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Surface



Corona



Chromosphere

The Core

Photosphere

15,000,000 degrees c

hydrogen

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

helium

Gamma ray photons

Radiative Zone

7,000,000 - 2,000,000 degrees c

Proton

Proton

Proton

Proton

Proton

X-ray and UV photons

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

Convection Zone

3,700 degrees c

+

+

+

-

-

-

-

Plasma

The wavelength of the photon continues to decrease to visible light as they travel with the plasma of the convection zone towards the surface.

Gamma ray photons

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

7,700 degrees c

1,000,000 degrees c

2,000,000 degrees c
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Surface



Corona



Chromosphere

The Core

Photosphere

15,000,000 degrees c

hydrogen

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

helium

Gamma ray photons

Radiative Zone

7,000,000 - 2,000,000 degrees c

Proton

Proton

Proton

Proton

Proton

X-ray and UV photons

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

Convection Zone

3,700 degrees c

+

+

+

-

-

-

-

Plasma

The wavelength of the photon continues to decrease to visible light as they travel with the plasma of the convection zone towards the surface.

Gamma ray photons

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

7,700 degrees c

1,000,000 degrees c

2,000,000 degrees c
Create your own at Storyboard That

Surface



Corona



Chromosphere

The Core

Photosphere

15,000,000 degrees c

hydrogen

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

helium

Gamma ray photons

Radiative Zone

7,000,000 - 2,000,000 degrees c

Proton

Proton

Proton

Proton

Proton

X-ray and UV photons

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

Convection Zone

3,700 degrees c

+

+

+

-

-

-

-

Plasma

The wavelength of the photon continues to decrease to visible light as they travel with the plasma of the convection zone towards the surface.

Gamma ray photons

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

7,700 degrees c

1,000,000 degrees c

2,000,000 degrees c
Create your own at Storyboard That

Surface



Corona



Chromosphere

The Core

Photosphere

15,000,000 degrees c

hydrogen

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

helium

Gamma ray photons

Radiative Zone

7,000,000 - 2,000,000 degrees c

Proton

Proton

Proton

Proton

Proton

X-ray and UV photons

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

Convection Zone

3,700 degrees c

+

+

+

-

-

-

-

Plasma

The wavelength of the photon continues to decrease to visible light as they travel with the plasma of the convection zone towards the surface.

Gamma ray photons

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

7,700 degrees c

1,000,000 degrees c

2,000,000 degrees c
Create your own at Storyboard That

Surface



Corona



Chromosphere

The Core

Photosphere

15,000,000 degrees c

hydrogen

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

helium

Gamma ray photons

Radiative Zone

7,000,000 - 2,000,000 degrees c

Proton

Proton

Proton

Proton

Proton

X-ray and UV photons

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

Convection Zone

3,700 degrees c

+

+

+

-

-

-

-

Plasma

The wavelength of the photon continues to decrease to visible light as they travel with the plasma of the convection zone towards the surface.

Gamma ray photons

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

7,700 degrees c

1,000,000 degrees c

2,000,000 degrees c
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Storyboard Text

  • 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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