The Absorption Line Spectra For Six Hypothetical Stars Each With Different Temperatures Are Shown Below For Each Abso 1 (34.7 KiB) Viewed 40 times
Do cold stars always appear to have a different (greater or fewer) number of lines intheir absorption spectra than hot stars? Cite evidence from the above spectra to supportyour answer.2) Do cold stars always appear to have more lines at either the blue or red ends of theirabsorption spectra than hot stars? Cite evidence from the above spectra to support youranswer.3) Consider the absorption line spectrum given below for Star G. Can you determine theapproximate temperature for Star G by comparing its absorption line spectrum to theabsorption line spectra and temperatures of Stars A-F given above? If so, write in your estimate in the space below. if not explain why
Do cold stars always appear to have a different (greater or fewer) number of lines in
their absorption spectra than hot stars? Cite evidence from the above spectra to support
your answer.
2) Do cold stars always appear to have more lines at either the blue or red ends of their
absorption spectra than hot stars? Cite evidence from the above spectra to support your
answer.
3) Consider the absorption line spectrum given below for Star G. Can you determine the
approximate temperature for Star G by comparing its absorption line spectrum to the
absorption line spectra and temperatures of Stars A-F given above? If so, write in your estimate in the space below. if not explain why
The Absorption Line Spectra For Six Hypothetical Stars Each With Different Temperatures Are Shown Below For Each Abso 2 (63.73 KiB) Viewed 40 times
The absorption line spectra for six hypothetical stars, each with different temperatures, are shown below. For each absorption line spectrum, the short wavelengths of light (or blue end) of the electromagnetic spectrum are shown on the left side, and the long wavelengths of light (or red end) of the spectrum are shown on the right side.
Indiame Twropurs for Nomeourrorr As? Taure
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