Density deficit of Earth’s core revealed by a multimegabar primary pressure scale
An accurate pressure scale is a fundamental requirement to understand planetary interiors. Here, we establish a primary pressure scale extending to the multimegabar pressures of Earth’s core, by combined measurement of the acoustic velocities and the density from a rhenium sample in a diamond anvil...
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Published in: | Science advances Vol. 9; no. 36; p. eadh8706 |
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Main Authors: | , , , , , , |
Format: | Journal Article |
Language: | English |
Published: |
American Association for the Advancement of Science
08-09-2023
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Subjects: | |
Online Access: | Get full text |
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Summary: | An accurate pressure scale is a fundamental requirement to understand planetary interiors. Here, we establish a primary pressure scale extending to the multimegabar pressures of Earth’s core, by combined measurement of the acoustic velocities and the density from a rhenium sample in a diamond anvil cell using inelastic x-ray scattering and x-ray diffraction. Our scale agrees well with previous primary scales and shock Hugoniots in each experimental pressure range and reveals that previous scales have overestimated laboratory pressures by at least 20% at 230 gigapascals. It suggests that the light element content in Earth’s inner core (the density deficit relative to iron) is likely to be double what was previously estimated, or Earth’s inner core temperature is much higher than expected, or some combination thereof.
A primary pressure scale to multimegabar pressure may double the light element content of Earth’s inner core. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 Present address: Institute for Planetary Materials, Okayama University, Misasa, Tottori 682-0193, Japan. |
ISSN: | 2375-2548 2375-2548 |
DOI: | 10.1126/sciadv.adh8706 |