Berlin, Germany
[10] Inst Astrofis Andalucia IAA CSIC, Granada, Spain
[11] Univ Malaga, Escuela Ingn Ind, CSIC Dept Ingn Sistemas & Automat, Unidad Asociada, Malaga, Spain
[12] Univ Jaen, Dept Ingn Cartog Geodes & Fotogrametria, Jaen, Spain
[13] Univ Vienna, Dept Lithospher Res, Vienna, Austria
[14] Nat Hist Museum Vienna, Vienna, Austria
[15] Nat Hist Museum Abu Dhabi, Abu Dhabi, U Arab Emirates
[16] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia
[17] Sch Mech Engn, Landshut, Germany
基金
芬兰科学院;
关键词
LUMINOUS EFFICIENCY; EARTHS ATMOSPHERE; NETWORK; ORBIT; RADAR; NEUSCHWANSTEIN; BOLIDES; FALL; MASS; SIMULATION;
D O I
10.1111/maps.14173
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
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.
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收藏
页码:1658 / 1691
页数:34
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