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

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Maria Gritsevich, Jarmo Moilanen, Jaakko Visuri, Matthias M. M. Meier, Colin Maden, Jürgen Oberst, Dieter Heinlein, Joachim Flohrer, Alberto J. Castro-Tirado, Jorge Delgado-García, Christian Koeberl, Ludovic Ferrière, Franz Brandstätter, Pavel P. Povinec, Ivan Sýkora, Florian Schweidler
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引用次数: 0

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.

Abstract Image

1970 年 11 月 24 日的火球是伊施格尔陨石最可能的来源
伊施格尔陨石的发现以一种引人入胜的方式展开。1976 年 6 月,人们在高海拔阿尔卑斯山环境中的一条山路上采集到一块重约 1 千克的原始陨石,上面覆盖着一层新鲜的黑色熔壳。这块陨石是在奥地利伊施格尔镇西北 2 公里处清理雪崩残留物时捡到的。找到样本后,它一直被藏在发现者的私人住宅中,没有经过任何科学检查或鉴定,直到 2008 年才被送到因斯布鲁克大学。经过评估,该样本被归类为保存完好的 LL6 型软玉,风化等级为 W0,这意味着从陨石坠落到取回之间的时间相对较短。为了研究伊施格尔陨石与有记录的火球事件之间的潜在联系,我们查阅了德国火球摄影站拍摄到的所有有记录的火球。通过这次审查,我们确定了 1970 年 11 月 23/24 日晚由 10 个不同的欧洲网络站在德国观测到的 EN241170 火球为最有可能的候选火球。我们采用最先进的技术重建了火球的轨迹,并详细再现了火球的明暗飞行阶段。我们发现,确定的散射场和生成的热图与伊施格尔陨石的复原位置非常吻合。此外,本文所报告的放射性核素测量数据表明,伊施格尔陨石在进入大气层前的大小与我们沿轨迹进行减速分析所推断的质量估计值一致。我们的发现有力地支持了伊施格尔陨石源自 EN241170 火球的结论,有效地将其确定为已确认的陨石坠落。这一发现使我们能够确定伊施格尔陨石的物理特性以及日心轨道和宇宙历史。
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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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