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The Sun

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Chapter 18 Our Star, the Sun - Strongsville City Schools ... The Sun – PowerPoint PPT presentation

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Title: The Sun


1
The Sun
2
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3
The Suns Atmosphere
4
Surface of the sun Most of the visible light
comes from this layer
Photosphere
5
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6
Granulations
  • Blotchy pattern on the photosphere caused by
    convection

7
Chromosphere
  • Dim layers of less dense gas above the
    photosphere
  • Glows red
  • Visible during a total solar eclipse
  • Temperature rises from 6000C to about 20,000C.
    due to strong magnetic fields
  • Spicules small jet like eruptions that eject
    material into the corona

8
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9
Corona
  • Seen during a total solar eclipse.
  • Also seen using a coronograph
  • Thin gas at millions of degrees
  • Parts of the corona that escape into space is
    called the solar wind.

10
The Suns Interior
11
Thermonuclear reactions in the Suns core turn
mass into energy.
At extremely high temperatures and pressures, 4
Hydrogen atoms can combine to make 1 Helium atom
and release energy by E mc2 4H ? He
energy HYDROGEN FUSION (page 283)
12
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13
Radiative Zone
  • Energy generated by nuclear fusion in the core
    moves outward as electromagnetic radiation.
  • Very Dense! It takes 170,000 years for energy
    from the core to get to the surface (50cm/hr)
    (20x slower than a snail)

14
Convective Zone
  • A region of turbulent plasma through which energy
    is transferred by convection.
  • Hot plasma rises, cools as it nears the surface,
    and falls to be heated and rise again.

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16
The Active Sun
17
SUNSPOTS
  • cooler areas within photosphere
  • caused by magnetic fields
  • occur on an 11 year cycle
  • Can last hours or several months

18
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19
  • The average sunspot is about the size of Earth,
    though the largest can be 20 times the size of
    Earth.

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21
Extreme peaks or absences of sunspots may change
Earths climate
  • Maunder Minimum 1650
  • Few sunspots
  • Colder climate
  • Famine in Europe
  • Thames froze
  • Medieval Maximum 1100
  • Many sunspots
  • Hotter climate
  • Famine in N. America
  • Ancient Pueblo people abandoned Chaco canyon
  • Icemelt permitted Vikings to reach N. America

22
The latitude at which new sunspots appear changes
throughout the sunspot cycle. Starts at 30
degrees north and south and moves toward the
equator
23
The last solar cycle
Many cycles are double peaked but this is the
first in which the second peak in sunspot number
was larger than the first. We are currently over
five years into Cycle 24. The current predicted
and observed size makes this the smallest sunspot
cycle since Cycle 14 which had a maximum of 64.2
in February of 1906.
  • Dotted lines show range of prediction solid
    curve is the average jagged lines are monthly
    counts

24
The daily movement of sunspots reveals that the
Suns rotation takes about 4 weeks.
25
Rotation
  • The sun does not rotate at the same rate
    everywhere because it is a gas (average 27 days)
  • Poles are slower than equator
  • This causes the magnetic fields to be stretched
    and solar storms develop

26
The sunspot cycle is partly due to the Suns
differential rotation. This helps solar magnetic
fields twist up, intensify, emerge, cancel, then
repeat the cycle.
  • Rotates faster at equator and slower at poles

27
Sunspots are produced by a 22-year cycle in the
Suns magnetic field.
  • Charged particles, such as electrons, will move
    along magnetic field lines.
  • The Suns positive pole is in the North for 11
    years, then switches to the South for 11 years

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29
Helioseismology.
  • Exploring the Suns interior by studying its
    vibrations.
  • Computer generated images blue moving outward,
    red moving inward

30
Astronomers probe the solar interior using the
Suns own vibrations.
Sections of the Suns surface quickly oscillate
up on down.
31
Solar Prominences
  • - Clouds of glowing gas
  • Form huge loops from one sunspot to
    another
  • Follow magnetic field lines
  • Anchored to the Sun's surface in the photosphere,
    and extend outwards into the Sun's corona.

32
Solar Flares
  • The most violent solar disturbance
  • Sudden outward eruption of plasma

33
Coronal Mass Ejection
  • Parts of the corona are thrown off the sun.
  • Can be larger than the sun.
  • Can cause a disturbance in the earths magnetic
    field

34
Visible photosphere, sunspots
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36
Ultraviolet upper chromosphere and lower corona
37
Infra-red chromosphere, sunspots are cooler and
darker
38
Microwave
39
X-Ray - corona
40
UV
Infrared
Visible
Radio
X-Ray
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