This resource identifies the sources of the Earth's internal heat energy as extraterrestrial impacts, gravitational contraction of the Earth's interior, and the radioactive decay of unstable isotopes, each of which is explained in detail. A discussion of melting and compositional differentiation of the early Earth is followed by a description of the present layers, including the inner and outer core, mantle, and crust. In addition, the asthenosphere and lithosphere are described and illustrated. Educational levels: High school, Middle school, Undergraduate lower division
The Earth's mantle convects to lose heat (Holmes, 1931); doing so drives plate tectonics (Turcotte a...
The energy budget of the Earth’s core balances the heat lost through cooling with the sum of gravita...
We model the internal thermal evolution of planets with Earth-like composition and masses ranging fr...
This website contains class notes from a Geology 101 (physical geology) course. It discusses the com...
This United States Geological Survey (USGS) publication discusses the interior of the Earth, includi...
This site contains information about the crust, lithosphere, mantle, convection currents, outer core...
This set of lecture notes covers several topics relating to the earth's interior. Seismic waves and ...
Since this course is about how Earth processes can adversely affect us as human beings, we need to f...
The heat production budget of a planet exerts a first order control on its thermal evolution, tecton...
The early thermal history of the Earth is reconsidered with the constraint that core formation occur...
The energy aspects of the problem of intraterrestrial heat transfer in various forms are discussed. ...
The present internal state of the earth and the age of various events such as core formation and con...
This lesson discusses the interior structure of the earth as defined by research on the behavior of ...
The earth is considered to have been formed in several stages in a solar nebula by accretion of carb...
The magnetic field of the Earth is generated by convection in the liquid-core and the energy necessa...
The Earth's mantle convects to lose heat (Holmes, 1931); doing so drives plate tectonics (Turcotte a...
The energy budget of the Earth’s core balances the heat lost through cooling with the sum of gravita...
We model the internal thermal evolution of planets with Earth-like composition and masses ranging fr...
This website contains class notes from a Geology 101 (physical geology) course. It discusses the com...
This United States Geological Survey (USGS) publication discusses the interior of the Earth, includi...
This site contains information about the crust, lithosphere, mantle, convection currents, outer core...
This set of lecture notes covers several topics relating to the earth's interior. Seismic waves and ...
Since this course is about how Earth processes can adversely affect us as human beings, we need to f...
The heat production budget of a planet exerts a first order control on its thermal evolution, tecton...
The early thermal history of the Earth is reconsidered with the constraint that core formation occur...
The energy aspects of the problem of intraterrestrial heat transfer in various forms are discussed. ...
The present internal state of the earth and the age of various events such as core formation and con...
This lesson discusses the interior structure of the earth as defined by research on the behavior of ...
The earth is considered to have been formed in several stages in a solar nebula by accretion of carb...
The magnetic field of the Earth is generated by convection in the liquid-core and the energy necessa...
The Earth's mantle convects to lose heat (Holmes, 1931); doing so drives plate tectonics (Turcotte a...
The energy budget of the Earth’s core balances the heat lost through cooling with the sum of gravita...
We model the internal thermal evolution of planets with Earth-like composition and masses ranging fr...