INTRODUCTION
The Origin of the Earth
Origin of the solar system.
How and when did it begin? Any theory must answer the following:
Hypotheses to explain the origin of the solar system
Gross Structure of the Earth's Interior (Figure below)
1) Crust - 5-50 km thick. Density 2.85 gr/cm3
2) Mantle - 2900 km thick. Density 3.3 gr/cm3
3) Core - 3400 km thick. Density 15 gr/cm3
Knowledge of the interior structure of the Earth is based largely on the study of seismic waves as they travel through the Earth and studies of meteorites, which are thought to represent fragments of extraterrestrial planetary material.
Planetary Evolution
No recent hypothesis. Thought that planetesimals form by accretion of condensed clumps of silicon. oxygen, iron and magnesium. Accreted material attracted to other accreted material by the force of gravity. Compression provides heat. Further infalling chunks of material convert energy of motion to heat energy. Finally radioactivity generates additional heat. All three combine to heat Earth to the melting point. Iron and magnesium sink to the core (iron catastrophe). This differentiates the Earth into a core and mantle/crust.
|
Elemental Composition of the Earth |
||
|
Element |
Crust (wt.%) |
Core (wt.%) |
|
Oxygen |
46.6 |
30 |
|
Silicon |
27.7 |
15 |
|
Aluminum |
8.1 |
1 |
|
Iron |
5.0 |
35 |
|
Calcium |
3.6 |
-- |
|
Sodium |
2.8 |
-- |
|
Potassium |
2.6 |
-- |
|
Magnesium |
2.1 |
17 |
Looking at the Crust
a) Igneous rock - Formed from the cooling of a magma.
b) Sedimentary rock - Rocks formed from fragments of pre-existing rocks at the Earth's surface in response to weathering.
c) Metamorphic rock - Rocks which are changed from their original nature in response to heat and pressure.
Geologic Time
Basic Concepts
Types of Geologic Time
Relative Time
First attempts to establish ages based on relative age dating and the basic principles given above. Go through figures on relative age dating.
These attempts worked only over short distances (physical correlation). The problem is what happens over longer distances. Introduce the concept of differing sedimentary facies due to differences in the environments of deposition. Use analogy of So. Cal. (Figure) showing different environments of deposition. Another example is England and France (Figure).

Second figure shows how the correlation using fossils in England and France was much more successful (Figure). With fossil assemblages it is possible to create a chronologic sequence of rocks based on relative ages. This sequence is termed the Geologic Column.

Geologic Time Scale
Precambrian - Thought to represent all rocks deposited prior to the evolution of life. Now recognized to be period of time prior to the evolution of complex organisms. (4/5 ths of earth's history)
Paleozoic - Generally period of time when life was confined to the seas. (about 1/2 of the remaining 1/5th)
Absolute Time
While relative time provides useful information regarding the timing of one event relative to another, it does nothing to answer the fundamental question about the age of the Earth.
Early Attempts at Absolute Age Dating
Radioactive Decay
Matter - Anything that occupies space and can be seen by the human eye. Definition serves well until the first microscope is built (17th century). Scientists realize there are particles smaller than the eye can see.
Atom - The smallest particle of which matter is composed.
Scientists could not see atoms, but over centuries they devised a model of the atom based on simple logic. They reasoned the atom had to be composed of at least two sub-atomic particles, which they termed the proton (+) and the electron (-). The latter revolved in orbitals around the former, analogous to the revolution of the planets around the Sun. Mass deficiencies lead them to propose a third sub-atomic particle, the neutron (no charge) which they place in the nucleus with the protons. From this was born the concept of the element.
Element - A unique combination of protons, electrons and neutrons. Each element differs in the number of protons in the nucleus.
Atomic Number - The number of protons in an atom of a particular element.
Atomic Weight - The number of protons and neutrons. Electrons have less than 1% of the total mass of an atom and can be ignored.
Late in the 19th century the theory of radioactivity was first proposed. It explained why certain elements were unstable, that is, they were observed to spontaneously decay to other differing elements. Central to this theory was the concept of the isotope.
Isotope - An atom of an element that differs from another atom of the same element only by the number of neutrons in the nucleus. Example 12C 13C 14C
Certain isotopes are radiogenic (unstable) and with time will decay to another element. There are several decay schemes.
Decay Schemes

The usefulness of radioactive decay to geology comes from the fact that the rate of decay is a constant that is unaffected by any physical process. Figure shows how the decay of parent atoms and growth of daughter atoms with time.

How does it work in nature?
Using this method we can date:
Since we cannot age date most sedimentary rocks and the geologic column was complied on the basis of sedimentary rocks we have a slight problem assigning ages to rocks in the geologic column. Figure shows how we reconciled this problem.

The age of the Earth based on
From these the age of the Earth is at least 4.5 BY and generally agreed to be 4.6 BY.