The Sun By Mrs. Allen
I.  Layers of the Sun The Core:  The center of the sun where fusion takes place. Radiation zone:  energy flows from core. Convection zone:  energy circles back toward core and is then pushed back out by energy coming from radiation zone.
I.  Layers of the Sun Photosphere:  The layer from which light is given off. Chromosphere:  The layer that extends above the photosphere. Corona:  Largest layer of the suns atmosphere and extends millions of km.
II.  Parts of the Sun Sunspots:  Cool areas around the sun which are not permanent. 1.  Caused by Magnetic Fields. 2.  High numbers occur every 11 years. 3.  Occur in pairs. 4.  When 2 sunspots come together, prominences and flares are produced.
II.  Parts of the Sun Prominences:  Huge arching columns of gas. Flares:  Violent eruptions shooting outward from the sun at high speeds.
III.  Characteristics of the Sun 99% of all the matter in our solar system is in the sun. The sun is the center of the solar system. The sun is a main-sequence star.  The sun produces energy by fusion. 75% Hydrogen and 25% Helium fuse in the core. Fusing means two atoms combine to form a heavier atom.
IV.  Interesting Facts The sun is a G2 star. The temperature of the core is 15.6 million Kelvin. The sun is approximately 4.5 billion years old. The sun emits a low-density stream of charged particles known as the solar wind. Our sun is unique, not part of a binary system, 2 stars orbiting each other.
 

The Sun

  • 1.
    The Sun ByMrs. Allen
  • 2.
    I. Layersof the Sun The Core: The center of the sun where fusion takes place. Radiation zone: energy flows from core. Convection zone: energy circles back toward core and is then pushed back out by energy coming from radiation zone.
  • 3.
    I. Layersof the Sun Photosphere: The layer from which light is given off. Chromosphere: The layer that extends above the photosphere. Corona: Largest layer of the suns atmosphere and extends millions of km.
  • 4.
    II. Partsof the Sun Sunspots: Cool areas around the sun which are not permanent. 1. Caused by Magnetic Fields. 2. High numbers occur every 11 years. 3. Occur in pairs. 4. When 2 sunspots come together, prominences and flares are produced.
  • 5.
    II. Partsof the Sun Prominences: Huge arching columns of gas. Flares: Violent eruptions shooting outward from the sun at high speeds.
  • 6.
    III. Characteristicsof the Sun 99% of all the matter in our solar system is in the sun. The sun is the center of the solar system. The sun is a main-sequence star. The sun produces energy by fusion. 75% Hydrogen and 25% Helium fuse in the core. Fusing means two atoms combine to form a heavier atom.
  • 7.
    IV. InterestingFacts The sun is a G2 star. The temperature of the core is 15.6 million Kelvin. The sun is approximately 4.5 billion years old. The sun emits a low-density stream of charged particles known as the solar wind. Our sun is unique, not part of a binary system, 2 stars orbiting each other.
  • 8.