Most interstellar gas is at a lower temperature than that of stellar atmospheres and the density of interstellar gas is less than that of stellar atmospheres.
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The dark lines are absorption spectrum, the energy absorbed by Atoms in the atmosphere of the star. ================================ Fraunhofer's spectral lines.
Absorption lines
The lines will not move.
The density or pressure of this gas is much lower than can be produced in a laboratory.
Need a different, better answer.
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The dark lines are absorption spectrum, the energy absorbed by Atoms in the atmosphere of the star. ================================ Fraunhofer's spectral lines.
There is one way for gathering information about chemical composition of stellar objects - spectral analysis! Astronomical spectroscopy began with Isaac Newton's initial observations of the light of the Sun, dispersed by a prism. He saw a rainbow of colour, and may have seen absorption lines. The absorption lines in stellar spectra can be used to determine the chemical composition of the star.
Absorption lines
absorption lines! :)
There are a lot more. Each element has several possible absorption lines. In fact the element iron has several hundred lines.
The lines will not move.
On the earth (and planetary/stellar bodies) they are called latitudes and longitudes.
The density or pressure of this gas is much lower than can be produced in a laboratory.
No. Those would be absorption lines.