Ch.1: The Earth in Context Flashcards

1
Q

Geology

A

The study of the earth

Focuses on materials the earth is made out of: rocks, minerals, mountains

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2
Q

Layers of the earth

A
Crust (oceanic thinner and continental thicker, boyant)
Moho = base of the crust
Upper mantle
Lower mantle
Liquid molten outer core
Solid inner core
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3
Q

Sialic vs. Mafic

A

Continental crust = sialic (Si + Al) granite

Oceanic crust = mafic (Mg + Fe) basalt

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4
Q

Lithosphere

A

Strong outer shell, about 100 km thick; plates are made of lithosphere
Crust + upper mantle

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5
Q

Asthenosphere

A

weak, zone of partial melting; flow in asthenosphere moves the over-riding plates
Upper mantle

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6
Q

Pre-Socrates

A

Believed earth was flat and in the center (geocentric)

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7
Q

Aristotle 350 BCE

A

Spherical earth surrounded by concentric spheres
Aristotle on geologic time:
“But the whole vital process of the earth takes place
so gradually and in periods of time which are so
immense compared with the length of our life, that
these changes are not observed, and before their
course can be recorded from beginning to end whole
nations perish and are destroyed.”

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8
Q

Eratosthanes 200 BCE

A

Determined earth’s size using oblekes
On summer solstice at noon in Alexandria, he measured
the length of an obelisk’s shadow.
At the same time, the sun’s rays cast no shadow down
a vertical pit in Syene, therefore the rays were vertical.
He calculated the sun’s angle from its zenith as 7.2°, or 1/50th of the earth’s circumference.

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9
Q

Copernicus

A

Published evidence for heliocentricity 15th centruty europe

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10
Q

Galileo

A

observations (phases of Venus,

moons orbiting Jupiter) confirmed heliocentrism.

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11
Q

Hutton

A
Wrote Theory of the Earth:
• Earth is very old, having " ...no vestige
of a beginning, no prospect of an end"
• Formulated idea of Uniformitarianism:
"The present is the key to the past"
18th c Scottish
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12
Q

Lynell

A

19th C.
Principles of Geology
Found fossils in rocks
“Sea has been changed into land. Marine shells lie far distant from the deep.”

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13
Q

Big Bang

A

13.8 billion years ago
This theory proposes that all matter and energy in the Universe started out as a single infinitesimally small point that exploded and has been expanding ever since

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14
Q

Nebular Theory

A

~4.6 billion years ago from older stars.
The nebula condensed into a protoplanetary disk.
The center of the nebular disk glowed with heat and ignited into nuclear fusion.
big bang-> disk -> stars -> planets->differentiation->moon

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15
Q

Planetary Acretion Model

A

The dust in the rings accreted or coalesced to form planetesimals, which gradually combined into planets.

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16
Q

Earth and moon formation

A

1) Nebula becomes a disk
2) Birth of the sun
3) Planetesimals coalesce
4) Differentiation
5) Moon formation
6) Atmosphere evolves
After earth’s differentiation, a Mars-sized planetoid collided with us, blasting out a large part of the mantle.
Debris from the collision coalesced to form the Moon

17
Q

Differentiation of the Earth’s Interior

A

Early on, the Earth was fairly homogeneous inside.
When the temperature got hot enough, iron began to melt. The iron accumulated at the center of the planet to form a metallic core.

18
Q

Composition of the earth as a whole

A
90% percent of Earth is comprised of 4 elements
– Iron (Fe) – 35%
– Oxygen (O) – 30%
– Silicon (Si) – 15%
– Magnesium (Mg) – 10%
• The remaining elements
– Form 10% of Earth
MAFIC ( rich in Magnesium and Iron)
19
Q

Composition of Earth’s crust

A
Oxygen 46%
Silicon 28%
Aluminum 11%
Iron 6%
SIALIC (rich in Silicon and Aluminum)
20
Q

Henry Hess

A

Sea floor spreading

21
Q

Robert Diatz

A

Subduction

22
Q

J. Tuzo Wilson

A

Hot spot volcano track

23
Q

Wadarti and Benioff

A

Inclined plane of earthquakes within subduction zone

24
Q

Tanya Atwater

A

San Andreas Fault