Thermal history modelling of the L chondrite parent body

@article{Gail2019ThermalHM,
  title={Thermal history modelling of the L chondrite parent body},
  author={Hans-Peter Gail and Mario Trieloff},
  journal={Astronomy \& Astrophysics},
  year={2019}
}
Context.The cooling history of individual meteorites can be reconstructed if closure temperatures and closure ages of different radioisotopic chronometers are available for a couple of meteorites. If a close similarity in chemical and isotopic composition suggests a common origin from the same parent body, some basic properties of this body can be derived.Aims.The radius of the L chondrite parent body, its formation time, and its evolution history are determined by fitting theoretical models to… 

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Petrology and geochemistry of Patuxent Range 91501, a clast‐poor impact melt from the L‐chondrite parent body and Lewis Cliff 88663, an L7 chondrite

Abstract— We have performed petrologic and geochemical studies of Patuxent Range (PAT) 91501 and Lewis Cliff (LEW) 88663. PAT 91501, originally classified as an L7 chondrite, is rather a unique, near
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