scispace - formally typeset
Journal ArticleDOI

The Constitution and Structure of the Lunar Interior

TLDR
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 as discussed by the authors, which is the framework that unifies our knowledge of the structure and composition of the Moon.
Abstract
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 Apollo missions provided a general picture of the lunar interior and spawned the concept of the lunar magma ocean. In particular, the discovery of anorthite clasts in the returned samples led to the view that a large portion of the Moon was initially molten, and that crystallization of this magma ocean gave rise to mafic cumulates that make up the mantle, and plagioclase flotation cumulates that make up the crust (Smith et al. 1970; Wood et al. 1970). This model is now generally accepted and is the framework that unifies our knowledge of the structure and composition of the Moon. The intention of this chapter is to review the major advances that have been made over the past decade regarding the constitution of the Moon’s interior. Much of this new knowledge is a direct result of data acquired from the successful Clementine and Lunar Prospector missions, as well as the analysis of new lunar meteorites. As will be seen, results from these studies have led to many fundamental amendments to the magma ocean model. Much of what we know from sample analyses has been previously summarized elsewhere, and only their most important aspects will be discussed in this chapter. The reader is referred to the relevant chapters in the books Basaltic Volcanism on the Terrestrial Planets (Basaltic Volcanism Study Project 1981), The …

read more

Citations
More filters
Journal ArticleDOI

Making the Moon from a fast-spinning Earth: a giant impact followed by resonant despinning.

TL;DR: Computer simulations show that a giant impact on early Earth could lead to a Moon with a composition similar to Earth’s, and shows that a faster-spinning early Earth-Moon system can lose angular momentum and reach the present state through an orbital resonance between the Sun and Moon.
Journal ArticleDOI

Volatile content of lunar volcanic glasses and the presence of water in the Moon’s interior

TL;DR: The results indicate that, contrary to prevailing ideas, the bulk Moon might not be entirely depleted in highly volatile elements, including water, and the presence of water must be considered in models constraining the Moon’s formation and its thermal and chemical evolution.
Journal ArticleDOI

Seismic detection of the lunar core

TL;DR: Reinterpreted Apollo-era seismic data from the Moon reveal a solid inner core and a fluid outer core, overlain by a partially molten boundary layer, consistent with a volatile-depleted interior.
Book ChapterDOI

Gravity and Topography of the Terrestrial Planets

TL;DR: A general review of the mathematical formalism that is used in describing gravity and topography of the terrestrial planets is given in this article, where the basic properties of Earth, Venus, Mars, Mercury, and the Moon are characterized.
Journal ArticleDOI

Lunar apatite with terrestrial volatile abundances

TL;DR: Quantitative ion microprobe measurements of late-stage apatite from lunar basalt 14053 are reported that document concentrations of H, Cl and S that are indistinguishable from apatites in common terrestrial igneous rocks, suggesting portions of the lunar mantle or crust are more volatile-rich than previously thought.
References
More filters
Journal ArticleDOI

To each plutonic rock its proper name

TL;DR: In this article, the IUGS Subcommission on the Systematics of Igneous Rocks agreed at Montreal, August 1972, comments on the recommendations on which the UUGS subcommission agreed.
Book

Impact Cratering: A Geologic Process

H. J. Melosh
TL;DR: In this article, the authors derived the Hugoniot equations for impact cratering, and derived the state of the art for the state for the impact crater problem in the United States.
Book

Rock Magnetism: Fundamentals and Frontiers

TL;DR: In this article, the basic magnetism in nature has been studied and the fundamental properties of magnetism have been discussed. But the authors focus on the magnetism of metamorphic and igneous rocks rather than extraterrestrial magnetism.
Journal ArticleDOI

Strength of the lithosphere: Constraints imposed by laboratory experiments

TL;DR: The concept of strength envelopes, developed in the 1970s, allowed quantitative predictions of the strength of the lithosphere based on experimentally determined constitutive equations as mentioned in this paper, which can be applied to understand a broad range of topical problems in regional and global tectonics both on the Earth and on other planetary bodies.
Related Papers (5)