2022
DOI: 10.1029/2021je007133
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Shock Recovery With Decaying Compressive Pulses: Shock Effects in Calcite (CaCO3) Around the Hugoniot Elastic Limit

Abstract: Shock metamorphism of minerals in meteorites provides insights into the ancient Solar System.Calcite is an abundant aqueous alteration mineral in carbonaceous chondrites. Return samples from the asteroids Ryugu and Bennu are expected to contain calcite-group minerals. Although shock metamorphism in silicates has been well studied, such data for aqueous alteration minerals are limited.Here, we investigated the shock effects in calcite with marble using impact experiments at the Planetary Exploration Research Ce… Show more

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Cited by 9 publications
(23 citation statements)
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“…Impact‐cratering experiments with two‐stage light‐gas guns, on the other hand, are typically afflicted with the excavation of shocked material from the growing transient crater, which makes the reconstruction of the pre‐impact positions and therefore the peak pressures and temperatures experienced in specific parts of the target challenging (e.g., Wünnemann et al., 2016). With some exceptions (e.g., Hamann et al., 2016; Kohout et al., 2020; Kurosawa et al., 2022; Nagaki et al., 2016), direct transitions between shock stages that form as a result of a continuously decaying shock wave have therefore rarely been studied. Excavation of fragmented and brecciated material in cratering experiments also makes it difficult to assess the amount and mode of local shear‐induced melting at bulk peak pressures far below those typically required for incipient melting (e.g., Kenkmann et al., 2000; Langenhorst et al., 2002).…”
Section: Introductionmentioning
confidence: 99%
“…Impact‐cratering experiments with two‐stage light‐gas guns, on the other hand, are typically afflicted with the excavation of shocked material from the growing transient crater, which makes the reconstruction of the pre‐impact positions and therefore the peak pressures and temperatures experienced in specific parts of the target challenging (e.g., Wünnemann et al., 2016). With some exceptions (e.g., Hamann et al., 2016; Kohout et al., 2020; Kurosawa et al., 2022; Nagaki et al., 2016), direct transitions between shock stages that form as a result of a continuously decaying shock wave have therefore rarely been studied. Excavation of fragmented and brecciated material in cratering experiments also makes it difficult to assess the amount and mode of local shear‐induced melting at bulk peak pressures far below those typically required for incipient melting (e.g., Kenkmann et al., 2000; Langenhorst et al., 2002).…”
Section: Introductionmentioning
confidence: 99%
“…The experimental method employed in this study is basically the same as that developed by Kurosawa et al. (2022), except for the samples that were used. The method allows us to collect shocked samples that retain the pre‐impact stratigraphy.…”
Section: Methodsmentioning
confidence: 99%
“…A shock recovery experiment was conducted with a two-stage light gas gun at the Planetary Exploration Research Center of the Chiba Institute of Technology, Japan (Kurosawa et al, 2015). The experimental method employed in this study is basically the same as that developed by Kurosawa et al (2022), except for the samples that were used. The method allows us to collect shocked samples that retain the pre-impact stratigraphy.…”
Section: Impact Experimentsmentioning
confidence: 99%
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