How Do Astronomers Accurately Count Stars in the Universe?

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Discussion Overview

The discussion revolves around the methods astronomers use to estimate the number of stars in galaxies, including the implications of dark matter and the relationship between a galaxy's mass and its star count. Participants explore various estimation techniques, the role of rotation speeds, and the impact of non-stellar matter in these calculations.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants propose that star counts in galaxies are estimates based on average number density and volume.
  • Others suggest that the mass of a galaxy can be estimated from its rotation speed, which is measured using Doppler effects.
  • A participant questions whether the estimates of star counts consider the presence of dark matter, noting that estimates can change over time.
  • It is mentioned that the average mass of stars in the Milky Way is believed to be around 1/2 solar mass, but this is not universally accepted.
  • One participant discusses how the mass of the Milky Way is estimated to be around 1 trillion solar masses, with only a fraction attributed to stars, suggesting that dark matter constitutes a significant portion of the galaxy's mass.
  • Concerns are raised about how non-stellar components, such as gas clouds and nebulae, are factored into star count estimates.

Areas of Agreement / Disagreement

Participants express various viewpoints on the methods of estimating star counts and the influence of dark matter, indicating that multiple competing views remain and the discussion is unresolved.

Contextual Notes

Participants acknowledge that estimates of star counts and galaxy mass are subject to change and depend on the methods and assumptions used, particularly regarding dark matter and the average mass of stars.

ShadowKnight
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I was looking at some maps of the known universe (http://www.anzwers.org/free/universe/) and a question occurred to me - how can astronomers say how many stars are in a certain galaxy? What method is being used to count them? Is it direct observation or is it some kind of formula?
 
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Originally posted by ShadowKnight
I was looking at some maps of the known universe (http://www.anzwers.org/free/universe/) and a question occurred to me - how can astronomers say how many stars are in a certain galaxy? What method is being used to count them? Is it direct observation or is it some kind of formula?
It's an estimate based on the average number density and volume.

- Warren
 
So for example, in some far off area where astronomers are estimating there are 1 million stars in a cluster, it very well could be a few massive stars?
 


Originally posted by chroot
It's an estimate based on the average number density and volume.

- Warren

this is a pretty interesting question

the MASS of a galaxy can be estimated by its speed of rotation
which can be told by doppler
at various distances from center

there is a kind of rotation speed curve that plots speed of rotation compared with distance out

the mass can be told from this rotation curve

and the mass is related to the number of stars
but the relationship is not a completely simple one because of the
existence of dark matter

a few years back an astronomer told me that it was believed that the average mass of star in Milkyway was 1/2 solar mass. That may be true or it may not be----estimates change.

If Milky mass is 1 trillion solar (told from rotation speeds) and if there is no dark matter (untrue!) and if the average star is 1/2 solar-----then Milky has 2 trillion stars.

But those numbers are just "for example let's say" type numbers.

I think its interesting and could be basis of some more discussion.

Warren (chroot) teaches astro, I believe, so he may have quite a bit more to say about this.
 
OK, that makes sense to me. So I wonder if astronomers take any dark matter into consideration when they make their estimates. I've heard compelling evidence that it exists (though unproven?) On one map of the galaxy (http://www.anzwers.org/free/universe/milkyway.html) it shows this data in a table:

Number of stars in the Galaxy: 200 billion
Mass of the Galaxy: 1 trillion solar masses

Ignoring any dark matter this would mean that they came up with an average of 5 solar masses per star. How do gas clouds and nebula and other non-stars in the galaxy get figured into this?
 
Originally posted by ShadowKnight
OK, that makes sense to me. So I wonder if astronomers take any dark matter into consideration when they make their estimates. I've heard compelling evidence that it exists (though unproven?) On one map of the galaxy (http://www.anzwers.org/free/universe/milkyway.html) it shows this data in a table:

Number of stars in the Galaxy: 200 billion
Mass of the Galaxy: 1 trillion solar masses

Ignoring any dark matter this would mean that they came up with an average of 5 solar masses per star. How do gas clouds and nebula and other non-stars in the galaxy get figured into this?

tho not an expert I will tell you how I understand those numbers

I feel very sure that astronmers have seen enough stars they have come to the conclusion the average one is 1/2 solar mass

so the guy with the numbers is telling you that Milky is LOADED with dark matter

he measures it at 1 trillion solar (which is in line with many estimates I have seen over the past 10 years, it is not a bad figure based on rotation speeds which can be measured by radioastronomy of neutral hydrogen even in parts of Milky which we cannot see optically)

But he says that of the 1 trillion solar masses only about 100 billion solar masses belongs to the (estim. 200 billion) stars!

He is telling you that he thinks only a TENTH of the mass of Milky is stars.
 

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