Exploring Red Supergiants: Size Limits and Birth Possibilities

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In summary, the conversation discusses the size and formation of stars, particularly supergiants, and their role in creating new stars. A link is provided for further information on red supergiant evolution, but it is noted that the topic is still not fully understood. It is also mentioned that red giants evolve from main sequence stars and that a predominantly helium-based star may theoretically be born as a red giant, but it would not be able to initiate helium fusion without exploding.
  • #1
vincentm
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How big can these stars get, Also can a star be born at a Supergiant level?

I'm having a hard time understanding a particular object. The Helix Nebula is said to be the result of a supernova explosion, a closeup reveals tiny knots of gas, now these knots are said to be at least the size of our solar system, which means that the star dying to cause the Helix Nebula must've been huge, but how big was this star?
 
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  • #2
According to Wikipedia, "A supergiant is a very large type of star which is ~10 to 50 solar masses on the Hertzsprung-Russell diagram. Supergiants can have radii in excess of 1000 solar radii."
 
  • #3
My question is will those knots of gas create new stars?
 
  • #4
Possibly this will answer the question.

http://phobos.physics.uiowa.edu/~srs/lec16/lec16.html

Otherwise google with "Red supergiant evolution".

There are a number of pdf's and one site suggests the evolution of red supergiants is still poorly understood.

Of recent supernovae observed, how many were red sg's before.
 
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  • #5
Based on current knowledge [which is not precise or complete] red giants evolve from HR main sequence stars. The core temperature necessary to inflate the photosphere to red giant proportions cannot be achieved by hydrogen fusion. Perhaps a star formed predominantly from helium could theoretically be born a red giant, but I doubt it could ever get hot enough to initiate helium fusion without blowing itself apart.
 

What are Red Supergiants?

Red Supergiants are a type of star that are among the largest and brightest in the universe. They are typically 10 to 20 times more massive than our sun and can be up to a billion times larger in size.

What is the lifespan of a Red Supergiant?

The lifespan of a Red Supergiant varies, but on average they can live for about 10 million years. This may seem like a long time, but it is relatively short compared to other types of stars.

How do Red Supergiants form?

Red Supergiants are formed when a star runs out of hydrogen fuel in its core and starts to fuse heavier elements. This causes the star to expand and become a Red Supergiant.

What is the temperature of a Red Supergiant?

The temperature of a Red Supergiant can range from 3,000 to 5,000 Kelvin. This is much cooler than other types of stars, such as our sun, which has a temperature of around 5,500 Kelvin.

How do Red Supergiants eventually die?

Red Supergiants eventually die in a massive explosion called a supernova. This occurs when the star's core can no longer support its own weight and collapses, releasing a tremendous amount of energy and creating elements that are essential to life, such as carbon and oxygen.

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