APOD: 2005 February 27 - The Solar Spectrum
Astronomy Picture of the Day
Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
2005 February 27
The Solar Spectrum
Credit & Copyright: Nigel Sharp (NSF), FTS, NSO, KPNO, AURA, NSF
Explanation: It is still not known why the Sun's light is missing some colors.
Shown above are all the visible colors of the
Sun, produced by passing the Sun's light through a prism-like device.
The above spectrum was created at the McMath-Pierce Solar Observatory and shows, first off, that although our yellow-appearing Sun emits light of nearly every color, it does indeed appear brightest in yellow-green light.
The dark patches in the
above spectrum arise from gas at or above the Sun's surface absorbing sunlight emitted below.
Since different types of gas absorb different colors of light, it is possible to determine what gasses compose the Sun.
Helium, for example, was first discovered in 1870 on a solar spectrum and only later found here on Earth.
Today, the majority of
spectral absorption lines have been identified - but not all.
Tomorrow's picture: plates unknown