Interior structure of the Moon: Constraints from seismic tomography, gravity and topography
Interior structure of the Moon constrained from seismic tomography, gravity and topography. * A thick (about 225km or more) and heterogeneous lunar lithosphere is suggested. * The observed flattening is likely a "fossil" bulge unrelated to present-day mantle anomalies.
Gespeichert in:
| Autor*in: |
Steinberger, Bernhard [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Rechteinformationen: |
Nutzungsrecht: © COPYRIGHT 2015 Elsevier B.V. |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Physics of the earth and planetary interiors - Amsterdam [u.a.] : Elsevier, 1967, 245(2015), Seite 26-39 |
|---|---|
| Übergeordnetes Werk: |
volume:245 ; year:2015 ; pages:26-39 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.pepi.2015.05.005 |
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Interior structure of the Moon: Constraints from seismic tomography, gravity and topography |
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Interior structure of the Moon constrained from seismic tomography, gravity and topography. * A thick (about 225km or more) and heterogeneous lunar lithosphere is suggested. * The observed flattening is likely a "fossil" bulge unrelated to present-day mantle anomalies. |
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Interior structure of the Moon constrained from seismic tomography, gravity and topography. * A thick (about 225km or more) and heterogeneous lunar lithosphere is suggested. * The observed flattening is likely a "fossil" bulge unrelated to present-day mantle anomalies. |
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Interior structure of the Moon constrained from seismic tomography, gravity and topography. * A thick (about 225km or more) and heterogeneous lunar lithosphere is suggested. * The observed flattening is likely a "fossil" bulge unrelated to present-day mantle anomalies. |
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