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Transcript
Origins of the Ocean Planet
Resources from Garrison Textbook
(2010)
It’s Only a Theory
Laws:
• Well supported explanations that describe a
situation
• Have been supported through observable and
testable experiments
• Considered facts
Theories:
• Cannot become laws
• They explain a series of observations to try and
explain the phenomenon or situation
It’s Only a Theory
http://youtu.be/9Re8QxKZdm0
Objective 1 & 2
• Be able to describe how marine scientists
conduct investigations
• Be able to distinguish what information about
the ocean is of utmost importance to us now-adays and in the future
Earth is an Ocean World
• Facts about the Ocean
– 97% of Earth’s water is found in or near the ocean
– < 3% is found on land, ice, groundwater, and all
freshwater lakes/rivers
• Functions of the Ocean
– Moderate temperature
– Influences weather
– Nurtures life
– Crucial natural resource (renewable)
Water Amounts by Location
(Garrison, 2010)
Ocean Divisions
• Imaginary divisions that compartmentalize the
oceans and seas, by using continental
boundaries
• Truly the entire ocean (world ocean) is
connected, the terms for the oceans is meant to
simplify the compartmentalization
Ocean’s Size
• 361 million km2 (square kilometers) = 139
million squared miles
• Depth = 3,796 meters (12,451 feet)
• Volume = 1.37 billion km3 (cubic kilometers)
[329 million cubic miles]
• Average temperature = 39OF
• Mass = 1.41 billion billion metric tons
Earth Is an Ocean World
Average ocean depth is 4 ½ times as great as
average land elevation.
(Garrison, 2010)
Proportion of Sea vs. Land
(Garrison, 2010)
Comparison’s
• On a planetary scale, the Earth’s ocean is
insignificant in size
• There is more water inside the Earth’s interior
than there is in the ocean and atmosphere
S.T.E.M. Career Connection
•
•
•
•
•
•
Marine Geologists
Chemical Oceanographers
Physical Oceanographers
Climatologists
Marine Biologists
Marine Engineers
What do they do…
• Marine Geologists
– Study earth’s crust and composition
• Chemical Oceanographers
– Study the ocean’s chemical composition (gases/solids
dissolved in the ocean)
• Physical Oceanographers
– Study of the waves, currents, and climate prediction
• Climatologists
– Determine the role the ocean play’s within the changes in
the climate
• Marine Biologists
– Study the nature and distribution of marine organisms
• Marine Engineers
– Design and create structures utilized in the ocean
Studying what?????
• Oceanography
– is the study of the earth's oceans and their interlinked ecosystems , geological,
chemical and physical processes.
• Geological oceanography
• the study of geologic processes in the oceans (plate tectonics, coastal
morphology)
• Chemical oceanography
• the study of the chemistry of the oceans
• Meteorological oceanography
• the study of the interaction between atmosphere and the oceans
• Physical oceanography
• the study of the physical attributes of the oceans (temperature-salinity structure,
waves, tides, currents)
• Biological oceanography
• the study of the flora and fauna of the oceans
Three of the most prominent
oceanographic institutions in
the US:
Lamont-Doherty Earth
Observatory of Columbia
University, NY
Woods Hole
Oceanographic
Institute, Cape Code,
MA (MIT)
Scripps Institution of
Oceanography, La Jolla
CA (UC-San Diego)
Objective 3
• Describe how the study of the past can help us
predict the future of our oceans
Understanding the Ocean Began with
Voyaging for Trade and Exploration

Voyaging on water was important to many early civilizations. The
Egyptians, Cretans, and Phoenicians were all skilled sailors.

Cartographers, or chart makers, recorded information about locations
and landmarks and currents.

Today, charts are detailed graphic representations of water and waterrelated information.

The Library at Alexandria, in Egypt, was founded in the third century
B.C. This library stored information on every area of human endeavor.

Eratosthenes of Cyrene was the second librarian at Alexandria. He was
the first to calculate the circumference of Earth. He also invented a system
of longitude and latitude.

The principles of celestial navigation were invented at the Library at
Alexandria.
(Garrison, 2010)
Objective 5 & 6
• Be able to describe how life begun in the
ocean environment
• Be able to describe the intercorrelation of
studying the cosmos and the ocean
Stars and Seas
• To understand the ocean, we need to understand
how it formed and evolved through time.
• Because the world ocean is the largest feature of
Earth’s surface, scientists believe the origin of
the ocean is linked to Earth’s origin.
• The origin of Earth is linked to that of the solar
system and the galaxies.
Earth Was Formed of Material
Made in Stars
• The universe apparently had a beginning called
the big bang that occurred ~13.7 billion years
ago.
• All of the mass and energy of the universe was
concentrated at a geometric point at the beginning
of space and time, the moment when the
expansion of the universe began.
• We don’t know what initiated the expansion, but
it continues today and will probably continue for
billions of years, perhaps forever.
Stars and Planets are Contained
within Galaxies
Our Milky Way Galaxy pictured from afar. We’re inside and dust obscures our view,
but this painting is a good guess about what our galaxy looks like, based on many
different types of observations. Our solar system is a little more than half-way out from
the center in one of the blue spiral arms.
Stars and Planets Are Contained
within Galaxies
• What do stars have to do with the ocean?
• Most of the substance of Earth, its ocean, and all
living things, was formed by stars.
• Every chemical element heavier than hydrogen
was manufactured and released into space by
stars.
• Our sun, like all normal stars, is powered by
nuclear fusion.
Stars and Planets Are Contained
within Galaxies
A filament of hot gas erupts from the face of our sun. Like all normal stars, the sun is
powered by nuclear fusion – the welding together of small atoms to make larger ones.
The entire Earth could easily fit into this filament’s outstretched arms.
Stars Make Heavy Elements from
Lighter Ones
The origin of a solar
system in the spiral arm
of a galaxy. Our sun and
its family of planets
were formed in this way
about 5 billion years
ago.
Solar Systems Form by Accretion
Planet-building in progress. Accretion of planets occurs when small particles clump
into large masses.
Earth Accumulated in Layers
Sorted by Density
• How did Earth become density stratified?
• Young Earth was probably homogeneous
• Heat and gravitational pressure caused Earth to
partially melt
• Gravity then pulled the iron present into the
center of Earth
• This heated Earth further and lighter minerals
migrated to Earth’s surface and formed the crust
Earth Accumulated in Layers
Sorted by Density
(top) The planet grew by the aggregation of
particles. Meteors and asteroids bombarded
the surface, heating the new planet and
adding to its growing mass. At the time,
Earth was composed of a homogeneous
mixture of materials.
(middle) Earth lost volume because of
gravitational compression. High
temperatures in the interior turned the inner
Earth into a semisolid mass; dense iron (red
drops) fell toward the center to form the
core, while less dense silicates move
outward. Friction generated by this
movement heated Earth even more.
(bottom) The result of density stratification
is evident in the formation of an inner and
outer core, a mantle, and the crust.
Earth Accumulated in Layers
Sorted by Density
• How did water and water vapor form on early
Earth?
• The Sun stripped away Earth’s first atmosphere
• Gases, including water vapor, released by the
process of out-gassing, replaced the first
atmosphere.
• Water vapor in the atmosphere condensed into
clouds.
• Eventually, the surface cooled enough for water
to collect in basins.
Earth Accumulated in Layers
Sorted by Density
Comets may have delivered some of Earth’s surface water. Intense bombardment of the
early Earth by large bodies – comets and asteroids – probably lasted until about 3.8 billion
years ago.
Earth Accumulated in Layers
Sorted by Density
The early atmosphere was very different from the atmosphere today.
Life Probably Originated in the
Ocean
Fossil of a bacteria-like
organism (with an artist’s
reconstruction) that
photosynthesized and
released oxygen into the
atmosphere.
Among the oldest fossils
ever discovered, this
microscopic filament
from northwestern
Australia is about 3.5
billion years old.
What Will Be the Future of Earth?
• How long can Earth exist?
• Our Sun will begin to die in 5 billion years.
• 6 billion years from now the sun will enter the red
giant phase and will engulf the inner planets.
• At that time, Earth will probably be recycled into
component atoms.
• See Figure 1.8 for a timeline of Earth.
What Will Be the Future of Earth?
Are There Other Ocean Worlds?
• Where have scientists found evidence of water?
• Europa
– The gravitational pull of Jupiter twists Europa,
cracking the ice crust and warming the interior.
– In some areas the ice has broken into large pieces that
have shifted away from one another but fit together
like a jigsaw puzzle.
– This suggests the ice crust is lubricated by slush or
water. A global ocean greater in volume than Earth’s
ocean may lie beneath the movable crust. It may also
be salty - salinity has been detected by Galileo’s
magnetometers.
Are There Other Ocean Worlds?
In 2005, Europe’s Mars Express orbiter imaged a glacier in an unnamed crater in the vast
plains of northern Mars. This 200 meter (656 foot) thick remnant of a larger ice sheet is
shielded by the frosty shade of the crater walls.
Are There Other Ocean Worlds?
• Where have scientists found evidence of water?
• Titan – Saturn’s largest moon, may have an ocean
of hydrocarbons.
• Mars
– Early in its history, Mars may have had a thick
atmosphere of carbon-dioxide, much like the
atmosphere of the early Earth.
– An ocean may have existed on Mars about 3.2 billion
years ago.
– Over the eons, rocks on the Martian surface absorbed
the carbon dioxide and the atmosphere grew thin and
cold and the ocean disappeared
Resources
Garrison, T. (2010). Oceanography: An
invitation to marine science (7th ed.). Brooks
& Cole: Australia