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Sun and Moon

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Sun and Moon * * * * * * * * * * * The Sun is . A star In the Main Sequence stage 99% of the total mass in the solar system 109 times as big as the Earth Energy ... – PowerPoint PPT presentation

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Title: Sun and Moon


1
Sun and Moon
2
The Sun is.
  • A star
  • In the Main Sequence stage
  • 99 of the total mass in the solar system
  • 109 times as big as the Earth

3
Energy Production in the Sun
  • Nuclear fusion occurs in the sun to give it its
    energy.
  • Hydrogen is converted into Helium.

4
Structure of the Sun
  • The sun does not have a solid surface. The
    visible surface is where its atmosphere becomes
    so thick that you cant see through it.
  • The sun is divided into 6 layers.

5
Layers of the sun
6
Layers of the Sun
  • Corona- Outermost part of the suns atmosphere.
    Visible only during a solar eclipse
  • Chromosphere- section of the suns atmosphere
    below the corona.
  • Photosphere- the visible part of the suns
    atmosphere. The surface we see.
  • Convective Zone- Section where convection
    currents carry energy to the outer atmosphere of
    the sun

7
Layers of the Sun Continued...
  • Radiative Zone- Very dense section of the sun
    where energy is trapped.
  • Core- inner part of the sun where the suns
    energy is produced by nuclear fusion.

What Layer is shown here? Hint Solar Eclipse
8
Solar Activity
  • The circulation of energy causes gas in the
    photosphere to churn, causing magnetic fields
    that reach into space.
  • Sunspots- when the activity slows down in one
    spot, and the photosphere becomes cooler than
    other areas. Sunspots are cooler, dark spots on
    the sun.
  • Sunspots change in a regular pattern. About
    every 11 years there is a peak in sunspots. They
    might affect our climate and cause lower
    temperatures on earth.

9
Sunspots
10
Solar Activity continued...
  • Solar Flares- regions of extremely high
    temperatures and brightness that develop on the
    suns surface. When they erupt, they send
    streams of electrically charged particles into
    the solar system.
  • They can extend several thousand miles into space
    within minutes.
  • Particles from solar flares reach earth and
    interrupt radio and cell signals.

11
Solar Flare
12
Aurora BorealisNorthern Lights
  • When solar particles enter our atmosphere, they
    are attracted to the poles, and cause Aurora
    Borealis

13
Formation of the Moon
  • Three explanations for how the moon could have
    formed
  • Twin Theory
  • Meteor Theory
  • Capture Theory

14
Twin Theory
  • The moon formed at the same time as Earth.
  • Gravity pulled particles in the solar system
    together to make the earth and the moon out of a
    nebula

15
Meteor Theory
  • When Earth was first cooling, a meteor struck it
    and splashed a piece off which hardened to form
    the moon.

16
Capture Theory
  • The Moon formed someplace else, it flew by Earth
    and gravity captured it into orbit.

17
Features of the Moon
  • Maria- smooth dark plains on the moon
  • Highlands- rugged mountains on the moon that
    appear as light places.

18
Features of the Moon
  • Rilles- lines on the moon where the crust of the
    moon cracked when it cooled.
  • Craters- round impacts from meteors

19
Why are there so many craters on the moon?
  • The moon has no ATMOSPHERE, so it has no WEATHER,
    so there is no EROSION.
  • Therefore, when the moon gets struck by a meteor,
    the crater stays there forever.

20
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21
Label each section 1- 9
22
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