The anomalous polymict ordinary chondrite breccia of Elmshorn ( H3 ‐6)—Late reaccretion after collision between two ordinary chondrite parent bodies, complete disruption, and mixing possibly about 2.8 Gyr ago - Université de Bretagne Occidentale Access content directly
Journal Articles Meteoritics and Planetary Science Year : 2024

The anomalous polymict ordinary chondrite breccia of Elmshorn ( H3 ‐6)—Late reaccretion after collision between two ordinary chondrite parent bodies, complete disruption, and mixing possibly about 2.8 Gyr ago

Addi Bischoff
Markus Patzek
Romain Alosius
Jasper Berndt
  • Function : Author
Henner Busemann
Detlev Degering
  • Function : Author
Tommaso Di Rocco
  • Function : Author
Mattias Ek
Jérôme Gattacceca
Jose Godinho
  • Function : Author
Dieter Heinlein
  • Function : Author
Daniela Krietsch
Colin Maden
Oscar Marchhart
  • Function : Author
Martin Martschini
  • Function : Author
Silke Merchel
  • Function : Author
Andreas Pack
  • Function : Author
Stefan Peters
  • Function : Author
Miriam Rüfenacht
Jochen Schlüter
  • Function : Author
Maria Schönbächler
Aleksandra Stojic
  • Function : Author
Jakob Storz
  • Function : Author
Wolfgang Tillmann
  • Function : Author
Alexander Wieser
  • Function : Author
Karl Wimmer
  • Function : Author
Reiner Zielke
  • Function : Author

Abstract

Abstract Elmshorn fell April 25, 2023, about 30 km northwest of the city of Hamburg (Germany). Shortly after the fall, 21 pieces were recovered totaling a mass of 4277 g. Elmshorn is a polymict and anomalous H3‐6 chondritic, fragmental breccia. The rock is a mixture of typical H chondrite lithologies and clasts of intermediate H/L (or L, based on magnetic properties) chondrite origin. In some of the 21 pieces, the H chondrite lithologies dominate, while in others the H/L (or L) chondrite components are prevalent. The H/L chondrite assignment of these components is based on the mean composition of their olivines in equilibrated type 4 fragments (~Fa 21–22 ). The physical properties like density (3.34 g cm −3 ) and magnetic susceptibility (log χ <5.0, with χ in 10 −9 m 3 kg −1 ) are typical for L chondrites, which is inconsistent with the oxygen isotope compositions: all eight O isotope analyses from two different fragments clearly fall into the H chondrite field. Thus, the fragments found in the strewn field vary in mineralogy, mineral chemistry, and physical properties but not in O isotope characteristics. The sample most intensively studied belongs to the stones dominated by H chondrite lithologies. The chemical composition and nucleosynthetic Cr and Ti isotope data are typical for ordinary chondrites. The noble gases in Elmshorn represent a mixture between cosmogenic, radiogenic, and primordially trapped noble gases, while a solar wind component can be excluded. Because the chondritic rock of Elmshorn contains (a) H chondrite parent body interior materials (of types 5 and 6), (b) chondrite parent body near‐surface materials (of types 3 and 4), (c) fragments of an H/L chondrite (dominant in many stones), (d) shock‐darkened fragments, and (e) clasts of various types of impact melts but no solar wind‐implanted noble gases, the different components cannot have been part of a parent body regolith. The most straightforward explanation is that the fragmental breccia of Elmshorn represents a reaccreted rock after a catastrophic collision between an H chondrite parent body and another body with H/L (or L) chondrite characteristics but with deviating O isotope values (i.e. that of H chondrites), complete disruption of the bodies, mixing, and reassembly. This is the only straightforward way that the implantation of solar wind gases could have been avoided in this kind of complex breccia. The gas retention ages of about 2.8 Gyr possibly indicate the closure time after the catastrophic collision between H and H/L (or L) chondrite parent bodies, while the cosmic ray exposure age for Elmshorn, which had a preatmospheric radius of 25–40 cm, is ~17–20 Myr.
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hal-04612235 , version 1 (14-06-2024)

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Addi Bischoff, Markus Patzek, Romain Alosius, Jean-Alix Barrat, Jasper Berndt, et al.. The anomalous polymict ordinary chondrite breccia of Elmshorn ( H3 ‐6)—Late reaccretion after collision between two ordinary chondrite parent bodies, complete disruption, and mixing possibly about 2.8 Gyr ago. Meteoritics and Planetary Science, 2024, ⟨10.1111/maps.14193⟩. ⟨hal-04612235⟩
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