Award Abstract # 2317025
Collaborative Research: GLOW: Iron Redox Reactions in Magma Oceans and Differentiation of Rocky Planets

NSF Org: EAR
Division Of Earth Sciences
Recipient: TRUSTEES OF INDIANA UNIVERSITY
Initial Amendment Date: July 19, 2023
Latest Amendment Date: July 19, 2023
Award Number: 2317025
Award Instrument: Standard Grant
Program Manager: Jennifer Wade
jwade@nsf.gov
 (703)292-4739
EAR
 Division Of Earth Sciences
GEO
 Directorate for Geosciences
Start Date: August 15, 2023
End Date: July 31, 2026 (Estimated)
Total Intended Award Amount: $35,468.00
Total Awarded Amount to Date: $35,468.00
Funds Obligated to Date: FY 2023 = $35,468.00
History of Investigator:
  • Catherine Macris (Principal Investigator)
    camacris@iu.edu
Recipient Sponsored Research Office: Indiana University
107 S INDIANA AVE
BLOOMINGTON
IN  US  47405-7000
(317)278-3473
Sponsor Congressional District: 09
Primary Place of Performance: Indiana University Purdue University Indianapolis
723 W. Michigan St., SL 118D
Indianapolis
IN  US  46202-5191
Primary Place of Performance
Congressional District:
07
Unique Entity Identifier (UEI): YH86RTW2YVJ4
Parent UEI:
NSF Program(s): Petrology and Geochemistry
Primary Program Source: 01002324DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s):
Program Element Code(s): 157300
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.050

ABSTRACT

Earth?s mantle is far more oxidized than its building blocks. The oxidation of the mantle has a large effect on our planet?s habitability. Because of the oxidation, our atmosphere contains enough oxygen to support life. One theory suggests that mantle oxidation occurred during the ?magma ocean? stage of Earth?s history. When early Earth was still molten and forming, it was covered by a hot and deep ocean of magma. Studying the oxidation process is important for understanding the role of the magma ocean in making Earth habitable. Scientists also want to know how this process applies to other planets and exoplanets. This research project will bring together geoscientists and astronomers to study how planets become habitable through mantle oxidation. The project will also create educational materials and answer questions about the relationship between geology and life.

This Geoscience Lessons for and from Other Worlds (GLOW) award will enable researchers to conduct experiments at pressures, temperatures, and compositions directly relevant to silicate-metal reactions in magma oceans of Earth and Earth-like planets. The experiments will use peridotite glass starting materials synthesized in a levitation furnace. The samples will be subjected to pressures and temperatures up to 140 GPa and 6000 K in laser-heated diamond anvil cells. The products will be analyzed for their ferric and ferrous iron ratio using synchrotron Mössbauer spectroscopy. The experimental results will be incorporated into a thermodynamic model that will allow prediction of the oxidation of a planetary mantle and its habitability, depending on the size of the planet and the conditions of formation of its core.

This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

Please report errors in award information by writing to: awardsearch@nsf.gov.

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