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The Shape and Internal Structure of the Moon from the Clementine Mission

Zuber, Maria T., Smith, David E., Lemoine, Frank G., Neumann, Gregory A.·1994·Science

Abstract

Global topographic and gravitational field models derived from data collected by the Clementine spacecraft reveal a new picture of the shape and internal structure of the moon. The moon exhibits a 16-kilometer range of elevation, with the greatest topographic excursions occurring on the far side. Lunar highlands are in a state of near-isostatic compensation, whereas impact basins display a wide range of compensation states that do not correlate simply with basin size or age. A global crustal thickness map reveals crustal thinning under all resolvable lunar basins. The results indicate that the structure and thermal history of the moon are more complex than was previously believed.

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Metadata

Authors
Zuber, M. T., Smith, D. E., Lemoine, F. G., & Neumann, G. A.
Venue
Science
Published
1994-12-16
Volume
266
Issue
5192
Pages
1839-1843
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2053257020
Cited by
401
References
0
FWCI
28.51
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: The Shape and Internal Structure of the Moon from the Clementine Mission. https://app.cochat.ai/papers/10.1126/science.266.5192.1839
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Zuber, M. T., Smith, D. E., Lemoine, F. G., & Neumann, G. A. (1994). The Shape and Internal Structure of the Moon from the Clementine Mission. Science. https://doi.org/10.1126/science.266.5192.1839

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.