Lecture 7 - The Terrestrial and Jovian Planets Flashcards

1
Q

what are the 3 layers of Earth?

A
  1. Core
  2. Mantle
  3. Crust
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2
Q

what is the density of the core?
what is it made of? what is happening to these elements?
outer core vs. inner core

A

core has highest density

made of nickel and iron –> heavy metals slowly burning away via nuclear fission

outer core is molten, inner core is solid bc of high pressure even tho higher temp

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3
Q

what is the density of the mantle?

what is it made of? how do we know this?

A

moderate density

made of silicon + oxygen, we know about this because of earthquakes propagating soundwaves thru it

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4
Q

what is the density of the crust?

what is it made of?

where is it thick? where is it thin?

A

lowest density

made of granite, basalt

thick where land is, thin where water is

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5
Q

describe what happens during differentiation

what does this indicate about Earth’s temp?

A

gravity pulls high-density material to center and low-density material rises to surface –> allows material to be separated by density

planet must have been hot enough for interior rock and lithium to melt

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6
Q

is the lithosphere related to lithium?

A

no

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7
Q

what is the lithosphere? what happens when it is thick/thin?

A

outer layer of cool, rigid rock that “floats” on warmer, softer rock beneath

thin = brittle, cracks easily
thick = stronger, prevents passage of molten rock so there are less volcanic eruptions and mountain formations

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8
Q

which planet is taken up the most by its metal core?

A

mercury

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9
Q

what do geological processes on planets lead to? what is this driven by

A
  1. volcanic eruptions
  2. earthquakes
  3. erosion

driven by interiors heating up and cooling off from sun’s nuclear fusion

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10
Q

what is fueled by heat of nuclear fusion from the sun? what are 2 exceptions?

A

EVERYTHING is fueled by heat of nuclear fusion from sun

  1. except heat pumps using fluid to heat from core of earth
  2. except tidal power using energy of tides extracted from orbits to generate power with turbines
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11
Q

what are the 3 sources of energy for heating planets?

A
  1. accretion
  2. differentiation
  3. radioactive decay
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12
Q

how is energy produced via accretion?

A

gravitational PE converted to KE converted to thermal energy when planets were young

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13
Q

how is energy produced from differentiation?

A

light materials rise, dense materials fall and convert gravitational PE to thermal energy when planets were young

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14
Q

how is energy produced from radioactive decay?

A

mass-energy contained in nuclei converted to thermal energy (from sun)

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15
Q

why are planets slowly cooling?

A

due to fewer collisions

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16
Q

what are the 3 sources for planets cooling?

A
  1. convection
  2. conduction
  3. radiation
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17
Q

what is convection?

A

transports heat as hot material rises and cool material falls

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18
Q

what is conduction?

A

transfers heat from hot to cool material

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19
Q

what is radiation?

A

sends energy to space

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20
Q

what is geological activity controlled by?

A

planetary size controls geological activity

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21
Q

what happens to smaller planets? what has happened to mercury and the moon?

A

cool off faster and harden earlier bc easier to get heat out

mercury and the moon now geologically dead

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22
Q

what happens to craters if a planet has no crust?

A

if a planet has no crust, there would be no craters

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23
Q

are magnetic fields constant?

A

no, they change very quickly

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24
Q

what cause magnetic fields in a planet(2)?

A
  1. motions of charged particles
  2. molten core
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25
are the magnetic poles on Earth a monopole? what happens to magnetic North each year?
North and South magnetic poles are always connected --> NEVER a monopole magnetic north changes every year
26
what are the 3 requirements for magnetic fields on a planet?
1. molten, electrically conducting interior (moving charged particles) 2. convection 3. moderately rapid rotation
27
which of convection, conduction, or radiation is responsible for how energy is transported from sun to Earth?
RADIATION
28
What does Einstein's theory of relativity prove?
can never prove anything --> has been disproven
29
when does Einstein's theory apply? when is it a poor description of events?
applies only when things are really heavy (planets, black hole) poor description when gravity and quantum mechanics are involved bc Einstein doesn't account for uncertainty
30
what are 2 situations where Einstein's theory doesn't make sense?
1. doesn't make sense with Big Bang 2. doesn't make sense with Black Hole --> Einstein says infinite density
31
what are 4 processes that shape surfaces?
1. impact cratering 2. volcanism 3. tectonics 4. erosion
32
how does impact cratering shape surfaces? when did most of this occur?
planet impacted by asteroids or comets that releases enough energy to vapourize solid rock and debris flying onto planet or into space most craters occurred soon after the solar system was formed
33
are there more large or small craters? what does this indicate?
more small craters --> indicates more small planetesimals formed during the birth of the solar system
34
why do we not see the meteorite? where do we find fragments?
cannot see the meteorite bc the heat produced caused it to vapourize bit often find fragments within or near the crater
35
is there a lot of energy in the collision of a crater?
YES
36
What is volcanism? what does it require?
eruption of molten rock (magma) thru lithosphere onto surface --> then molten rock becomes lava at surface requires internal heat
37
what does the thickest type of lava make?
steep-sloped volcanoes --> stratovolcanoes
38
what type of volcano does slightly runny lava make?
shallow-sloped volcanoes --> shield volcanoes
39
what does runny lava make?
flat volcanic plains like on the moon
40
is the moon geologically dead or alive?
dead
41
what are tectonics? what causes it and what is required for this process?
disruption of a planet's surface by internal stresses caused by convection of the mantle that produces stresses in the crust --> Tectonic Forces requires internal heat
42
what creates mountain ranges?
compression of crust from tectonics
43
what creates valleys?
forms where crust is pulled apart
44
how do Earth's continents slide around?
slide around on separate plates of crust
45
describe plate tectonics on earth
plates are produced from ongoing stress of mantle convection that fractures the lithosphere into >dozen pieces plates move over, under, and around each other
46
what do measurements of plate motions tell us?
tells us past and future layout of continents and geological features
47
describe structures on mercury that are due to tectonics and how does this affect mercury's size?
mercury has long cliffs which indicate it shrank early in its history
48
what causes erosion?
wind, water, ice --> break down or transport rock
49
when did most cratering occur?
in the first billion years
50
what does it mean if a planet has many craters? what does this indicate about the age of the surface
its surface has not changed much in the past 3 billion years more craters = older surface
51
describe cratering on the moon what happened to the younger regions? why do we know that the surface has remained unchanged for billions of years?
some areas more heavily cratered than others younger regions were flooded by lava after most cratering but we see many craters so the surface has remained virtually unchanged for billions of years
52
does earth have a lot or few craters? what does this indicate about its age?
earth has very few craters so it is younger
53
describe Lunar Maria vs Lunar Highlands in terms of craters and age when did heavy bombardment likely end? why?
Lunar Maria - smooth + dark, less craters - 3-3.9 billion years old Lunar Highlands - craters on top of craters - 4.4 billion years old therefore, the lava flow that made the volcanic plains had occurred by that time and heavy bombardment must have ended by 4 billion years ago
54
why do we not see significant crater features on Earth like Mercury and the Moon?
erosion and volcanic activity on Earth has resurfaced the earth since it was heavily bombarded
55
what happens to geology on smaller planets? larger planets?
SMALLER: cool off faster and harden earlier so geology ends soon bc the surface stops changing sooner --> therefore more craters, no atmosphere so no erosion LARGER: remain warm to cause convection in mantle, promote volcanism, tectonics, and erosion due to gravity retaining an atmosphere, and molten core may produce magnetic field if rotation is fast enough
56
describe the atmosphere of larger planets
larger atmosphere bc their
57
describe the relationship between distance from sun and erosion
close to sun: - too hot for rain, snow, ice - difficulty in retaining an atmosphere - less erosion far from sun: - too cold for rain - less erosion medium distance: - liquid water
58
how does the speed of rotation affect: 1. weather 2. erosion 3. magnetic field
SLOW ROTATION: 1. less weather 2. less erosion 3. weak magnetic field FAST ROTATION: 1. more weather 2. more erosion 3. stronger magnetic field
59
what were the canals on mars initially thought to be?
initially thought to be machine-built by martians
60
describe cratering on mars
amount of cratering varies across Mars' surface many early craters have been erased
61
describe volcanism on mars. what is its most significant volcano?
mars has many large shield volcanoes Olympus Mons is the largest volcano in solar system
62
what is a feature of Mars that is thought to have originated from tectonics?
system of valleys called Valles Marineris
63
why do we believe water likely flowed on mars at one point?
we can see dried up riverbeds in close-up photos
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