The Sun's Final Form: Radius, Mass & Composition

In summary, the future of our Sun involves it becoming a white dwarf, with a radius of 1/100th of its current size and mostly composed of carbon and oxygen. It will continue to emit light for a long time before eventually becoming a black dwarf with no visible radiation. This information can be found on a web page created by Helmut Schattl of the Max Planck Institute, which also includes a video discussing the topic.
  • #1
Helios
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63
When the Sun burns out entirely and reaches the ambient temperature of outer space, what will be its radius, mass, and composition? What would we call such a thing?
 
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  • #2
The Sun will blow off its outer layers and will exist as nothing more than an exposed, dead core. This is known as a white dwarf. It'll be mostly carbon and oxygen, and will have a radius of only about 1/100th of the Sun in its present state. It will continue to shine for a very long time, since it'll be hot and have a small surface area. Eventually, it'll cool to the point where it will no longer emit any visible radiation. It will become a "black dwarf."

http://en.wikipedia.org/wiki/White_dwarf

- Warren
 
  • #3
I've cut and paste the following I posted in a previous thread regarding the future of our sun- https://www.physicsforums.com/showthread.php?p=1267025#post1267025

'Below is a link to a web page created by Helmut Schattl of the Max Planck Institute regarding the future of our sun-

http://home.arcor.de/helmut.schlattl/astro/animation/english/anim_index.html

There's a 7 minute video which is informative (this is a bit tricky to d/l. Right click on "The Future of Our Sun" and 'save target as'. In the 'file name' box, replace the second suffix .avi with .bz2 so the file name reads sun.avi.bz2, then in the 'save as type' box, change to 'all files', then save the file to your computer. Once saved, the zipped file can be opened with bzip2 or winRAR software. Alternatively, the video is posted on YouTube under the same title).'

regards
Steve
 

1. What is the final form of the Sun?

The final form of the Sun is a white dwarf, which is a small, dense, and extremely hot star that has used up all of its nuclear fuel and is no longer able to generate energy through nuclear fusion.

2. What is the radius of the Sun's final form?

The radius of a white dwarf is typically around 0.01 times the radius of the original star, making it much smaller than the Sun's current size.

3. How does the mass of the Sun change in its final form?

The mass of a white dwarf is around 0.6 times the mass of the original star, as the outer layers are blown away during the star's death and only the core remains.

4. What is the composition of the Sun's final form?

The composition of a white dwarf is mostly made up of carbon and oxygen, as these are the elements that remain after nuclear fusion has ceased. There may also be traces of other elements, depending on the mass of the original star.

5. How long does it take for the Sun to reach its final form?

The Sun is estimated to have a lifespan of around 10 billion years. It is currently about halfway through its life, so it will take another 5 billion years for it to reach its final form as a white dwarf.

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