Replication Data for: Hydrogen isotopic composition of CI- and CM-like clasts from meteorite breccias – Sampling unknown sources of carbonaceous chondrite materials ...

Volatile-rich, CI- and CM-like clasts occur in different brecciated achondrite and chondrite groups. The CI-like clasts in HEDs, polymict ureilites, as well as ordinary, CR, and CB chondrites have a similar mineralogy, indicating a similar alteration history. However, when viewed in detail, their mi...

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Bibliographic Details
Main Author: Universitätsbibliothek Der FU Berlin
Format: Dataset
Language:unknown
Published: Freie Universität Berlin 2023
Subjects:
Online Access:https://dx.doi.org/10.17169/refubium-39169
https://refubium.fu-berlin.de/handle/fub188/39452
id ftdatacite:10.17169/refubium-39169
record_format openpolar
spelling ftdatacite:10.17169/refubium-39169 2023-06-11T04:17:13+02:00 Replication Data for: Hydrogen isotopic composition of CI- and CM-like clasts from meteorite breccias – Sampling unknown sources of carbonaceous chondrite materials ... Universitätsbibliothek Der FU Berlin 2023 https://dx.doi.org/10.17169/refubium-39169 https://refubium.fu-berlin.de/handle/fub188/39452 unknown Freie Universität Berlin Chemistry Earth and Environmental Sciences Carbonaceous chondrite Deuterium Secondary ion mass spectrometry Dataset dataset 2023 ftdatacite https://doi.org/10.17169/refubium-39169 2023-06-01T12:00:47Z Volatile-rich, CI- and CM-like clasts occur in different brecciated achondrite and chondrite groups. The CI-like clasts in HEDs, polymict ureilites, as well as ordinary, CR, and CB chondrites have a similar mineralogy, indicating a similar alteration history. However, when viewed in detail, their mineral chemistry shows some minor differences between the clasts from different meteorite groups. For CM-like clasts found in HED meteorites, the clasts are, based on their mineralogy, clearly fragments of CM chondrites. To be able to decipher whether CI- (or CM-)like clasts from different meteorite groups are related to certain meteorite classes known to contain volatiles, we obtained D/H ratios of several clasts from the meteorite groups mentioned above and compared them with those of CI and CM chondrites as well as to unique carbonaceous chondrites such as Bells, Essebi, and Tagish Lake. Considering the δD-values, CM-like clasts in HEDs span a similar range compared to bulk values of CM chondrites, further ... Dataset Tagish DataCite Metadata Store (German National Library of Science and Technology) Tagish ENVELOPE(-134.272,-134.272,60.313,60.313) Tagish Lake ENVELOPE(-134.233,-134.233,59.717,59.717)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Chemistry
Earth and Environmental Sciences
Carbonaceous chondrite
Deuterium
Secondary ion mass spectrometry
spellingShingle Chemistry
Earth and Environmental Sciences
Carbonaceous chondrite
Deuterium
Secondary ion mass spectrometry
Universitätsbibliothek Der FU Berlin
Replication Data for: Hydrogen isotopic composition of CI- and CM-like clasts from meteorite breccias – Sampling unknown sources of carbonaceous chondrite materials ...
topic_facet Chemistry
Earth and Environmental Sciences
Carbonaceous chondrite
Deuterium
Secondary ion mass spectrometry
description Volatile-rich, CI- and CM-like clasts occur in different brecciated achondrite and chondrite groups. The CI-like clasts in HEDs, polymict ureilites, as well as ordinary, CR, and CB chondrites have a similar mineralogy, indicating a similar alteration history. However, when viewed in detail, their mineral chemistry shows some minor differences between the clasts from different meteorite groups. For CM-like clasts found in HED meteorites, the clasts are, based on their mineralogy, clearly fragments of CM chondrites. To be able to decipher whether CI- (or CM-)like clasts from different meteorite groups are related to certain meteorite classes known to contain volatiles, we obtained D/H ratios of several clasts from the meteorite groups mentioned above and compared them with those of CI and CM chondrites as well as to unique carbonaceous chondrites such as Bells, Essebi, and Tagish Lake. Considering the δD-values, CM-like clasts in HEDs span a similar range compared to bulk values of CM chondrites, further ...
format Dataset
author Universitätsbibliothek Der FU Berlin
author_facet Universitätsbibliothek Der FU Berlin
author_sort Universitätsbibliothek Der FU Berlin
title Replication Data for: Hydrogen isotopic composition of CI- and CM-like clasts from meteorite breccias – Sampling unknown sources of carbonaceous chondrite materials ...
title_short Replication Data for: Hydrogen isotopic composition of CI- and CM-like clasts from meteorite breccias – Sampling unknown sources of carbonaceous chondrite materials ...
title_full Replication Data for: Hydrogen isotopic composition of CI- and CM-like clasts from meteorite breccias – Sampling unknown sources of carbonaceous chondrite materials ...
title_fullStr Replication Data for: Hydrogen isotopic composition of CI- and CM-like clasts from meteorite breccias – Sampling unknown sources of carbonaceous chondrite materials ...
title_full_unstemmed Replication Data for: Hydrogen isotopic composition of CI- and CM-like clasts from meteorite breccias – Sampling unknown sources of carbonaceous chondrite materials ...
title_sort replication data for: hydrogen isotopic composition of ci- and cm-like clasts from meteorite breccias – sampling unknown sources of carbonaceous chondrite materials ...
publisher Freie Universität Berlin
publishDate 2023
url https://dx.doi.org/10.17169/refubium-39169
https://refubium.fu-berlin.de/handle/fub188/39452
long_lat ENVELOPE(-134.272,-134.272,60.313,60.313)
ENVELOPE(-134.233,-134.233,59.717,59.717)
geographic Tagish
Tagish Lake
geographic_facet Tagish
Tagish Lake
genre Tagish
genre_facet Tagish
op_doi https://doi.org/10.17169/refubium-39169
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