How Do Astronomers Count the Number of Stars in the Sky?

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    Counting Sky Stars
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SUMMARY

Astronomers utilize various techniques to estimate the number of stars in the sky, primarily relying on signal processing methods and observational data. While direct counting of visible stars is impractical due to intergalactic obscurations, estimates are derived from extrapolations based on deep-sky photographs and observations in different wavelengths, such as far-infrared and radio frequencies. In clearer regions like globular clusters, stellar mass averages can be inferred through spectroscopy, allowing for population estimates based on luminosity and redshift measurements.

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  • Understanding of signal processing techniques
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  • Knowledge of spectroscopy and its applications in astronomy
  • Basic concepts of redshift and its significance in distance measurement
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  • Explore the role of far-infrared and radio frequency observations in star counting
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n.karthick
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Hi
I want to know how astronomers count the number of stars (or any other celestial object for that matter) in the sky.

Will they take a photograph and do some signal processing like counting the number of brightest spots? Is it possible to count accurately since there are billions and billions of stars. Or only a rough estimate based on some equation or theory is available to do that job?

I am not related to this field but just want to know, whether there is any scope for application of signal processing techniques.
 
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Simply counting visible stars by brute force doesn't work all that well. If you look at deep-sky photographs of the night sky, you'll see that many areas of our night sky are obscured by intergalactic materials, including heavy dust clouds. It's possible to detect some stars in back of such obscurations by "looking" in the far-infrared or perhaps in radio frequencies. Still, estimates of the total number of stars in the MW are just that - estimates based on extrapolations from observations.

In bodies that are not dusty (globular clusters, for instance), one can infer stellar mass averages from spectroscopy, and estimate the stellar population from the luminosity of the body, with distances calculated from redshift measurements. There are many ways of skinning this cat.
 

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