A Portrait of Terrestrial Volatile Evolution From Mantle Noble Gases

Volatile elements and compounds provide important insights into large-scale planetary and tectonic processes. The chapters in this thesis exploit the wealth of information provided by noble gas measurements to address a variety of questions regarding the origins and distributions of volatiles in the...

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Main Author: Tucker, Jonathan M.
Other Authors: Mukhopadhyay, Sujoy, Langmuir, Charles, Jacobsen, Stein, Johnston, David
Format: Thesis
Language:English
Published: 2017
Subjects:
Online Access:http://nrs.harvard.edu/urn-3:HUL.InstRepos:37944946
id ftharvardudash:oai:dash.harvard.edu:1/37944946
record_format openpolar
institution Open Polar
collection Harvard University: DASH - Digital Access to Scholarship at Harvard
op_collection_id ftharvardudash
language English
topic Geochemistry
Geology
spellingShingle Geochemistry
Geology
Tucker, Jonathan M.
A Portrait of Terrestrial Volatile Evolution From Mantle Noble Gases
topic_facet Geochemistry
Geology
description Volatile elements and compounds provide important insights into large-scale planetary and tectonic processes. The chapters in this thesis exploit the wealth of information provided by noble gas measurements to address a variety of questions regarding the origins and distributions of volatiles in the Earth. Chapter 1 presents new He-Ne-Ar-Xe data from basalts from the equatorial Mid-Atlantic Ridge, demonstrating a large degree of heavy noble gas heterogeneity in mid-ocean ridge basalts (MORBs). The He and Ne data can be explained primarily by a mixture of a depleted mantle component and a HIMU-like component, with the constraint that the HIMU component is a combination of recycled and primitive material. While most mantle-derived Xe is recycled atmospheric Xe, the compositions of depleted MORBs, HIMU-type MORBs, and the Iceland plume cannot be related solely by different amounts of recycled air. Rather, HIMU-type MORBs and the Iceland plume sample a less degassed reservoir. Furthermore, differences in the amount of 129I-derived 129Xe between the depleted and HIMU-type MORBs suggests that HIMU-type MORBs are sampling a reservoir that formed within the first 100 Myr of solar system history and has not extensively mixed with the depleted mantle since. Chapter 2 explores the hypothesis that high 3He/22Ne ratios intrinsic to the depleted mantle were generated by multiple episodes of magma ocean outgassing and atmospheric loss during Earth's accretion. We argue that magma ocean outgassing in the aftermath of giant impacts during accretion can raise the mantle 3He/22Ne ratio, but multiple episodes of outgassing and atmospheric loss are required to achieve the ratio observed in the depleted mantle. The preservation of low 3He/22Ne ratios in primitive plumes suggests that later giant impacts such as the Moon-forming giant impact did not homogenize the whole mantle. The requirement for episodes of atmospheric loss to achieve high 3He/22Ne ratios during accretion may also provide an explanation for Earth's nonchondritic volatile element ratios such as N/H as N would be more susceptible to loss processes than H. Chapter 3 uses the combined constraints of the radiogenic noble gases 4He*, 21Ne*, 40Ar*, and 136Xe*U to examine degassing processes at mid-ocean ridges. We show that ratios of radiogenic noble gases cannot be simultaneously explained by any equilibrium degassing model, questioning the use of such models to reconstruct pre-degassing magmatic contents and hence mantle fluxes of elements like C. We argue that kinetic fractionation prevents slowly diffusing volatiles from achieving their equilibrium partitioning between vesicles and melt and present a new simple model of disequilibrium degassing that self-consistently explains CO2-4He*-21Ne*-40Ar* compositions in MORBs. Application of this model suggests that the average MORB mantle C/3He ratio and C flux may be a factor of 2 higher than that inferred from equilibrium degassing-based estimates. Chapter 4 presents new He data on depleted MORBs from the subtropical north Mid-Atlantic Ridge. Correlations between He and Pb isotopic compositions in this region as well as others globally suggest that, absent plume influence, He isotopes in MORBs can be explained by a mixture of an intrinsic, relatively unradiogenic depleted component and highly radiogenic recycled oceanic crust, a manifestation of the "marble cake" mantle. With a simple mixing model, we estimate that the mantle source of average MORBs has ~5% recycled oceanic crust. Chapter 5 presents new He-Ne-Ar-Xe data on a subset of the depleted MORB samples described in Chapter 4. Ne isotopic compositions are less nucleogenic than average MORBs, indicating the influence of a relatively undegassed component, which may be especially strongly sampled near 29°N. Ar, and Xe isotopic compositions extend from moderately radiogenic values to highly unradiogenic values, demonstrating extreme variability absent significant variability in lithophile chemistry. Globally, Ar and Xe isotopic compositions correlate in oceanic basalts, interpreted to result from mixtures of degassed material having radiogenic Ar and Xe with undegassed material and recycled air having unradiogenic Ar and Xe. Earth and Planetary Sciences noble gas; geochemistry; mantle; volatiles; accretion
author2 Mukhopadhyay, Sujoy
Langmuir, Charles
Jacobsen, Stein
Johnston, David
format Thesis
author Tucker, Jonathan M.
author_facet Tucker, Jonathan M.
author_sort Tucker, Jonathan M.
title A Portrait of Terrestrial Volatile Evolution From Mantle Noble Gases
title_short A Portrait of Terrestrial Volatile Evolution From Mantle Noble Gases
title_full A Portrait of Terrestrial Volatile Evolution From Mantle Noble Gases
title_fullStr A Portrait of Terrestrial Volatile Evolution From Mantle Noble Gases
title_full_unstemmed A Portrait of Terrestrial Volatile Evolution From Mantle Noble Gases
title_sort portrait of terrestrial volatile evolution from mantle noble gases
publishDate 2017
url http://nrs.harvard.edu/urn-3:HUL.InstRepos:37944946
geographic Mid-Atlantic Ridge
geographic_facet Mid-Atlantic Ridge
genre Iceland
genre_facet Iceland
op_relation http://nrs.harvard.edu/urn-3:HUL.InstRepos:37944946
orcid:0000-0002-3870-5079
_version_ 1766043005626613760
spelling ftharvardudash:oai:dash.harvard.edu:1/37944946 2023-05-15T16:52:38+02:00 A Portrait of Terrestrial Volatile Evolution From Mantle Noble Gases Tucker, Jonathan M. Mukhopadhyay, Sujoy Langmuir, Charles Jacobsen, Stein Johnston, David 2017-03 application/pdf http://nrs.harvard.edu/urn-3:HUL.InstRepos:37944946 en eng http://nrs.harvard.edu/urn-3:HUL.InstRepos:37944946 orcid:0000-0002-3870-5079 Geochemistry Geology Thesis or Dissertation text 2017 ftharvardudash 2022-04-05T18:53:07Z Volatile elements and compounds provide important insights into large-scale planetary and tectonic processes. The chapters in this thesis exploit the wealth of information provided by noble gas measurements to address a variety of questions regarding the origins and distributions of volatiles in the Earth. Chapter 1 presents new He-Ne-Ar-Xe data from basalts from the equatorial Mid-Atlantic Ridge, demonstrating a large degree of heavy noble gas heterogeneity in mid-ocean ridge basalts (MORBs). The He and Ne data can be explained primarily by a mixture of a depleted mantle component and a HIMU-like component, with the constraint that the HIMU component is a combination of recycled and primitive material. While most mantle-derived Xe is recycled atmospheric Xe, the compositions of depleted MORBs, HIMU-type MORBs, and the Iceland plume cannot be related solely by different amounts of recycled air. Rather, HIMU-type MORBs and the Iceland plume sample a less degassed reservoir. Furthermore, differences in the amount of 129I-derived 129Xe between the depleted and HIMU-type MORBs suggests that HIMU-type MORBs are sampling a reservoir that formed within the first 100 Myr of solar system history and has not extensively mixed with the depleted mantle since. Chapter 2 explores the hypothesis that high 3He/22Ne ratios intrinsic to the depleted mantle were generated by multiple episodes of magma ocean outgassing and atmospheric loss during Earth's accretion. We argue that magma ocean outgassing in the aftermath of giant impacts during accretion can raise the mantle 3He/22Ne ratio, but multiple episodes of outgassing and atmospheric loss are required to achieve the ratio observed in the depleted mantle. The preservation of low 3He/22Ne ratios in primitive plumes suggests that later giant impacts such as the Moon-forming giant impact did not homogenize the whole mantle. The requirement for episodes of atmospheric loss to achieve high 3He/22Ne ratios during accretion may also provide an explanation for Earth's nonchondritic volatile element ratios such as N/H as N would be more susceptible to loss processes than H. Chapter 3 uses the combined constraints of the radiogenic noble gases 4He*, 21Ne*, 40Ar*, and 136Xe*U to examine degassing processes at mid-ocean ridges. We show that ratios of radiogenic noble gases cannot be simultaneously explained by any equilibrium degassing model, questioning the use of such models to reconstruct pre-degassing magmatic contents and hence mantle fluxes of elements like C. We argue that kinetic fractionation prevents slowly diffusing volatiles from achieving their equilibrium partitioning between vesicles and melt and present a new simple model of disequilibrium degassing that self-consistently explains CO2-4He*-21Ne*-40Ar* compositions in MORBs. Application of this model suggests that the average MORB mantle C/3He ratio and C flux may be a factor of 2 higher than that inferred from equilibrium degassing-based estimates. Chapter 4 presents new He data on depleted MORBs from the subtropical north Mid-Atlantic Ridge. Correlations between He and Pb isotopic compositions in this region as well as others globally suggest that, absent plume influence, He isotopes in MORBs can be explained by a mixture of an intrinsic, relatively unradiogenic depleted component and highly radiogenic recycled oceanic crust, a manifestation of the "marble cake" mantle. With a simple mixing model, we estimate that the mantle source of average MORBs has ~5% recycled oceanic crust. Chapter 5 presents new He-Ne-Ar-Xe data on a subset of the depleted MORB samples described in Chapter 4. Ne isotopic compositions are less nucleogenic than average MORBs, indicating the influence of a relatively undegassed component, which may be especially strongly sampled near 29°N. Ar, and Xe isotopic compositions extend from moderately radiogenic values to highly unradiogenic values, demonstrating extreme variability absent significant variability in lithophile chemistry. Globally, Ar and Xe isotopic compositions correlate in oceanic basalts, interpreted to result from mixtures of degassed material having radiogenic Ar and Xe with undegassed material and recycled air having unradiogenic Ar and Xe. Earth and Planetary Sciences noble gas; geochemistry; mantle; volatiles; accretion Thesis Iceland Harvard University: DASH - Digital Access to Scholarship at Harvard Mid-Atlantic Ridge