The Constitution and Structure of the Lunar Interior

@article{Wieczorek2006TheCA,
  title={The Constitution and Structure of the Lunar Interior},
  author={Mark A. Wieczorek and Bradley L. Jolliff and Amir Khan and Matthew E. Pritchard and Benjamin P. Weiss and James G. Williams and Lon L. Hood and Kevin Righter and Clive R. Neal and Charles Shearer and I. S. Mccallum and Stephanie Tompkins and Bernard Ray Hawke and Christopher Peterson and Jeffrey J. Gillis and B. J. Bussey},
  journal={Reviews in Mineralogy \& Geochemistry},
  year={2006},
  volume={60},
  pages={221-364}
}
The current state of understanding of the lunar interior is the sum of nearly four decades of work and a range of exploration programs spanning that same time period. Missions of the 1960s including the Rangers, Surveyors, and Lunar Orbiters, as well as Earth-based telescopic studies, laid the groundwork for the Apollo program and provided a basic understanding of the surface, its stratigraphy, and chronology. Through a combination of remote sensing, surface exploration, and sample return, the… 
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References

SHOWING 1-10 OF 713 REFERENCES
The Stratigraphy and Evolution of the Lunar Crust
Reconstruction of stratigraphic relationships in the ancient lunar crust has proved to be a formidable task. The intense bombardment during the first 700 m.y. of lunar history has severely perturbed
Crustal diversity of the moon: Compositional analyses of Galileo solid state imaging data
The multispectral images of the lunar limb and farside obtained by the solid state imaging (SSI) system on board the Galileo spacecraft provide the first new pulse of compositional data of the Moon
The Composition of the Prebasin Crust in the Central Highlands of the Moon
RANDY L.KOROTEVDepartment of Earth and Planetary Sciences and McDonnell Center for the Space Sciences,Washington University, St. Louis, Missouri 63130, USAAuthor's e-mail address:
Geophysical and geochemical evolution of the lunar magma ocean
There is increasing evidence that at least the outer few hundred kilometers of the moon were melted immediately following accretion. This paper studies the evolution of this lunar magma ocean. The
THE ISOTOPIC RECORD OF LUNAR VOLCANISM
A New View Of The Moon In Light Of Data From Clementine And Prospector Missions
Results from the 1994 Clementine and 1998–99 Lunar Prospector orbital missions are forcing a reevaluation of existing models of the origin and evolution of the Moon. Data on global topography and
A model of early lunar differentiation
The presence of anorthosites and the scarcity of complementary mafic rocks in the lunar crust suggest a body of melt with depth of the order of the depth of the crust itself (about 60 km). This depth
Structure, composition, and properties of lunar crust.
Lunar seismic data from three Apollo seismometers are interpreted to determine the structure of the moon's interior to a depth of about 100 km. The travel times and amplitudes of P and S arrivals
Composition of the lunar highland crust from near‐infrared spectroscopy
Near-infrared reflectance spectra of the lunar highlands are synthesized to obtain global information about the composition of the lunar near-side crust. Immature exposed surfaces from small fresh
An inquiry into the lunar interior: A nonlinear inversion of the Apollo lunar seismic data
[1] This study discusses in detail the inversion of the Apollo lunar seismic data and the question of how to analyze the results. The well-known problem of estimating structural parameters (seismic
...
...