What Are Population I and Population II Stars?

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Discussion Overview

The discussion centers around the classification of stars into Population I and Population II, exploring their characteristics, formation, and distribution within the Milky Way galaxy. Participants examine the distinctions based on metallicity, age, and spatial distribution, as well as the implications of these classifications in astrophysics.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Population I stars are described as the youngest stars with the highest metal content, including the Sun.
  • Some participants note that the distinction between Population I and II is somewhat arbitrary and relates to a bimodal distribution of metallicity in the Milky Way.
  • Population I stars are suggested to have formed later than Population II stars, from gas enriched by supernovae.
  • Population I stars are associated with the thin disk of the Milky Way, while Population II stars dominate the halo.
  • Participants discuss the specific features of Population I and II stars, including their spatial distribution, age, and composition, with Population I having roughly solar metallicity and Population II having significantly lower metallicity.
  • Questions are raised about the exact cutoff in metallicity that differentiates Population I from Population II stars.
  • There is an observation regarding the association of Population I stars with Type II supernovae and Population II stars with Type I supernovae.

Areas of Agreement / Disagreement

Participants express various viewpoints on the definitions and characteristics of Population I and II stars, indicating that multiple competing views remain and the discussion is not resolved.

Contextual Notes

Some limitations include the lack of consensus on the precise metallicity cutoff between Population I and II stars, as well as the dependence on definitions of terms like "metallicity" and "star formation." Unresolved aspects of the discussion include the implications of these classifications for understanding stellar evolution.

randa177
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Can anybody explain to me what a Pop. I object is?
 
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The youngest stars, including the Sun, that have the highest metal content, are known as Population I stars.
 
I guess you answered your own question...

Anyway, the Population I/II distinction is fairly arbitrary, but is based on an apparent bimodality in the metallicity distribution of the Milky Way. Pop I objects probably formed later than Pop II objects and were therefore made from gas that had already been polluted with a lot of heavy metals (mainly by supernovae). This type of star dominates the thin disk of the Milky Way, while the halo is dominated by Pop II objects.
 
Some discussions on Pop I and Pop II objects/stars, what they are and where they are:

http://hyperphysics.phy-astr.gsu.edu/hbase/starlog/pop12.html

http://www.astro.umd.edu/educationalresources/astro/mw/pop.html

http://www.aoc.nrao.edu/~smyers/courses/astro12/L21.html#pop

http://www.astronomy.ohio-state.edu/~dhw/Intro/lec17.html
astronomy.osu.edu said:
17.4 POPULATION I
The two stellar populations differ from each other in spatial distribution, age, and composition.

Features of Population I:
• occurs in disk
• old and young stars
• open clusters (and isolated/binary stars)
• roughly solar metallicity
[typical composition 70% hydrogen, 28% helium, 2% metals]

Associated with Population I:
• interstellar gas and dust
• star-forming gas clouds
• Type II supernovae

17.5 POPULATION II

Features of Population II:
• occurs in spheroid, especially the stellar halo
• old stars only (no blue main sequence stars)
• globular clusters (and isolated/binary stars)
• low metallicity, 1/1000 to 1/100 solar
[typical composition 75% hydrogen, 24.99% helium, 0.01% metals]

Associated with Population II:
• very little interstellar gas or dust
• no star formation
• only Type I supernovae
So where is the cutoff between Pop I and Pop II in terms of metallicity? 0.1% or 1% metals?

Interesting how Pop I stars are associated with Type II SN and Pop II stars are associated with Type I SN.

How Population I and II relate to Galaxies - http://www.astro.psu.edu/users/kluhman/a1/lec25.html

Milky Way Spiral Structure - http://www.seds.org/messier/more/mw_arms.html

http://articles.adsabs.harvard.edu/cgi-bin/nph-build_image?bg=%23FFFFFF&/seri/AJ.../0062/600/0000146.000&db_key=AST&bits=4&res=100&filetype=.gif
 
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