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it means it just diesnt

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Q: What does it mean when a star has no hydrogen lines in its spectrum?
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What happens when a star burns up all of its hydrogen?

When a star burns up all of its hydrogen,it becomes red in color.As hydrogen is the fuel for star and it will burst after it.


Why does the amount of hydrogen in a star decrease?

Because Hydrogen is the fuel of Stars, hydrogen consumed and Helium is formed.


Suppose you want to know the chemical composition of a distant star Which piece of information is most useful to you?

A telescope, whose light output would be sent through a spectral analysis machine of some type. That analysis of the emission spectra of the star would be compared to the known spectra of the elements to find the composition of the star.


What are the two main elements in a star?


If a star becomes a red gaint when all its hydrogen is used up and later becomes a nebula How can a nebula star form without hydrogen?

The key to this is that NO star uses up ALL of its hydrogen. In fact, they only use up the Hydrogen in their cores, where pressure and temperature are highest. In the case of a red giant, the star is at the stage of burning Helium into Beryllium, Boron and Carbon, which requires much more heat (the heat is "borrowed" from the previous collapsing of the star at the end of the main sequence phase) and continues with a much denser core. When a star expands into a red giant, it blows some of its Hydrogen mass into space. Later, when it simply cannot sustain any fusion reactions in its core, it still contains a considerable amount of hydrogen in the outermost layers, and the subsequent collapse causes a rebound (supernova) that blows about 50% of the original star's mass - most of the hydrogen plus some of the heavier elements into space. When that blown away material collides with a large gas cloud in space which is mostly hydrogen, and compresses that cloud enough that the material can then collapse and form another new star.

Related questions

What are the absorption lines in the infrared portion of the spectrum of a star that are produced by hyrdrogen are from?

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.


What part of the star is responsible for the dark lines in its spectrum?

Atoms in the atmosphere of the star is responsible for the dark lines in its spectrum.


The composition of a star can be identified by?

the lines in its spectrum


Why can elements in a star be separated?

Because the spectrum of the star's light can be seen to have dark lines all the way through, and each element has its own set of dark lines in the star's spectrum.


What is the continuous spectrum of a star?

A continous spectrum hasn't discrete gaps between lines.


What are the Dark lines that appear in a spectrum of light from a star called?

absorption lines! :)


How are absorption and emission lines produced in a stellar spectrum What information might absorption lines in the spectrum of a star reveal about a cloud of cool gas lying between us and the star?

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How do scientists determine the elements in a star since they cannot collect a sample from a star?

They analyze the star's spectrum. Each element produces characteristic lines in a spectrum.


What are dark lines in a stellar spectrum called?

The dark lines are absorption spectrum, the energy absorbed by Atoms in the atmosphere of the star. ================================ Fraunhofer's spectral lines.


What can be said about the star composition if the spectrum of a star shows the same absorption lines as the sun?

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.


If a star is moving away from you the absorption lines in its spectrum will?

If a star is moving away from you, the emission lines in its spectrum will be shiftedtoward longer wavelengths/lower frequency/the red end of the spectrum, since theyoriginate on the star itself.But there's no effect on the absorption lines, because those are caused by materialthat's unrelated to the star, and just happens to be in the line of sight between thestar and you.


The spectrum of a star is called a what?

... a photonic 'fingerprint'. The picture of a star's spectral lines is its photo-spectrograph.