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Szablon:Shrbený (2022)

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'''Abstract:''' We present the description of an observation of a fireball recorded during the sunrise on July&nbsp;15, 2021. Atmospheric trajectory, impact area, and heliocentric orbit were determined on the basis of three instrumental video records. The terminal part of the fireball was not instrumentally recorded due to clouds. Based on our computations, one meteorite was found in the predicted impact area by Polish searchers. The specimen was, soon after recovery, analyzed for the presence of short-lived radionuclides and the measurement confirms a&nbsp;very fresh fall, coinciding with the time of the fireball event. The recovered meteorite, Antonin, is an unbrecciated&nbsp;L5 chondrite with shock stage&nbsp;S3, weathering grade&nbsp;W0, and bulk density of 3.42&nbsp;g cm<sup>−3</sup>. Unusual for&nbsp;L chondrites, it contains assemblages composed of metal and two sulfides, troilite and mackinawite. We interpret these assemblages to have been formed as products of shock metamorphism and post-shock annealing on the parent body. This suggests that the thermal and collisional history of the [[Antonin]] parent body was complex.
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'''Abstract:''' We present the description of an observation of a fireball recorded during the sunrise on July&nbsp;15, 2021. Atmospheric trajectory, impact area, and heliocentric orbit were determined on the basis of three instrumental video records. The terminal part of the fireball was not instrumentally recorded due to clouds. Based on our computations, one meteorite was found in the predicted impact area by Polish searchers. The specimen was, soon after recovery, analyzed for the presence of short-lived radionuclides{{!SLRs|}} and the measurement confirms a&nbsp;very fresh fall, coinciding with the time of the fireball event. The recovered meteorite, Antonin, is an unbrecciated&nbsp;L5 chondrite with shock stage&nbsp;S3, weathering grade&nbsp;W0, and bulk density of 3.42&nbsp;g cm<sup>−3</sup>. Unusual for&nbsp;L chondrites, it contains assemblages composed of metal and two sulfides, troilite and mackinawite. We interpret these assemblages to have been formed as products of shock metamorphism and post-shock annealing on the parent body. This suggests that the thermal and collisional history of the [[Antonin]] parent body was complex.
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<gallery caption="" widths="200px" heights="200px" perrow="3">
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File:Antonin_(Shrbený_2022_fig08).jpg|'''''Fig. 8.''' Recovered 352 g specimen in situ''
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File:Antonin_(MaPS_57-12).jpg|Meteoryt [[Antonin]] trafił na okładkę numeru 57(12) czasopisma [[Meteoritics & Planetary Science/Artykuły|Meteoritics & Planetary Science]]
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</gallery>
{{Przypisy|ncol=1}}
{{Przypisy|ncol=1}}

Aktualna wersja na dzień 21:35, 11 cze 2026

Shrbený Lukáš, Krzesińska Agata M., Borovička Jiří, Spurný Pavel, Tymiński Zbigniew, Kmieciak Kryspin, (2022), Analysis of the daylight fireball of July 15, 2021, leading to a meteorite fall and find near Antonin, Poland, and a description of the recovered chondrite, Meteoritics & Planetary Science, vol. 57(12), 2022, s. 2108-2126 (abstrakt). Plik doi.



Abstract: We present the description of an observation of a fireball recorded during the sunrise on July 15, 2021. Atmospheric trajectory, impact area, and heliocentric orbit were determined on the basis of three instrumental video records. The terminal part of the fireball was not instrumentally recorded due to clouds. Based on our computations, one meteorite was found in the predicted impact area by Polish searchers. The specimen was, soon after recovery, analyzed for the presence of short-lived radionuclides[1] and the measurement confirms a very fresh fall, coinciding with the time of the fireball event. The recovered meteorite, Antonin, is an unbrecciated L5 chondrite with shock stage S3, weathering grade W0, and bulk density of 3.42 g cm−3. Unusual for L chondrites, it contains assemblages composed of metal and two sulfides, troilite and mackinawite. We interpret these assemblages to have been formed as products of shock metamorphism and post-shock annealing on the parent body. This suggests that the thermal and collisional history of the Antonin parent body was complex.


Przypisy

  1. ^ krótkożyciowe izotopy promieniotwórcze (SLRs, ang. Short-lived radionuclides) – radionuklidy o okresach półtrwania krótkich w porównaniu z wiekiem Układu Słonecznego (~4,567 mld lat), które były obecne podczas jego formowania, ale dziś już niemal całkowicie zanikły. Ich dawną obecność poznajemy po produktach rozpadu zachowanych w meteorytach. Najważniejsze SLRs w kosmochemii (w nawiasie okresy połowicznego rozpadu): 26Al (0,717 mln lat), 41Ca (0,10 mln lat), 36Cl (0,30 mln lat), 60Fe (2,6 mln lat), 63Mn (3,7 mln lat). Rozpad 26Al→26Mg był prawdopodobnie głównym źródłem ogrzewania młodych planetozymali prowadzącym do: metamorfizm chondrytów, topienie skał krzemianowych, oddzielenie jąder metalicznych, powstania meteorytów zdyferencjonowanych. Mierząc stężenie ekstremalnie krótkożyciowych izotopów promieniotwórczych (ang. short-lived radioactive nuklides) w meteorycie można określić tzw. wiek ziemski okazu (ang. terrestrial age; patrz → cosmogenic isotopes), tzn. czas od spadku meteorytu na Ziemię do chwili obecnej, gdy już ustały w nim procesy wytwarzania nowych nuklidów powstających w wyniku bombardowania meteoroidu promieniowaniem kosmicznym w przestrzeni pozaziemskiej. Przykładowe ekstremalnie krótkożyciowe izotopy promieniotwórcze występujące w chondrytach zwyczajnych to: 52Mn (5,6 dni), 48V (15,97 dni), 51Cr (27,7 dni), 59Fe (44,5 dni), 58Co (70,4 dni), 56Co (77,23 dni), 46Sc (83,8 dni), 57Co (271,8 dni), 54Mn (312 dni) (patrz → Antonin  ●  Sołtmany/Badania, Laubenstein et al. 2012). Wikipedia (EN) – Cosmogenic nuclide
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