Lecture 2: The Planet Earth Flashcards

1
Q

Differentiate heliocentrism from geocentrism

A

Heliocentrism - Copernican Model

Geocentrism - Ptolemaic Model

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2
Q

Explain the Big Bang

A

“singularity” – explosion of space-time; extremely hot and dense state which expanded rapidly and then slowly (dark matter) while cooling

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3
Q

What were the pieces of evidence for the Big Bang?

A
  1. Hubble’s Law (red shift) – 1929; star moves away
  2. Cosmic Microwave Background Radiation – remnant/heat
  3. Abundance of H, He
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4
Q

What were the limitations of the big bang?

A
  1. Only explains the universe
  2. What was present before Big Bang?
  3. How will it end? Will it ever end?
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5
Q

Explain how the solar system forms

A

spins (contraction)

  • conversion of Gravitational Energy to Thermal Energy
  • cooling
  • Temperature coalesce forming extraterrestrial bodies
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6
Q

Differentiate terrestrial planets and jovian planets in terms of:
*composition

A

Rocky composition
Gaseous liquid form composition
(denser materials go through the center of mass)

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7
Q

Differentiate terrestrial planets and jovian planets in terms of:
*elements

A
Si, Fe, O (Silicate rocks and metals)
Light elements (H, He, Ar, C, O, Ni)
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8
Q

shape of earth

A

Oblate Spheroid

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9
Q

Describe Oblate Spheroid

A

*flattened at poles; bulging at the equator

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10
Q

Earth’s Axial Tilt

A

21.5 to 24.5 degrees

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11
Q

Obliquity

A

23.4 degrees

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12
Q

Orbital Speed

A

30 km/s

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13
Q

Nebula planetesimals protoplanets

A

accretion, differentiation

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14
Q
  • accretion * differentiaion *
A

Nebula, planetesimals, protoplanets

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15
Q

*: the process of growth or increase, typically by the gradual accumulation of additional layers of material

A

Accretion

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16
Q

Accretion: the process of * or increase, typically by the gradual * of additional * of material

A

growth, accumulation, layers

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17
Q

*: random chunks of primordial matter were transformed into a body whose interior is divided into concentric layers that differ from one another both physically and chemically.

A

Differentiation

18
Q

Differentiation: random * were transformed into a * whose interior is divided into * that * from one another both physically and chemically.

A

chunks of primordial matter, body, concentric layers, differ

19
Q

In Stage 1 of the formation of earth:

A

Fe, O, Si, Mg

*no continents, oceans, atmospheres

20
Q

*Temperature of the planet reached and surpassed the melting point of iron; denser elements sink to center and lighter elements float to top.

A

Iron Catastrophe

21
Q

Chemically distinct layers

  • Core:
  • Mantle:
  • Crust:
A

Fe, Ni
O, Si, Fe, Mg
O, Si

22
Q

exposures on the surface of the Earth; large scale sequence of rocks

A

Ophiolites

23
Q

foreign rock (rock from mantle)

24
Q

CO Age

A

4 Ga

160 Ma

25
CO Thickness
35-40 km, 7-10 km
26
CO Composition
Granitic (Si, O) | Basaltic (Mg, Fe)
27
CO Density
2.7 g/cc, 3.0 g/cc
28
* is the thickest layer | how thick?
Mantle | ~2,900 km
29
Mantle is rich in the mineral
perovskite
30
uppermost mantle rock type:
peridotite
31
Core is ____ alloy
Fe-Ni
32
Crust * Mantle * Outer Core * Inner core | {Discontinuity}
Crust Mantle Outer Core
33
Layers of Earth according to Physical Properties:
Lithosphere,
34
Lithosphere is composed of: | It is ______
Crust + uppermost mantle * solid but brittle * ~100 km
35
contrary to lithosphere, asthenosphere is ...
solid but plastic or mobile
36
*weak layer resulting from temperature/pressure conditions
asthenosphere
37
*solid, rocky layer
mesosphere
38
* 2,900 – 5,100 km in depth | * molten
outer core
39
* 5,100 – 6,370 km in depth | * solid
inner core
40
Differentiation of Earth’s Interior: P-waves: S-waves:
parehong solid and liquid | solid lang