Lecture 1-8 Flashcards

1
Q

What is a planet?

A

Cold object that orbita around a central luminous start

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2
Q

What is a Planetary body?

A

General term for any body orbiting a star includes planets and their natural satellites/moons

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3
Q

Terrestrial (Inner) planets

A

Relatively small, rocky (“Earth-like”) bodies closest to the sun
↳ moon is studied as a terrestrial planet

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4
Q

General planet info

A
  • Mercury
    ↳ larger than earths moon & closes to sun
  • Venus
    ↳ 2nd closest planet & shrouded by clouds
    ↳ lots of craters and mountain belts
  • Earth
    ↳ lots of plate tectonics, erosion, has life along with atmosphere
  • Moon
    ↳ orbits earth
  • Mars
    ↳ very thin atmosphere
    ↳ erosion by water, lots of volcanoes & valleys
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5
Q

Asteroid

A

small rocky or metal-rich planetary body orbiting the sun

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6
Q

Asteroid belt

A
  • region between the orbits of Mars and Jupiter where most asteroids are found
  • asteroids range from 1 - 1000km in diamerter
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7
Q

Gas Giants (outer Planets)

A

Large planets that have a deep atmosphere and no solid surfaces
↳ icy/rocky

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8
Q

Comets

A

small, ice rich bodies which formed at the outer edges of the solar system

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9
Q

Neptune & Uranus

A
  • Both are gas and ice rich
  • Have icy moons
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10
Q

The three main tock types

A

Igneous, Sedimentary, and Metamorphic

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11
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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12
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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13
Q

Law of Inclusions?

A

One rock included in another is older than the rock that includes it

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14
Q

Law of original horizontality

A

Sedimentary layers are deposited horizontally

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15
Q

Crust

A

The outermost layer, on top of the mantle

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16
Q

Mantle

A

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

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17
Q

Asthenosphere

A

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

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18
Q

Lithosphere

A

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

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19
Q

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

A

Density, Seismic data, Meteorites

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20
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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21
Q

Fusion

A

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

22
Q

What Keeps a Star together?

A
  • Gravity attempts to make the star collapse
  • High gas pressure opposes gravity
23
Q

Supernova

A

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

24
Q

Nebula

A

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

25
Gravitational Collapse
When molecules are concentrated, attracted to each other; may be triggered by a nearby supernova
26
T Tauri stars
stars that are similar in mass to the Sun, but only about 1 million years old
27
Proplyds
disks of dust and gas around young stars; contraction of “protoplanetary disks"
28
Meteorites
extraterrestrial rock that's fallen through our atmosphere
29
Refractory
materials that form solids at very high temperatures
30
Volatile
materials that condense/solidify at very low temperatures
31
Planetesimal
Small solid bodies, ~100km across, that formed from grain-to-grain accretion of dust
32
Accretion
Solids come together to form larger objects through gravitational attraction and collisions
33
Differentiation
The separation of materials in a planetary body according to density and chemical affinity
34
Conduction
The vibrational energy of an atom is transferred to adjacent atoms
35
Convection
Warm material expands and moves upwards, displacing cooler, denser materials downwards
36
Radiation
The emission of electromagnetic waves from a hot body’s surface to its surroundings
37
Law of Cross-cutting Relationships for impact cratering
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
38
Three things that must be explained by any model for how the solar system was formed
- 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
39
Why the Moon always shows the same side to the Earth
The period of rotation and period of revolution are exactly the same
40
Two surfaces on the Moon that can be easily seen from Earth
- Maria (smooth surfaces) - Terrae (cratered highland)
41
Crater sizes on the moon
- 20 to 200km diam ↳ have central peaks - crater > 300km diam ↳ called multi ring basins & spacing of rings increases outward
42
What is KREEP
KREEP is a component found in soils, breccias and impact melts
43
Fire fountaining
Volcanic activity on the Moon, it creates Lunar Glass Beads
44
Anorthosite
Most abundant and oldest rock type
45
Breccia
A rock made up of angular fragments of other rocks ↳ more basalts
46
Regolith
- Mixture of rock fragments - Formed during micrometeorite impacts;
47
Explain why mare basalts can flow such great distances on the Moon
They contain more iron and less silicate and aluminum, which causes lunar basalts to have a lower viscosity
48
List the main observations that any model for the formation of the Moon must explain
- size of the moon relative to earth - The low bulk density/size of its iron core and its composition - Moon has little water and is depleted in other elements - it's orbit
49
Giant Impact Hypothesis
- The giant impact hypothesis proposes that the Moon formed from debris ejected during a collision between the early Earth and a Mars-sized protoplanet around 4.5 billion years ago.
50
The major discoveries made by the Lunar Reconnaissance Orbiter mission
evidence of water on the Moon, Moon caves, map of the lunar south poles, more topography, temperature map
51
Describe how the crystallization of a magma ocean explains the anorthosite composition of the Moon’s crust
- pyroxene and olivine in the magma sink and the anorthosite (lighter mineral) floats