Save'm Star's related Questions Help Pz

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Homework Help Overview

The discussion revolves around methods astronomers use to determine the composition of stars, specifically focusing on the analysis of stellar spectra and the implications of observed absorption lines. The original poster seeks clarification on these topics and expresses urgency in finding answers.

Discussion Character

  • Exploratory, Conceptual clarification, Assumption checking

Approaches and Questions Raised

  • The original poster inquires about methods beyond telescopes for determining stellar composition and questions the interpretation of spectral lines in relation to the presence of elements in stars. Other participants provide initial resources and explanations regarding continuum radiation and absorption lines.

Discussion Status

The discussion is ongoing, with participants exploring different aspects of stellar composition and spectral analysis. Some guidance has been offered regarding the nature of stellar spectra, but the original poster remains uncertain about specific detection methods and the implications of spectral observations.

Contextual Notes

The original poster expresses a need for clarity on complex concepts and appears to be navigating the constraints of homework expectations while seeking deeper understanding.

mathaTon
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Urgent HELP Star's related Questions!

Good Morning, I need help to answer these questions if anyone out there knows the answer for them, please shout or type (whatever u prefer :smile: )it a.s.a.p
what are the few methods astronomers use to today to find what stars are made of ? (other than telescope?)

if in the line spectrum, u see certain line, not the rest! is it correct to conclude the other elements are nt present in the star? why or whynot?
thanks anyhoo
 
Last edited:
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This website ought to get you started:

http://www.astro.uiuc.edu/~kaler/sow/spectra.html
 
Last edited by a moderator:
The interior of a star generally produces continuum radiation, with no visible spectral features. The absorption lines you see in stellar spectra are actually due to that continuum light passing through elements in the cooler outer layers of the star.

- Warren
 
Thankyou both, Good start for now.
 
After browsing the site, I am still unsure for the answer :
The interior of a star generally produces continuum radiation, with no visible spectral features. The absorption lines you see in stellar spectra are actually due to that continuum light passing through elements in the cooler outer layers of the star.
then how did they detected 90% hydrogen and Helium, at first place? if " "
is there any chances of them (scientists) detecting any more elements if it is not the line spectrum? (I am annoying I know, but please try to help me comprehend this, will ya?)
 

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