Solve Your HR Diagram Problem with Expert Help - Tuugii

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In summary, the conversation is about solving a problem related to stellar evolution, specifically determining the significance of a 1M star leaving the main sequence at 20 L. A helpful equation for calculating star lifetimes is provided, along with additional resources for further understanding. It is emphasized that effort should be put into finding a solution before seeking assistance.
  • #1
Tuugii
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how to solve it?

thanks,
Tuugii
 
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  • #2
How about trying to write an equation for stellar evolution. One has a 1M (solar mass if I read the symbol correctly) leaving the main sequence at 20 L. What's the significance of that?

We ask students to provide some work and effort when asking for assistance.
 
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  • #3
thanks a lot. But what is the equation of evolution? if you can provide me a little more info on that, I think I can make it further.

Tuugii
 
  • #4
Here are some useful notes on stellar lifetimes. I haven't gone through the details, but there appears to be some variation. It would be worthwhile to do a comparison.

THE MAIN SEQUENCE
http://www.astronomy.ohio-state.edu/~ryden/ast162_4/notes14.html
http://ftp.astronomy.ohio-state.edu/~pogge/Ast162/Unit2/mainseq.html

http://www.astronomynotes.com/evolutn/s8.htm

Star main sequence lifetime = [star's mass / star's luminosity] × 1010 years.
Star main sequence lifetime = 1010 / (star's mass)(p - 1), where p = 3 for stars more massive than 30 solar masses and p = 4 for stars less massive than 10 solar masses.


http://astronomy.swin.edu.au/cosmos/M/Main+Sequence+Lifetime (this page seems pretty good)

http://csep10.phys.utk.edu/astr162/lect/mainseq/mainseq.html

http://zebu.uoregon.edu/~imamura/208/feb6/life.html

Notes on Stars
http://www.astro.uiuc.edu/~kaler/sow/class.html
 
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Related to Solve Your HR Diagram Problem with Expert Help - Tuugii

1. What is an HR diagram?

An HR diagram, or Hertzsprung-Russell diagram, is a graph used in astronomy to plot the luminosity (brightness) of stars against their surface temperature. The resulting plot reveals important information about the life cycle and characteristics of stars.

2. How can the HR diagram help with understanding stellar evolution?

The HR diagram is a useful tool for studying stellar evolution because it allows us to classify stars based on their stage in the life cycle, from protostars to main sequence stars to red giants or white dwarfs. It also helps us understand the relationship between a star's mass, temperature, and luminosity.

3. Can the HR diagram be used to compare different stars?

Yes, the HR diagram can be used to compare stars from different regions of space or different galaxies. By plotting stars on the same graph, we can see how they compare in terms of luminosity, temperature, and stage in their life cycle.

4. What is the main challenge in creating an HR diagram?

The main challenge in creating an HR diagram is obtaining accurate measurements of a star's luminosity and temperature. This requires precise instruments and techniques, as well as reliable data on a star's distance and composition.

5. How can the HR diagram be used to discover new stars or planets?

The HR diagram can be used to identify stars that are unusual or deviant from the expected pattern. This can lead to the discovery of new stars, such as brown dwarfs, or even exoplanets orbiting other stars. By studying the properties of these stars, we can learn more about their formation and the conditions necessary for the existence of other planets.

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