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Title: Terrestrial Planets


1
Terrestrial Planets
  • Lecture 15
  • NATS102-13
  • 13 October 2009

2
Exam Results
Exam Results
A gt 65 B 45-65 C 35-45 D 25-35 E lt25
B
C
E
Mean 45 Median 43
Highest 89 Lowest 10
3
Problems
Good News
Almost everyone understands why the Earth has
seasons
  • Orbital velocity
  • Why does the moon have phases?
  • Retrograde motion
  • Definition of the Equinox
  • Orbital problems

4
Advice
  • Show your work. We cant give partial credit
    otherwise.
  • Make sure that your work is legible.
  • Check the units.
  • Review lectures, come to class, pay attention.
  • Pay attention to the big topics - Falling
    objects, Galileo and the phases of Venus,
    Erathosthenes and the size of the Earth,
    Discoveries with telescopes, Keplers third law,

5
The moon goes through phases each month
because a) The distance between the Earth and
moon varies throughout the month. b) The shadow
of the Earth falls on different parts of the
moon. c) The orbit of the moon is tilted with
respect to the orbit of the Earth. d) The moon
moves along its orbit and we see different
amounts of its sunlit side.
Figure from Astronomy Today by Chaisson and
McMillan
6
Jupiter orbits the Sun in a nearly circular orbit
with a semi-major axis of 5.2 AU. How fast is
Jupiter moving? Express your result in km/s to
two significant figures.
C 2?a
velocitydistance/time distance
circumferencetime period v 2?a/p p2 a3 a
5.2 AU p 11.86 years v 2?(5.2)/(11.86)
AU/year v 2.75 AU/yearv 2.75?1.5?1011/(11.86?
3.15?107)m/s v 1.3?104 m/s 13 km/s
a
7
Please Think
  • Retrograde motion occurs when
  • The Earth changes the direction of its orbit.
  • The moon changes the direction of its orbit.
  • Mars changes the direction of its orbit.
  • Mars appears to change the direction that it
    moves relative to the stars.

8
Where was I last week?
41st annual meeting of the Division for Planetary
Sciences of the American Astronomical
Society Sunday October 4 to Friday October 9,
2009 El Conquistador Resort, Fajardo, Puerto
Rico, USA
9
Results from the MeetingThe saga of Asteroid
2008 TC3
Meteorites are rocks that are believed to come
from outside of Earth - they come to Earth in a
meteor shower. There are many instances of
meteorites being found associated with the
observation of a shooting star. The parent body
of meteorites are believed to be asteroids that
collided with the Earth. 2008 TC3 is the first
asteroid detected in space that actually hit the
Earth. Astronomers photographed the asteroid in
space and predicted where it would hit the Earth.
The meteor shower was seen and meteors were
found on the ground.
10
Asteroids
Main AsteroidBelt
Near EarthAsteroids
11
News Flash Oct 6th, 2008
Looking for a little excitement tonight? An
asteroid between 1-5 meters (3-15 feet) was
discovered just hours ago at an Arizona
observatory, and might provide a spectacular
light show as it comes through Earth's
atmosphere. But don't be alarmed scientists
predict it will be harmless and burn up before it
reaches the ground. It is expected to be visible
over eastern Africa, at approximately 246 a.m.
Greenwich Mean Time (1046 p.m. Eastern time ).
There is no danger to people or property since
the asteroid will not reach the ground. It will
burn up in the upper atmosphere, well above
aircraft heights. The Universe Today
12
U of A Catalina Sky Survey
Telescopes on Mount Lemon
13
Discovery Photo
Wheres the Asteroid?
14
Particulars
  • Detected by Richard Kowalski about 20 hours
    before impact
  • About 3-5 meters in size
  • Entered atmosphere at 13 km/s (29,000 mph). This
    corresponds to an energy of 1 kiloton of TNT
  • Disrupted near 25 miles altitude

15
Image of the fireball
EUMETSAT (weather satellite) photo
16
Seen from an airliner
This confirming report comes from Jacob Kuiper
ltmailtojacobkuiper at solcon.nlgt, General
Aviation meteorologist at the National Weather
Service in the Netherlands "Half an hour before
the predicted impact of asteroid 2008 TC3, I
informed an official of Air-France-KLM at
Amsterdam airport about the possibility that
crews of their airliners in the vicinity of
impact would have a chance to see a fireball.
And it was a success! I have received
confirmation that a KLM airliner, roughly 750
nautical miles southwest of the predicted
atmospheric impact position, has observed a short
flash just before the expected impact time 0246
UTC. Because of the distance it was not a very
large phenomenon, but still a confirmation that
some bright meteor has been seen in the
predicted direction.
17
Go to website
18
Predicted Track Impact Sudan
Remember the definition of UT?
19
Contrails from the Meteor
20
Meteorite Hunters (Students) in Sudan
21
Guess which rock is the meteorite
22
More Meteorites
23
Trouble with the bus
24
Some of the pieces were rather small
25
9.2 Shaping Planetary Surfaces
  • Our goals for learning
  • What processes shape planetary surfaces?
  • Why do the terrestrial planets have different
    geological histories?
  • How do impact craters reveal a surfaces
    geological age?

26
Terrestrial Planets
  • Mercury
  • Venus
  • Earth Moon

27
What processes shape planetary surfaces?
28
Processes that Shape Surfaces
  • Impact cratering
  • Impacts by asteroids or comets
  • Volcanism
  • Eruption of molten rock onto surface
  • Tectonics
  • Disruption of a planets surface by internal
    stresses
  • Erosion
  • Surface changes made by wind, water, or ice

29
Impact Cratering
  • Most cratering happened soon after solar system
    formed
  • Craters are about 10 times wider than object that
    made them
  • Small craters greatly outnumber large ones

30
Impact Craters
Meteor Crater (Arizona)
Tycho (Moon)
31
Impact Craters on Mars
standard crater
impact into icy ground
eroded crater
32
Volcanism
  • Volcanism happens when molten rock (magma) finds
    a path through lithosphere to the surface
  • Molten rock is called lava after it reaches the
    surface

33
Lava and Volcanoes
Runny lava makes flat lava plains
Slightly thicker lava makes broad shield volcanoes
Thickest lava makes steep stratovolcanoes
34
Outgassing
  • Volcanism also releases gases from Earths
    interior into atmosphere

35
Tectonics
  • Convection of the mantle creates stresses in the
    crust called tectonic forces
  • Compression forces make mountain ranges
  • Valley can form where crust is pulled apart

36
Plate Tectonics on Earth
  • Earths continents slide around on separate
    plates of crust

37
Erosion
  • Erosion is a blanket term for weather-driven
    processes that break down or transport rock
  • Processes that cause erosion include
  • Glaciers
  • Rivers
  • Wind

38
Erosion by Water
  • Colorado River continues to carve Grand Canyon

39
Erosion by Ice
  • Glaciers carved the Yosemite Valley

40
Erosion by Wind
  • Wind wears away rock and builds up sand dunes

41
Erosional Debris
  • Erosion can create new features by depositing
    debris

42
Why do the terrestrial planets have different
geological histories?
43
Role of Planetary Size
  • Smaller worlds cool off faster and harden earlier
  • Larger worlds remain warm inside, promoting
    volcanism and tectonics
  • Larger worlds also have more erosion because
    their gravity retains an atmosphere

44
Role of Distance from Sun
  • Planets close to Sun are too hot for rain, snow,
    ice and so have less erosion
  • More difficult for hot planet to retain
    atmosphere
  • Planets far from Sun are too cold for rain,
    limiting erosion
  • Planets with liquid water have most erosion

45
Role of Rotation
  • Planets with slower rotation have less weather
    and less erosion and a weak magnetic field
  • Planets with faster rotation have more weather
    and more erosion and a stronger magnetic field

46
Thought Question
  • How does the cooling of planets and potatoes
    vary with size?
  • a) Larger makes it harder for heat from inside
    to escape
  • b) Larger has a bigger ratio of volume (which
    needs to cool) to surface area (the surface is
    where cooling happens)
  • c) Larger takes longer to cool
  • d) All of the above

47
Thought Question
  • How does the cooling of planets and potatoes
    vary with size?
  • a) Larger makes it harder for heat from inside
    to escape
  • b) Larger has a bigger ratio of volume (which
    needs to cool) to surface area (the surface is
    where cooling happens)
  • c) Larger takes longer to cool
  • d) All of the above

48
How do impact craters reveal a surfaces
geological age?
49
History of Cratering
  • Most cratering happened in first billion years
  • A surface with many craters has not changed much
    in 3 billion years

50
Cratering of Moon
  • Some areas of Moon are more heavily cratered than
    others
  • Younger regions were flooded by lava after most
    cratering

51
Cratering of Moon
Cratering map of Moons entire surface
52
9.3 Geology of the Moon and Mercury
  • What geological processes shaped our Moon?
  • What geological processes shaped Mercury?

53
What geological processes shaped our Moon?
54
Lunar Maria
  • Smooth, dark lunar maria are less heavily
    cratered than lunar highlands
  • Maria were made by flood of runny lava

55
Formation of Lunar Maria
Early surface covered with craters
Cooled lava is smoother and darker than
surroundings
Large impact crater weakens crust
Heat build-up allows lava to well up to surface
56
Tectonic Features
  • Wrinkles arise from cooling and contraction of
    lava flood

57
Geologically Dead
  • Moon is considered geologically dead because
    geological processes have virtually stopped

58
What geological processes shaped Mercury?
59
Cratering of Mercury
  • A mixture of heavily cratered and smooth regions
    like the Moon
  • Smooth regions are likely ancient lava flows

60
Cratering of Mercury
Region opposite Caloris Basin is jumbled from
seismic energy of impact
Caloris basin is largest impact crater on Mercury
61
Tectonics on Mercury
  • Long cliffs indicate that Mercury shrank early in
    its history

62
What have we learned?
  • What geological processes shaped our Moon?
  • Early cratering still present
  • Maria resulted from volcanism
  • What geological processes shaped Mercury?
  • Cratering and volcanism similar to Moon
  • Tectonic features indicate early shrinkage

63
9.4 Geology of Mars
  • How did Martians invade popular culture?
  • What are the major geological features of Mars?
  • What geological evidence tells us that water once
    flowed on Mars?

64
How did Martians invade popular culture?
65
Canals on Mars
  • Percival Lowell misinterpreted surface features
    seen in telescopic images of Mars

66
What are the major geological features of Mars?
67
Cratering on Mars
  • Amount of cratering differs greatly across
    surface
  • Many early craters have been erased

68
Volcanism on Mars
  • Mars has many large shield volcanoes
  • Olympus Mons is largest volcano in solar system

69
Tectonics on Mars
  • System of valleys known as Valles Marineris
    thought to originate from tectonics

70
What geological evidence tells us that water once
flowed on Mars?
71
Dry Riverbeds?
  • Close-up photos of Mars show what appear to be
    dried-up riverbeds

72
Ancient Riverbeds
73
Islands in the Stream
74
Erosion of Craters
  • Details of some craters suggest they were once
    filled with water

75
Martian Rocks
  • Mars rovers have found rocks that appear to have
    formed in water

76
What have we learned?
  • How did Martians invade popular culture?
  • Surface features of Mars in early telescopic
    photos were misinterpreted as canals
  • What are the major geological features of Mars?
  • Differences in cratering across surface
  • Giant shield volcanoes
  • Evidence of tectonic activity

77
What have we learned?
  • What geological evidence tells us that water once
    flowed on Mars?
  • Features that look like dry riverbeds
  • Some craters appear to be eroded
  • Rovers have found rocks that appear to have
    formed in water
  • Gullies in crater walls may indicate recent water
    flows

78
9.5 Geology of Venus
  • Our goals for learning
  • What are the major geological features of Venus?
  • Does Venus have plate tectonics?

79
What are the major geological features of Venus?
80
Radar Mapping
  • Thick atmosphere forces us to explore Venus
    surface through radar mapping

81
Cratering on Venus
  • Impact craters, but fewer than Moon, Mercury,
    Mars

82
Volcanoes on Venus
  • Many volcanoes, including both shield volcanoes
    and stratovolcanoes

83
Tectonics on Venus
  • Fractured and contorted surface indicates
    tectonic stresses

84
Erosion on Venus
  • Photos of rocks taken by lander show little
    erosion

85
Does Venus have plate tectonics?
  • Most of Earths major geological features can be
    attributed to plate tectonics, which gradually
    remakes Earths surface
  • Venus does not appear to have plate tectonics,
    but entire surface seems to have been repaved
    750 million years ago

86
What have we learned?
  • What are the major geological features of Venus?
  • Venus has cratering, volcanism, and tectonics but
    not much erosion
  • Does Venus have plate tectonics?
  • The lack of plate tectonics on Venus is a mystery

87
9.6 The Unique Geology of Earth
  • Our goals for learning
  • How do we know Earths surface is in motion?
  • How is Earths surface shaped by plate tectonics?
  • Was Earths geology destined from birth?

88
How do we know Earths surface is in motion?
89
Continental Motion
  • Motion of continents can be measured with GPS

90
Continental Motion
  • Idea of continental drift was inspired by
    puzzle-like fit of continents
  • Mantle material erupts where seafloor spreads

91
Seafloor Crust
  • Thin seafloor crust differs from thick
    continental crust
  • Dating of seafloor shows it is usually quite young

92
How is Earths surface shaped by plate tectonics?
93
Seafloor Recycling
  • Seafloor is recycled through a process known as
    subduction

94
Surface Features
  • Major geological features of North America record
    history of plate tectonics

95
Surface Features
  • Himalayas are forming from a collision between
    plates

96
Surface Features
  • Red Sea is forming where plates are pulling apart

97
Rifts, Faults, Earthquakes
  • San Andreas fault in California is a plate
    boundary
  • Motion of plates causes earthquakes

98
Plate Motions
  • Measurements of plate motions tell us past and
    future layout of continents

99
Hot Spots
  • Hawaiian islands have formed where plate is
    moving over volcanic hot spot

100
Was Earths geology destined from birth?
101
Earths Destiny
  • Many of Earths features determined by size,
    rotation, and distance from Sun
  • Reason for plate tectonics not yet clear

102
What have we learned?
  • How do we know that Earths surface is in motion?
  • Measurements of plate motion confirm idea of
    continental drift
  • How is Earths surface shaped by plate tectonics?
  • Plate tectonics responsible for subduction,
    seafloor spreading, mountains, rifts, and
    earthquakes

103
What have we learned?
  • Was Earths geology destined from birth?
  • Many of Earths features determined by size,
    distance from Sun, and rotation rate
  • Reason for plate tectonics still a mystery
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