
NSF Org: |
OCE Division Of Ocean Sciences |
Recipient: |
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Initial Amendment Date: | July 22, 2014 |
Latest Amendment Date: | July 22, 2014 |
Award Number: | 1433212 |
Award Instrument: | Standard Grant |
Program Manager: |
Deborah K. Smith
OCE Division Of Ocean Sciences GEO Directorate for Geosciences |
Start Date: | August 1, 2014 |
End Date: | July 31, 2018 (Estimated) |
Total Intended Award Amount: | $92,327.00 |
Total Awarded Amount to Date: | $92,327.00 |
Funds Obligated to Date: |
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History of Investigator: |
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Recipient Sponsored Research Office: |
1000 JEFFERSON DR SW WASHINGTON DC US 20560-0008 (202)633-7110 |
Sponsor Congressional District: |
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Primary Place of Performance: |
1000 Constitution Ave Washington DC US 20560-0001 |
Primary Place of
Performance Congressional District: |
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Unique Entity Identifier (UEI): |
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Parent UEI: |
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NSF Program(s): | Marine Geology and Geophysics |
Primary Program Source: |
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Program Reference Code(s): |
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Program Element Code(s): |
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Award Agency Code: | 4900 |
Fund Agency Code: | 4900 |
Assistance Listing Number(s): | 47.050 |
ABSTRACT
Oxygen is an important element in Earth's mantle and makes up the bulk of most rocks. Its chemical activity (i.e. fugacity) is a controlling factor in determining: (1) the composition of magmas that form from mantle melting, (2) the minerals that are present and in equilibrium with one another in a rock, (3) the distribution of chemical species in associated magmatic fluids, and (4) the partitioning of elements between minerals during their formation and alteration. This research involves a collaboration of three institutions in different parts of the country, employs high temperature/atmospheric-pressure experiments to achieve research goals, and carries out a comparison of the geochemistry of seafloor igneous rocks from the Southwest Indian Ridge. Rock types include mid-ocean ridge basalts, also known as MORB, and abyssal peridotites which represent what is left over in Earth's upper mantle once MORB has been extracted by melting processes. Broader impacts of the work include interaction between scientists from universities and the Smithsonian Museum of Natural History, methods development that advances the infrastructure for science, and a strong integration of research and education. The project will involve the cross-training of a female PhD student who will travel between three laboratories and be trained in state-of-the-art geochemical analytical techniques, providing her with outstanding professional development and networking opportunities. Training of undergraduate students and a postdoc will also take place. The project supports three female researchers, one of whom is early career, and another who is from an institution in an EPSCoR (Experimental Program to Stimulate Competitive Research) state (Rhode Island). The researchers will use the Smithsonian public outreach engine to help implement and promote hands-on learning activities with seafloor rocks where the scientists interact directly with the public. The Smithsonian will also host and disseminate associated online mini-lessons.
This research involves petrologic, petrographic, and experimental work to examine the oxygen fugacity of the upper mantle and its variability. Rock samples come from an area of the seafloor that has an exceptional abundance of both basaltic and peridotitic material in close proximity. Most samples have already been well characterized analytically for major and trace elements and key radiogenic isotopes, allowing the research to focus on oxygen fugacity in a more efficient way. The research includes the cross-calibration of the two most frequently used oxybarometers in upper mantle studies: (1) oxygen fugacity determined from Fe3+/Total Fe ratios of mid-ocean ridge basalts determined by XANES, X-ray Absorption Near Edge Structure, spectroscopy and (2) oxygen fugacity derived from electron microprobe measurements of peridotite using Mossbauer-calibrated spinel standards. Because alteration can significantly impact oxybarometer signatures, its effects will be examined by comparing oxygen fugacity results of fresh and altered peridotites that have undergone various degrees of alteration. Experiments will be performed at 1 atm in a vertical gas mixing furnace at a range of oxygen fugacities that bracket the QFM (Quartz, Forsterite, Magnetite) buffer at a range of temperatures to 1225 C. Project goals include: (1) determining the oxygen fugacity of the upper mantle, (2) examining the processes that control the fugacity of oxygen in MORB and abyssal peridotite, and (3) trying to understand over what length scale oxygen fugacity in the mantle varies.
PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH
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PROJECT OUTCOMES REPORT
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This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.
Did you know that most of Earth?s volcanoes are underwater? It?s true. The global mid-ocean ridge system is a 56,000 kilometer-long chain of sea floor volcanoes. They erupt frequently such that Earth?s ocean floor is constantly being remade ? at about the rate your fingernails grow! We wanted to understand how the chemistry of Earth?s mantle ? the rock layer of Earth that reaches all the way to Earths? core ? affects the chemistry of Earth?s surface. Specifically, we wanted to measure the chemical activity of oxygen in the ocean crust, and what it is in the underlying mantle rocks. We need this information to predict the depth of melting in the Earth, which will help us interpret geophysical data and how our planet recycles its volatile compounds, like carbon dioxide and water.
We used samples from Smithsonian?s National Rock Collection. They were obtained decades ago by a ship dredging the seafloor with a big bucket ? fishing for rocks! Lucky for us, the Smithsonian saved and took care of these precious rocks because it would be REALLY expensive to collect them again. Our rocks are from a part of the ocean called the Southwest Indian Ridge; it is in the Indian Ocean, south and east of Africa. That ridge is special because the ship hauled up both volcanic rocks of Earth?s crust AND the mantle rocks that lie below.
We analyzed the volcanic rocks of the sea floor using X-ray spectroscopy at a synchrotron radiation facility (Argonne National Laboratory?s Advanced Photon Source). The spectra we obtained tell us something about how oxidized or reduced the volcanic glass is. We analyzed the underlying mantle rocks using an electron probe microanalyzer at the Smithsonian Institution. The chemical composition of the rocks tells us something about how oxidized or reduced the rocks are. When we compared the two types of samples (volcanic glass and mantle rocks) we found that they indicate similar chemical activity for oxygen. But we were surprised to learn that the mantle rocks are orders of magnitude more heterogenous. This might mean that the solid interior of the planet is very heterogenous but that when it melts it gets averaged out.
At the same time as the analytical work on ocean rocks, we did laboratory experiments using a gas-mixing furnace. These furnaces get so hot that rocks melt, and they allow us to control the amount of oxygen in the atmosphere. This is a way of simulating what happens when the Earth melts.
Through these experiments we learned about how ferric iron (iron that is oxidized) behaves when the solid mantle melts. We also learned that the computer models we have for this process don?t work very well, and that we will need to do more experiments to understand this.
At the end of our project, all of the scientists involved came to the National Museum of Natural History for an Ocean Rocks! Festival. We held our festival on World Ocean Day and had the opportunity to talk about marine geology to more than 600 members of the public ? mostly children and families.
Last Modified: 03/22/2019
Modified by: Elizabeth Cottrell
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