|
Welcome
to GLG101C Introduction to Geology
Fall 2004
Professor James Tyburczy |
Department
of Geological Sciences |
|
|
|
Chapter
1 Notes |
Note: These notes are intended
to give a brief overview of important topics in each chapter. They are not
a substitute for reading the textbook or for actually attending class.
updated 27 Aug 2004
Here are a few fun and interesting
web sites giving an overview of Geology and Plate Tectonics:
Chapter 1. BUILDING A
PLANET
Why study geology?
- Earth resources
- oil, minerals, groundwater
- Natural Disasters/Geologic
hazards - volcanoes, earthquakes, floods, landslides
- Understanding
the world around you
- Protecting the global
environment - groundwater, atmosphere/climate, waste disposal, mining
Basic themes throughout the course
- Earth as a system
of interacting components or sub-systems
- Plate Tectonics as a
unifying theory of Geology
- Changing Earth Systems
through Geologic Time
The Scientific Method -
observation, hypothesis, repeated testing of the hypothesis, theory
- Scientific Theory - coherent
explanation of for some natural phenomenon that is supported by a large body
of evidence. Make predictions, test predictions.
Uniformitarianism
- 'The present is the key to the past' -
- Types of geological processes
that shaped the Earth in the past are the same as those we can see and understand
operating today
Origin
of the Solar System and of the Earth
- Big Bang, Solar
nebula, contraction, condensation of the planets - 10 -15 billion years ago
- Earth accretion,
self-compression, heating, differentiation - Earth formed about 4.5
billion years ago
- Formation of the Moon
- Giant impact of Mars-sized body very early in Earth history - 4.5 billion
years ago
The Solar System
- Inner (Terrestrial)
Planets - Mercury, Venus, Earth, Mars - 'rocky'
- Outer Planets - Jupiter,
Saturn, Uranus, Neptune, Pluto - large, gaseous
- Other solar systems -
about 90 extra solar planets discovered so far
Earth's interior - Planetary
Differentiation
- Core - inner
core is solid, outer core is liquid, both are mostly iron (Fe)
- Mantle - most
of the Earth, made of solid silicates but convects (flows)
- Crust - thin
skin on surface, silicates
- Atmosphere/Oceans - volcanic
gases from Earth's interior or late stage coating from comets?
Elemental composition of
the Earth
- Whole Earth -
Iron (Fe) is most abundant, followed by Oxygen (O), Silicon (Si), and Magnesium
(Mg)
- Earth's Crust
- Oxygen (O) is most abundant, followed by Silicon (Si), Aluminum (Al), Iron
(Fe), and Magnesium (Mg)
Earth's Heat Engines
- Internal Heat Engine
of the Earth - heat from radioactive decay inside the Earth plus heat
from accretion drives mantle
convection, which is ultimately responsible for mountain building, earthquakes,
volcanoes, and plate tectonics on the Earth's surface
- External Heat Engine
- Solar energy provides energy for atmospheric circulation, weather, ocean
currents, and the hydrologic cycle. Precipitation and runoff erode
and disintegrate rocks, wear down mountains, form sediments
Earth as a system of
interacting components
- Atmosphere
- Hydrosphere
- Lithosphere (orLithospheric
plate) - major unit of plate tectonics, contains crust and uppermost mantle,
rigid, about 100 km thick
- Asthenosphere
- upper mantle below lithosphere, plastic, flows
- Deep Mantle
- Outer Core
- Inner Core
- Biosphere (Life is found
in Atmosphere, Hydrosphere, Lithosphere)
Interacting Earth Systems
- Climate System - Atmosphere,
Hydrosphere, Biospehre, Lithosphere - driven by solar energy (external energy)
- Plate Tectonic System
- Lithosphere, Asthenosphere, Deep Mantle - driven by Earth's internal energy
- Geodynamo System - Outer
core, inner core, Earth's magnetic field (internal energy)
Plate Tectonics - theory
- Lithospheric
plate or lithosphere- major unit of plate tectonics, contains crust and uppermost
mantle, rigid, about 100 km thick
- Asthenosphere
- upper mantle below lithosphere, plastic, flows
- Crust/mantle boundary
vs. lithosphere/asthenosphere boundary - crust-to-mantle is a difference in
chemical composition (and mineralogy and rock type). Lithosphere-to-asthenosphere
is a difference in strength
3 types of plate
margins:
- Divergent
margin -spreading centers - mid-ocean ridges, form new oceanic lithosphere
- Transform
margin - plates slide by one another (ex. San Andreas)
- Convergent
margin - for example, subduction zone -> volcanism, mountains
Geologic Time -
Darth is 4.5 billion (4,500,000,000 or 4.5 x 10^9) years old. Major events in
the history of the Earth
- 4.5 billiion years (b.y)
ago - Earth formed
- 4.0 b.y ago - heavy bombardment
ends - stable crust is formed
- 3.5 b,y ago - earliest
evidence for life - fossils of single celled bacteria
- 2.5 b.y ago - oxygen
begins to be a major compoenent of the atmosphere - because photosynthesis
is occurring - plant life
- 600 million years ago
(m.y.) - first animals
- 543 m.y. ago - Biology's
Big Bang - explosion of new life forms - earthworms, starfish, sand dollars,
moluscs, insects, trilobites, first appear - snimals with hard, calcium-rich
body parts appear.
- 65 m.y. ago - Major bolide
impact causes a mass extinction and ends the age of the dinosaurs
- 5 m.y. ago - first hominids
- 120,000 years ago - humand
first appeared
©2004, James A. Tyburczy, Department of Geologicl Sciences, Arizona
State University
If you have any questions or concerns regarding this page, please address
them to jim.tyburczy@asu.edu.
Be specific in your description of the problem!
Last update 8/27/04
|