Composition of the sun and spectrum of light

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SUMMARY

The sun's composition consists of 91% hydrogen, 8.7% helium, and 0.3% other elements. While hydrogen and helium primarily contribute to the atomic spectrum, the remaining 0.3% of elements plays a minimal role in the overall visible spectrum of sunlight. The sun behaves as a radiating black body, producing a continuous spectrum due to thermal equilibrium among photons, electrons, and nuclei in the solar plasma. Although there are absorption and emission lines present, they only slightly alter the blackbody spectrum, which is predominantly determined by the sun's temperature.

PREREQUISITES
  • Understanding of blackbody radiation principles
  • Familiarity with atomic spectra of hydrogen and helium
  • Knowledge of thermal equilibrium in plasma physics
  • Basic concepts of nuclear fusion processes
NEXT STEPS
  • Research the principles of blackbody radiation and its applications
  • Study the atomic spectra of various elements beyond hydrogen and helium
  • Explore the processes of nuclear fusion in stars, particularly in the sun
  • Investigate the effects of solar plasma on light emission and absorption
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Astronomers, physicists, students of astrophysics, and anyone interested in the composition of stars and the nature of light.

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I understand that the sun is made of 91% hydrogen, 8.7% Helium, and 0.3% other stuff. I looked up the atomic spectrum for helium and hydrogen [within the visible portion] and they leave most of the spectrum blank, albeit few lines of colour here and there, yet the white light that reaches us has a full (?) spectrum. Is that 0.3% of the sun responsible for the rest of the colours in white light? How complete is the white light that reaches us? There must be some shades or tones we never see.

Am I wrong in thinking of the sun as a radiating black body? I know that there are nuclear as well as thermal processes occurring, is the fission/fusion responsible for the rest of the visible spectrum?
 
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To a good approximation, the sun does radiate as a blackbody. Blackbody radiation is a continuous spectrum, and does not depend on the materials that the radiating body is made from. This is because repeated collisions between photons, electrons, nuclei, and neutral atoms in the solar plasma lead to photons which are in thermal equilibrium. Photons which are in thermal equilibrium lead to a continuous blackbody spectrum, which is only a function of temperature. There are absorption and emission lines in the sun's spectrum due to the atoms in the sun, but they cause only a relatively small deviation from the blackbody spectrum
 

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