Largest Known Star: Introducing Myself and Cosmology

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SUMMARY

The discussion centers on the methods used to estimate the size of stars, particularly focusing on Betelgeuse as the largest known star that can be resolved. It highlights that direct measurements of star sizes are not possible with current telescopes, and instead, astronomers rely on techniques such as interferometry and color temperature analysis. The conversation emphasizes the importance of understanding the limitations of star images and the theoretical frameworks that allow for size estimation based on temperature and luminosity relations.

PREREQUISITES
  • Understanding of interferometry in astronomy
  • Knowledge of color temperature and its relation to star classification
  • Familiarity with luminosity and size relations in astrophysics
  • Basic concepts of spectroscopy and its application in determining star properties
NEXT STEPS
  • Research the principles of optical interferometry in astronomy
  • Learn about the Hertzsprung-Russell diagram and its implications for star classification
  • Explore the methods for measuring stellar temperatures and their significance
  • Investigate the concept of eclipsing binaries and their role in direct size measurement of stars
USEFUL FOR

Astronomy enthusiasts, astrophysics students, and anyone interested in understanding stellar measurements and the limitations of astronomical imaging techniques.

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This is the first time I am posting here. I thought I whould show this website as a way to introduce myself. I'm interested in anything dealing with science, especially cosmology. I have always liked showing this website to everyone because it really shows how small we are.

http://www.techdo.com/images/largest-know-star.htm
 
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Do you know how you measure a stars size which you can't resolve in telescopes? The largets know star that can be resolved is Betelgeuse (as far as I remember)
 
It's important to note that all of the 'images' of the stars that are not the Sun in that slide show are not actual telescope images (apart from the Eta Carina nebula that is actually much bigger than that slide show suggests?). They look like either drawings or re-coloured images of the Sun to give an idea of what that star might look like. We cannot resolve any star other than the Sun with a single telescope (even the biggest and best we have) although we can get some information about sizes using interferometry with multiple optical telescopes. These techniques still don't give you the kind of detail implied in that slide show. Not being critical of it, it's quite cool, but just bear that in mind since it isn't clear from the images alone.

What is normally done to estimate the size of a star is to measure its temperature by measuring its colour (blue is hotter than yellow which is hotter than red). We then have theories that tell us based on the colour and type of star (which we can determine by other aspects of the spectrum) how big the Star must be. These theories have been checked and calibrated on stars where we can measure the size directly, either through eclipsing binaries or optical interferometry (google or ask for more info on any confusing or new terms!) so we have some confidence that they work for stars were we can't get such direct information.
 
I have done quite much astrophysics, but that was a time ago..

I know that the pictures in that perticular slide was'nt real ones, and I know of the temperatur-luminosity-size relations.

Maybe my question was not specific enough:-)

But you shed some light on how we can measure stars size directly, thanx!
 

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