Lectures 2-4 Flashcards

1
Q

The three main tock types

A

Igneous, Sedimentary, and Metamorphic

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2
Q

Law of Original Horizontality?

A

Sedimentary layers are deposited horizontally and continuously

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3
Q

Law of Superposition?

A

Each layer of sediment is older than the layer above it and younger than the layer below it

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4
Q

Law of Cross-cutting Relationships?

A

If a fault or other body of rock cuts through another body of rock then it must be younger in age than the rock through which it cuts

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5
Q

Law of Inclusions?

A

Clasts in a rock are older than the rock itself

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6
Q

Crust

A

The outermost layer, on top of the mantle

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7
Q

Mantle

A

It has upper and lower sections and includes the asthenosphere, iron, and magnesium-rich silicate minerals

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8
Q

Core

A

Mostly iron metal (very dense), solid inner core, liquid outer core

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9
Q

Asthenosphere

A

The top part of the upper mantle where it is plastic, and partly molten

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10
Q

Lithosphere

A

includes the rigid part of the mantle and the overlying crust, rides on the plastic asthenosphere

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11
Q

The three ways we know what the interior of the Earth looks like

A

Density, Seismic data, Meteorites

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12
Q

Main geologic processes active on Earth today

A

Tectonics, volcanic activity, mass wasting, water, wind, ice -> erosion and deposition of sediment, impact crater, life

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13
Q

Fusion

A

The combination of two or more nuclei to form a different, heavier, element; the by-product is radiation

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14
Q

Supernova

A

The cataclysmic explosion of a star, as a result of internal nuclear reactions

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15
Q

Nebula

A

Dust in space with a density of 1,000 gas molecules/10cm^3

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16
Q

Gravitational Collapse

A

When molecules are concentrated, attracted to each other; may be triggered by a nearby supernova

17
Q

T Tauri Star

A

Stars that are similar to the Sun, but only about 1 million years old

18
Q

Proplyds (Protoplanetary disk)

A

Disks of dust and gas around young stars, places where planets are possibly forming

19
Q

Refractory

A

Materials that condense at very high temperatures

20
Q

Volatile

A

Materials that condense at very low temperatures

21
Q

Meteorite

A

An extra terrestrial rock that has fallen through our atmosphere

22
Q

The two main sources of information for how the solar system formed

A

Astronomical observations and meteorite studies

23
Q

Planetesimal

A

Small solid bodies, ~100km across, that formed from grain-to-grain accretion of dust

24
Q

Accretion

A

Solids come together to form larger objects through gravitational attraction and collisions

25
Q

Differentiation

A

The separation of materials in a planetary body according to density and chemical affinity

26
Q

Conduction

A

The vibrational energy of an atom is transferred to adjacent atoms

27
Q

Convection

A

Warm material expands and moves upwards, displacing cooler, denser materials downwards

28
Q

Radiation

A

The emission of electromagnetic waves from a hot body’s surface to its surroundings

29
Q

Law of Cross-cutting Relationships for impact cratering

A

If an impact crater, fault, or body of rock cuts through another body of rock then it must be younger than the rock through which it cuts

30
Q

Three things that must be explained by any model for how the solar system was formed

A
  • The planets orbit in the same plane
  • They orbit the Sun in the same direction
  • The Solar System is zoned from rocky inner planets to gas-rich outer planets to ice-rich comets
31
Q

What Earth most likely looked like 3.8 Ga ago

A

Most of the surface is covered in an iron-rich ocean, a carbon dioxide-rich atmosphere, and surface temperature over 75 degrees