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  • The Core
  • hydrogen
  • helium
  • hydrogen
  • In the core of the sun, hydrogen atoms are forced together in nuclear fusion. This union creates helium, and releases highly energized photons in the form of gamma rays
  • 15,000,000 degrees c
  • Gamma ray photons
  • Radiative Zone
  • Proton
  • The photon slowly makes its way through the densely packed protons of the radiative zone. It takes anywhere from a few thousand to a few million years to escape. The photon loses energy from this travel, and becomes X-rays, then UV light
  • Proton
  • Gamma ray photons
  • 7,000,000 - 2,000,000 degrees c
  • Proton
  • Proton
  • X-ray and UV photons
  • Proton
  • Surface
  • -
  • Millions of years after its creation, the photon travels through the photosphere, chromosphere, and finally the corona. 93,000,000 miles and around 8 minutes later, it reaches earth's surface
  • Photosphere
  • -
  • Plasma
  • Chromosphere
  • +
  • 7,700 degrees c
  • Corona
  • +
  • -
  • 2,000,000 degrees c
  • +
  • -
  • The wavelength of the photon continues to decrease to visible light as they travel with the plasma of the convection zone towards the surface.
  • Convection Zone
  • 3,700 degrees c
  • 1,000,000 degrees c
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