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-PierceSolar 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.
das erinneret mich a's defragmentiere im windows98
also wenn ich das richtig verstande han chunnt nöd s'ganze spektrum a liecht uf de erde a wil spezielli gas uf de sunneoberfläche oder drüber die düend absorbiere? oder weiss mers immer nonig?
wie doet stoht: s'liecht wird vo gwuesse gas bi de sune absorbiert (chunnt jo noed druf a wo bi de sune).
und dass noed ali vo de streife haend neme stoff zueg'ordnet werde choene.
da sind kei spezielli gas, jedes gas bzw. jedes atömli oder molekül absorbiert irgend e frequenz, oder au e hampfle voll. ufgrund vo dene lässä bildli chasch denn ebe luege, was ime stern so dine het, und en ine kategorie stopfe. die diggä strahled z.b. energierichers liecht ab und sind drum churzwelliger, also blau, und die schmalspurige wie üsi sunne sind halt ehner gäl oder so.
