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Introduction to Earth Science

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Presentation on theme: "Introduction to Earth Science"— Presentation transcript:

1 Introduction to Earth Science
Or, How The Earth Works

2 Branches of Earth Science
Geology Solid Earth Much Larger than Other Parts Many More Kinds of Materials Preserves a History Meteorology – Climatology Oceanography Astronomy Planetary Geology

3 The Earth Systems External Effects (Astronomical)
Atmospheric Circulation Oceanic Circulation Hydrologic Cycle Rock Cycle Plate Tectonics

4 The Solid Earth


6 Earth and the Universe (external effects)
Earths’ Rotation (Day-Night) Lunar Effects (Tides) Annual Variation (Seasons) Precession and Orbit Variations (Ice Ages?) Galactic Rotation (250 m.y. period) Unpredictable Events Nearby Supernovae Meteor Impacts Long-Term Evolution of Sun

7 Atmospheric Circulation
Unequal Solar Heating Equator to Pole Day - Night Different Surfaces Buoyancy Heating and Cooling Coriolis Effect High and Low Air Pressures Fronts and Air Masses

8 Oceanic Circulation Surface Currents - Driven by Winds
Thermohaline - Deep Circulation Evaporation makes water more saline and denser Freezing makes water more saline and denser Cold water is denser than warm water

9 Surface Currents

10 Thermohaline Circulation

11 Hydrologic Cycle Evaporation from Oceans Precipitation on Land
Infiltration into Ground (Ground Water) Runoff (Erosion)

12 Hydrologic Cycle

13 Water Principal Agent in Modifying Earth’s Surface
Medium for Storing and Distributing Global Heat The Universal Solvent Essential for Life Destructive to Rocks Lowers Melting Point of Rocks Reduces Strength of Rocks Under Pressure

14 The Rock Cycle New Rocks Exposed by Erosion
Rocks Broken Down Mechanically and Chemically (Weathering) Components Transported by Erosion Components Cemented into Sedimentary Rocks Burial and Heating creates Metamorphic Rocks Melting Creates Igneous Rocks

15 The Rock Cycle

16 Plate Tectonics Outer Crust of Earth Moves a Few cm/yr
Driven by Convection in Earth’s Interior Accounts For: Earthquakes Volcanoes Mountain-Building (Orogeny) Configuration of Continents

17 Plate Tectonics

18 Plate Tectonics and Resources

19 Configuration of Continents
Oceanic Circulation Weather and Climate Patterns Deserts Mountains and Rain Shadows Pathways for Migration Ecological Niches

20 Some Unique Aspects of Geology
Importance of Relationships Sequential Spatial Importance of Time Distinctive Problems of Evidence Slow Rates Rare Events Destruction of Evidence Inaccessibility

21 Some Geologic Rates Cutting of Grand Canyon 2 km/3 m.y. = 1 cm/15 yr
Uplift of Alps 5 km/10 m.y. = 1 cm/20 yr. Opening of Atlantic 5000 km/180 m.y. = 2.8 cm/yr. Uplift of White Mtns. (N.H.) Granites 8 km/150 m.y. = 1 cm/190 yr.

22 Some Geologic Rates Movement of San Andreas Fault
5 cm/yr = 7 m/140 yr. Growth of Mt. St. Helens 3 km/30,000 yr = 10 cm/yr. Deposition of Niagara Dolomite 100 m/ 1 m.y.? = 1 cm/100 yr.

23 1 Second = 1 Year 35 minutes to birth of Christ 1 hour+ to pyramids
3 hours to retreat of glaciers from Wisconsin 12 days = 1 million years 2 years to extinction of dinosaurs 14 years to age of Niagara Escarpment 31 years = 1 billion years

24 Some Unique Aspects of Geology (Continued)
Reliance on Inference and Deduction Intrinsically "Unsolvable" Problems Ancient Landscapes Mass Extinctions Ancient Ocean Basins

25 Scientific Principles in Geology
Parsimony (Keep It Simple) Superposition Uniformitarianism Using these, plus observation, we establish facts about Earth Processes

26 Parsimony The simplest explanation that fits all the data is preferred
Doesn’t guarantee that things must be simple! Theories with lots of ad hoc or unsupported ideas are probably wrong.

27 Superposition: Road Cut, Superior, AZ

28 Geologic Map

29 Uniformitarianism Continuity of Cause and Effect
Apply Cause and Effect to Future - Prediction Apply Cause and Effect to Present - Technology Apply Cause and Effect to Past - Uniformitarianism

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