Large-scale impacts are known to have a significant effect on volatile systematics (e.g., hydrogen and chlorine) owing to syn- and post-shock pressures and temperatures allowing for ready volatile loss and isotopic fractionation. We determined the Cl isotopic composition and [Cl] and [H2O] for apatite from 10 samples of the Sudbury impact structure in Canada. The high [Cl] and invariant δ37Cl values in the lower norite are attributed to footwall assimilation in agreement with recent Zn and Pb data. The granophyre, the top of the Sudbury Igneous Complex, displays loss and fractionation of Cl (up to +6.26‰) indicative of degassing under a high gas pressure regime with high [H2O] further buffering isotope fractionation. Similar impacts on dry, airless bodies such as the Moon may have permitted greater amounts of isotopic fractionation, supporting extremely fractionated lunar materials as evidence for the large-scale impact-derived degassing hypothesis. The modest fractionation (up to +8.15‰) and morphologically distinct apatite of the Onaping Formation can be explained by post-impact hydrothermal alteration.
Research Article|
November 13, 2024
Early Publication
A chlorine isotope transect across Sudbury Basin (Canada) impact deposits reveals systematic isotope fractionation
T.J. Barrett;
T.J. Barrett
1
Lunar and Planetary Institute, Universities Space Research Association (USRA), 3600 Bay Area Boulevard, Houston, Texas 77058, USA
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K. Nagashima;
K. Nagashima
2
Hawaiʽi Institute of Geophysics and Planetology, University of Hawaiʽi at Mānoa, 1680 East-West Road, Honolulu, Hawaii 96822, USA
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G.R. Huss;
G.R. Huss
2
Hawaiʽi Institute of Geophysics and Planetology, University of Hawaiʽi at Mānoa, 1680 East-West Road, Honolulu, Hawaii 96822, USA
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J.W. Boyce;
J.W. Boyce
3
NASA Johnson Space Center, Houston, Texas 77058, USA
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K.L. Robinson;
K.L. Robinson
1
Lunar and Planetary Institute, Universities Space Research Association (USRA), 3600 Bay Area Boulevard, Houston, Texas 77058, USA
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D.A. Kring
D.A. Kring
1
Lunar and Planetary Institute, Universities Space Research Association (USRA), 3600 Bay Area Boulevard, Houston, Texas 77058, USA
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T.J. Barrett
1
Lunar and Planetary Institute, Universities Space Research Association (USRA), 3600 Bay Area Boulevard, Houston, Texas 77058, USA
K. Nagashima
2
Hawaiʽi Institute of Geophysics and Planetology, University of Hawaiʽi at Mānoa, 1680 East-West Road, Honolulu, Hawaii 96822, USA
G.R. Huss
2
Hawaiʽi Institute of Geophysics and Planetology, University of Hawaiʽi at Mānoa, 1680 East-West Road, Honolulu, Hawaii 96822, USA
J.W. Boyce
3
NASA Johnson Space Center, Houston, Texas 77058, USA
K.L. Robinson
1
Lunar and Planetary Institute, Universities Space Research Association (USRA), 3600 Bay Area Boulevard, Houston, Texas 77058, USA
D.A. Kring
1
Lunar and Planetary Institute, Universities Space Research Association (USRA), 3600 Bay Area Boulevard, Houston, Texas 77058, USA
Publisher: Geological Society of America
Received:
26 Jul 2024
Accepted:
30 Oct 2024
First Online:
13 Nov 2024
Online ISSN: 1943-2682
Print ISSN: 0091-7613
© 2024 The Authors
Geology (2024)
Article history
Received:
26 Jul 2024
Accepted:
30 Oct 2024
First Online:
13 Nov 2024
Citation
T.J. Barrett, K. Nagashima, G.R. Huss, J.W. Boyce, K.L. Robinson, D.A. Kring; A chlorine isotope transect across Sudbury Basin (Canada) impact deposits reveals systematic isotope fractionation. Geology 2024; doi: https://doi.org/10.1130/G52624.1
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