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An Introduction to the World’s Oceans Chap. Two - 8th Ed.
The Water Planet An Introduction to the World’s Oceans Chap. Two - 8th Ed.
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Chapter Two Highlights
Origin of our universe & solar system GeologicTime Shape & orientation of the Earth relative to the Sun Mapping and location systems Navigation The Water Cycle
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Beginnings Origin of the universe Origin of our solar system
Big Bang model Stars, galaxies, and clusters Wilkinson Microwave Anisotropy Probe - 380,000 years post BB Hubble Space Telescope (HST) Origin of our solar system Collapse of a rotating interstellar cloud Accretion to form planets
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Earth Origins Big Bang !!!! 13 bya extremely hot
subsequent formation of ~100 million galaxies with ~ million stars each Milky Way is our spiral galaxy ( galaktos = milk )
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A spiral galaxy structurally similar to the Milky Way Galaxy
A spiral galaxy structurally similar to the Milky Way Galaxy. 56,000 light years in diameter and 62 million years away.
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Earth Origins Planetary Accretion Theory 5 bya
solar nebula (swirling dust cloud) from a supernova ~75% H, 23% He, 2% other stuff most material drawn to center to form protosun rest accretes to form planets
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1 light year ~ 9.5 X 1012 kms.
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Origin of the Solar System and Earth
Cloud of gas and space dust (nebula) began to contract about 4.53 billion years ago. The Nebular Hypothesis
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Conceptualization of planetary accretion.
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Hubble Space Telescope image of solar nebula similar in size to ours
Hubble Space Telescope image of solar nebula similar in size to ours. Obscuring dust cloud across center.
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First image of a “possible” planet outside of our solar system.
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Water in the S0lar System
Extraterrestrial oceans Liquid oceans on Jupiter’s moons, Europa and Callisto Early planet Earth Separation of dense and lighter compounds through repeated melting and solidifying layered system, ocean, and atmosphere No free oxygen until photosynthetic organisms evolved
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Mars shows erosional and depositional features that suggest the presence of running water in the past.
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Origin of the Oceans Age of Earth: approximately 4 billion years
Water from interior of Earth Mantle Gas that escape volcanoes is 70% water vapor 4 billion years at current rate 100 times the volume of the oceans Water from outer space 10 million comets enter the atmosphere each year Layer of water mm deep added each year 4 billion years at current rate 2 to 3 times the volume of the oceans
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Outgassing
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Box Fig. 1, pg. 30
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Box Fig. 2, pg. 31
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Comets
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Age and Time Age of Earth Geologic time Natural time periods
History of estimates Bible 10/23/4004 B.C. , cooling time, rate of addition of salt in oceans by rivers, radiometric dating Radiometric dating billion years Geologic time Eons, eras, periods, epochs Important events Natural time periods Time required for Earth to complete one orbit around the Sun Length of day and seasons Lunar month Solar day Sidereal day
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A Timeline Of Earth’s History
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Table 2.2 bottom
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Table 2.2 top
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Fig. 2.6
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Shape of Earth Gravity Earth is nearly spherical Spin
Earth bulges at equator Distribution of continents Slightly pear shaped Topographic relief Minor compared to planet’s size
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Fig. 2.7
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Location Systems Latitude and longitude Chart projections
Latitudes (or parallels) are parallel to the equator Longitudes (or meridians) are formed at right angles to the latitude lines Prime meridian and international date line Great Circle Nautical mile (1 minute of arc at the equator) Chart projections Distorted images of Earth’s curved surface Projection types: cylindric, conic, and tangent
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Fig. 2.8
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Fig. 2.9
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Fig. 2.10
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Fig. 2.11
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Fig. 2.12
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Fig. 2.13
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Fig. 2.14
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Fig. 2.15
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Location Systems Measuring latitude North Star, Polaris
Longitude and time Use of clocks to record the time the Sun is at its zenith Greenwich Mean Time (GMT) or Universal Time
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Fig. 2.16
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Fig. 2.17
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Modern Navigational Techniques
Radar (radio detecting and ranging) Loran (long-range navigation) Satellite navigation system Global Positioning System (GPS) Shipboard computers Electronic atlas Surface charts Bathymetry Continuous tracking of ship’s position
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Fig. 2.18a
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Fig. 2.18b
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Earth: The Water Planet
Water on Earth’s surface Effect of seasons Effects length of day 71% of Earth’s surface is covered by water, while 29% of the surface area is land Hydrologic cycle Evaporation, transpiration, and sublimation Precipitation, rain, and snow
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Fig. 2.19
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Earth: The Water Planet
Reservoirs and residence time Large reservoirs long residence time Small reservoirs short residence time Distribution of land and water Northern Hemisphere (land) Southern Hemisphere (water) Oceans Hypsographic curve
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Fig. 2.20
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Table 2.3
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Geography of the oceans
Earth’s oceans: Cover 70.8% of Earth’s surface Are interconnected (“world ocean”) Have huge size and volume (as a reservoir, contain 97% of Earth’s water)
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Fig. 2.21
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Fig. 2.22
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The four principal oceans
Fig. 2.23
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Fig. 2.24
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The End
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