Origin Of Light
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- Written by:
- Karen Fox
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- Scientific consulting by:
- Holly Gilbert
- View full credits
An elegant interaction powers the sun, producing the light and energy that makes life possible. That interaction is called fusion, and it naturally occurs when two atoms are heated and compressed so intensely that their nuclei merge into a new element. This process often leads to the creation of a photon, the particles of light that are released from the sun. However, before exiting our star, each photon must first undergo a long journey. Over the course of 40,000 years it will be absorbed by other atoms and emitted repeatedly until reaching the sun's surface. Once there, the photons stream out, illuminating Earth, the solar system and beyond. The number released from the surface every second is so vast that it is more than a billion billion times greater than the number of grains of sand on our planet. Watch the animation to see how atoms deep inside the sun's core melt together and generate light.
Credits
Please give credit for this item to:
Conceptual Image Lab, NASA's Goddard Space Flight Center
Earth photo courtesy of NASA/ISS Expedition 13 crew
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Animators
- Michael Lentz (KBR Wyle Services, LLC)
- Walt Feimer (KBR Wyle Services, LLC)
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Writer
- Karen Fox (ADNET Systems, Inc.) [Lead]
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Video editor
- Genna Duberstein (ADNET Systems, Inc.)
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Scientist
- Holly Gilbert (NASA/GSFC) [Lead]
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Producer
- Walt Feimer (KBR Wyle Services, LLC)