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The Home World: EARTH

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Title: The Home World: EARTH


1
The Home WorldEARTH
a 1 AU
P 365 d
i (orb) 0o
e 0.017
Prot 1 d
i (rot) 23.5o
R 6378 km
M 6.0 x 1024 kg
r 5.5 g/cc
g 9.8 m/s2
vesc 11 km/s
A 0.37
2
Near-Earth Space The Van Allen Belts
3
Nature of the Belts
  • Discovered early in the space age with a Geiger
    counter.
  • Energetic charged particles are trapped in the
    Earths magnetic field.
  • The inner belt contains protons, and the outer
    contains electrons.
  • The inner belt begins at only 100 km or so above
    ground.

4
Aurorae
5
Space Aurora
6
Aurora Borealis from Yellowknife in Canada
7
Aurorae
  • Solar wind particles are generally repelled by
    the magnetosphere, but some sneak into the
    atmosphere by running along magnetic field lines
    toward the poles. (Outer van Allen belt)
  • Earth atmospheric particles sneak into the belts
    as well. (Inner van Allen belt)
  • At 100km altitude, solar wind particles collide
    with atmosphere particles to produce an auroral
    light display.

8
Comparison of Planetary Magnetic Fields
Equatorial Field (Gauss)
Mercury 0.002
Venus lt0.0003
Earth 0.305
Mars (0.0004)
Jupiter 4.2
Saturn 0.20
Uranus 0.23
Neptune 0.06-1.2
9
The space around the Earth is not exactly
crowded, but there is a great deal of space
debris in orbit around Earth.
Space Debris
10
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11
The Kessler Syndrome
12
The Earth at Night (issues of light pollution)
13
Atmosphere Appearance of the Sky
14
Understanding Sky Color
15
Sky Color from Two Places
16
Structure of the Earths Atmosphere
17
Atmosphere Ozone Layer Component
18
Antarctic Ozone Hole
19
Ozone Destruction
  • Ozone molecule O3
  • O3 protects use from harmful solar UV radiation
  • An efficient O3 destruction mechanism involves
    chlorofluorocarbons (CFCs Cl, F, C)
  • ltchemistrygt
  • A single Cl atom can be used 1000s of times to
    break up ozone molecules!

Catalyst process
20
Ozone Trends
South Pole
North Pole
21
Atmosphere and Surface Energy Budget of the
Earth
22
Global Warming Trends and Effects
  • The overall topic of global warming is
    complicated.
  • Increased greenhouse gases (carbon dioxide,
    methane, etc)
  • act like a blanket to block the escape of
    infrared heat light.
  • The Earth has also undergone cycles in the past.
  • The main concern is the impact and control of
    warming trends.

23
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24
Share Question
  • The previous figure displayed information about
    sea ice area.
  • Is area the best measure for the amount of
    ice?
  • If so, why?
  • If not, what would be better? And, why?

25
Climate Considerations
26
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27
Weather
  • Primarily driven by solar radiation.
  • Other significant influences include
  • Land mass and oceans
  • Planet rotation
  • Atmospheric composition
  • Ozone
  • Greenhouse effect
  • Volcanic activity

28
The Hadley Cell Fundamental circulation pattern
because of the fact that planets are round.
29
Coriolis Deflection Planet rotation causes
north-south weather circulation to deflect
east-west.
30
The Coriolis Force
31
Hadley Cells on the Earth
32
Volcanoes and Resurfacing
  • Magma is less dense than rock, and so rises from
    the interior
  • This breaks through, giving a volcano
  • Products
  • New rocks (esp. basalts)
  • Ash ( 1mm )
  • Cinders ( 1cm )
  • The key point is that volcanoes lead to
    resurfacing and are evidence of an active
    planetary interior

33
Mount St. Helens
34
Tungurahua (Andes)
35
Rock Types
  • Igneous (ignusfire) - form from
    crystallization of molten rock
  • Magma - molten inside earth
  • Lava - molten on surface
  • Of planetary interest
  • Basalt - fast cooling
  • Granite - slow cooling
  • Sedimentary - formed by deposition of small
    particles which become cemented (e.g., sandstone,
    shales)
  • Metamorphic - changed by heat, pressure, and/or
    chemistry (e.g., marble)

36
Crustal Plates and Tectonic Activity
  • Earths surface (or crust) is not a single solid
    piece, but consists of large and small plates
  • These plates slowly drift around
  • At points of convergence, get volcanoes, mountain
    ranges, and earthquakes

37
Crustal Plates
38
Long Term Plate Drifting
39
Plate Motion
40
Volcanic Activity on Earth and Relation to Motion
of Plates
41
Recycling process and resurfacing effects
42
Interior Structure of the Earth
43
Detail of Earth Interior
44
Share Question
  • Earthquakes are an important tool for scientists
    because their vibrations
  • a) influence the Earth's orbit about the Sun
  • b) allow the study of the Earth's internal
    structure
  • c) inform us of the mass of the Earth
  • d) are used to predict the future of plate
    tectonics

45
Seismology
  • Study of the Earths interior from how it carries
    vibrations
  • Types of vibrations
  • P-waves pressure waves that travel like sound
  • S-waves shear waves, like on a rope
  • Terminology
  • Focus point at which the earthquake originates
  • Epicenter surface point above the focus
  • Seismometer a device to measure P S waves and
    the strength of earthquakes

46
Earthquake
47
Wave Forms
48
Refraction of traveling sound waves in the Earth
reveals its components
49
Shuddering of the Earth
50
Earths Magnetic Field
  • Lines of force are somewhat like a bar magnet.
  • Its origin and maintenance comes from dynamo
    activity in the core
  • Circulation of conducting fluid (e.g., molten
    metals) generates magnetic fields.
  • So, planetary magnetic fields act like probes of
    unseen planetary interiors

51
Earth Dynamo
52
Share Question
  • The Earth's magnetic dynamo is caused by a
    combination of convection in its molten core and
  • a) the Earth's orbit around the Sun
  • b) the Earth's rotation
  • c) lunar tidal action
  • d) the aurora borealis
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