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24.3 The Sun

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Chromosphere is observable during a total solar eclipse. Chromosphere. Corona ... only during an eclipse when the bright photosphere ... result of solar flare ... – PowerPoint PPT presentation

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Title: 24.3 The Sun


1
24.3 The Sun
2
Hot facts
  • Sun ball of GAS (not fire!)
  • 99.9 of all matter of our Solar System is in the
    sun
  • The sun is an average star
  • It is a Main-Sequence star (well learn about
    later)
  • One of 100 billion stars that make up the Milky
    Way Galaxy
  • The only star whose surface we can study

3
The Active Sun
  • Not all parts of the sun rotate at the same speed
  • Equator rotates once in 25 days (faster)
  • Poles rotate once every 33 days (slower)
  • Conclusion the sun is gaseous

4
Structure of the Sun
  • Made of gas, no sharp boundaries exist between
    its internal layers
  • The sun is divided into four parts
  • Solar Interior
  • Photosphere (visible surface)
  • Chromosphere (layer of its atmosphere)
  • Corona (layer of its atmosphere)

5
Photosphere
  • Meaning photos light, sphere ball
  • Visible surface of the sun
  • Radiates energy to space
  • Has a grainy texture made of bright markings
    called granules produced by convection.
  • Temp averages approx 10,000ºF
  • 90 of the suns surface atoms are hydrogen

6
Chromosphere
  • The first layer of the solar atmosphere found
    directly above the photosphere.
  • - chroma color sphere
  • Relatively thin, hot layer of incandescent gases
    a few thousand miles thick.
  • Its top contains numerous spicules, which are
    narrow jets of rising material.
  • Chromosphere is observable during a total solar
    eclipse

7
Chromosphere
8
Corona
  • Meaning corona crown
  • Outermost layer of the solar atmosphere.
  • Visible only during an eclipse when the bright
    photosphere is covered
  • The temp at the top of the corona exceeds 2
    million degrees F.

9
  • Solar wind - stream of protons and electrons
    erupted at high speed from the solar corona
  • Interacts with bodies of the solar system
  • Earths magnetic field prevents
  • solar wind from reaching our surface

10
Sun Spots
  • Dark spots on the sun, they are cool in
    contrast to the surrounding photosphere.
  • Sunspots appear dark because of their
    temperature, which is about 2000 degrees less
    than that of the surrounding solar surface.
  • Some history During early nineteenth century it
    was believed a tiny planet named Vulcan orbited
    between Mercury and the Sun. It turned out the
    planet Vulcan was actually a series of sun spots!
    oops

11
Sun Spots
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Prominences
  • Meaning prominere to jut out
  • Huge cloudlike structures consisting of
    chromospheric gases.
  • Appear as arches
  • May seem to hang motionless for days or may be
    explosive
  • Prominences are ionized gases trapped by
    magnetic fields that extend from regions of
    intense solar activity.

15
Prominences
16
Solar Flares
  • Brief outbursts that normally last about an
    hour and appear as a sudden brightening of the
    region above a sunspot cluster.
  • Solar flares release enormous amounts of energy,
    much of it in the form of ultraviolet, radio, and
    X-ray radiation.
  • Auroras (Northern or Southern Lights)
  • result of solar flare
  • bright displays of light caused by solar
    radiation interacting with Earths upper
    atmosphere near the poles

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Nuclear Fusion
  • The way that the sun produces energy.
  • In this reaction four hydrogen nuclei combine to
    form one helium nucleus, releasing a tremendous
    amount of energy.

24
Nuclear Fusion
  • The sun has enough fuel to exist in its present
    stable state for 10 billion years.
  • The sun is already 4.5 billion years old, so it
    is middle-aged
  • When the sun does come to its final stages, it
    will expand and engulf the first 4 planets

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