The lines indicate which atoms are in the outer layers of stars. The location of the lines is always the same when they form.
absorption lines! :)
hpiwerjpijewgpihp0fhewpdv098sdkjfnsp7u093jrfknsucgf
absorption lines due to the thin outer layer above the photosphere
There are a lot more. Each element has several possible absorption lines. In fact the element iron has several hundred lines.
If the spectrum of a star shows the same absorption lines as the sun than you know that the star has the same composition as the sun. This means that the star is made of the same elements as the sun.
absorption lines! :)
Absorption lines
By looking at its emission spectrum and seing where the black lines are
because all of the different lines of a star's elements appear together i its spectrum, making the pattern different everytime
An emission spectrum depend on electrons transition in the atom of a chemical element; and elements are different.Absorption spectrum is based on the different absorption pics of different molecules, depending on the frequency of radiation.Spectral methods are largely used in analytical chemistry.
Dark lines especially in solar spectrum have been named as Fraunhofer lines. These line are good examples for line absorption spectrum
hpiwerjpijewgpihp0fhewpdv098sdkjfnsp7u093jrfknsucgf
When white light from mercury vapour lamp is passed through sodium vapour then we have as outcome a continuous spectrum of colours with two black lines in the yellow-orange region. These two lines stand for the absorption of 5890 A and 5896 A lines of sodium atom Another example is Fraunhofer lines seen in the continuous spectrum got from sun. These lines are due to absorption of characteristic frequencies of metals present in the chromosphere of the sun
The dark lines are absorption spectrum, the energy absorbed by Atoms in the atmosphere of the star. ================================ Fraunhofer's spectral lines.
A band spectrum is an absorption or emission spectrum consisting of bands of closely-spaced lines, characteristic of polyatomic molecules.
A band spectrum is an absorption or emission spectrum consisting of bands of closely-spaced lines, characteristic of polyatomic molecules.
The absorption lines in the infrared portion of the spectrum of a star that are produced by hydrogen are from the Balmer series. The Balmer series were discovered by Johann Balmer in 1885.