<p>It will become a <a href="https://en.wikipedia.org/wiki/Planetary_nebula" rel="noreferrer">planetary nebula</a> like e.g. the <a href="https://en.wikipedia.org/wiki/Cat%27s_Eye_Nebula" rel="noreferrer">Cat's Eye nebula</a> that was formed by the death of a star with about <a href="https://en.wikipedia.org/wiki/Solar_mass" rel="noreferrer">the same mass as the Sun</a> ~ $1\ M_\odot $:</p>

<p>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;<img src="https://i.sstatic.net/t1qgY.jpg" alt="enter image description here"></p>

<p>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;<sup>Composite image using optical images from the <a href="https://en.wikipedia.org/wiki/Hubble_Space_Telescope" rel="noreferrer">HST</a> and X-ray data from the <a href="https://en.wikipedia.org/wiki/Chandra_X-ray_Observatory" rel="noreferrer">Chandra X-ray Observatory</a></sup></p>

<p>The Sun, and any <a href="https://en.wikipedia.org/wiki/Red_dwarf" rel="noreferrer">red dwarfs</a> above about 0.25 solar masses, will expand into what's called a <a href="https://en.wikipedia.org/wiki/Red_giant" rel="noreferrer">red giant</a>, a late stage of stellar evolution. At this stage, the star starts to fuse different elements, and eventually throws off its layers as a planetary nebula, leaving behind a white dwarf made of carbon and oxygen.</p>

<p>A red dwarf that is too small to become a red giant will not turn into a planetary nebula: its fusion processes will eventually cease and it will probably produce a white <a href="http://en.wikipedia.org/wiki/White_dwarf" rel="noreferrer">dwarf made</a> mostly of helium. But the main-sequence lifetime of these very small stars is longer than the age of the universe, so this has never actually happened yet. The helium white dwarfs that do exist were formed in binary star systems (and were formed during their complex dynamics).</p>

<p>Red dwarfs are small main sequence stars - the smallest and dimmest that are still able to fuse hydrogen in their core. <a href="https://en.wikipedia.org/wiki/Brown_dwarf" rel="noreferrer">Brown dwarfs</a> are even smaller (in terms of mass), but cannot even fuse hydrogen - they are thought to be able to fuse deuterium and lithium. Stars smaller than a brown dwarf turn out to be gas giants like our Jupiter, Saturn, Uranus and Neptune.</p>

CC BY-SA 3.0
2013-11-05T18:33:17.067Z
2013-11-05T21:30:25.907Z
2013-11-05T21:30:25.907Z
TildalWave
<p>When our sun reaches the end of its lifetime , it will turn into a red giant. How long will it be a red giant, and what happens after a star has been a red giant? Does it turn into a planet after a long enough time spent, when it has used up all its helium?</p>

CC BY-SA 3.0
2013-11-05T20:08:10.910Z
No, the Sun will not turn into a red dwarf. Red dwarf stars theoretically will cool down over time -- but none have yet done so because they do so over a time span longer than the current age of the Universe.
Keith Thompson
CC BY-SA 3.0
2013-11-07T02:20:44.783Z
You might want to update your title and question, changing "red dwarf" to "red giant".
Keith Thompson
<star><red-giant>
What happens to a star after it has become a red giant?
bogen
# What happens to a star after it has become a red giant?

(Asked by: username_0 on 2013-11-05)

When our sun reaches the end of its lifetime , it will turn into a red giant. How long will it be a red giant, and what happens after a star has been a red giant? Does it turn into a planet after a long enough time spent, when it has used up all its helium?

**Tags:** star, red-giant

> **Comments:**
> **username_1**: No, the Sun will not turn into a red dwarf. Red dwarf stars theoretically will cool down over time -- but none have yet done so because they do so over a time span longer than the current age of the Universe.  
> **username_1**: You might want to update your title and question, changing "red dwarf" to "red giant".  

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## 1 answers

### Answer by username_2 on 2013-11-05. Score: 11 | Accepted answer

It will become a [planetary nebula](https://en.wikipedia.org/wiki/Planetary_nebula) like e.g. the [Cat's Eye nebula](https://en.wikipedia.org/wiki/Cat%27s_Eye_Nebula) that was formed by the death of a star with about [the same mass as the Sun](https://en.wikipedia.org/wiki/Solar_mass) ~ $1\ M\_\odot $:

![enter image description here](https://i.sstatic.net/t1qgY.jpg)

Composite image using optical images from the [HST](https://en.wikipedia.org/wiki/Hubble_Space_Telescope) and X-ray data from the [Chandra X-ray Observatory](https://en.wikipedia.org/wiki/Chandra_X-ray_Observatory)

The Sun, and any [red dwarfs](https://en.wikipedia.org/wiki/Red_dwarf) above about 0.25 solar masses, will expand into what's called a [red giant](https://en.wikipedia.org/wiki/Red_giant), a late stage of stellar evolution. At this stage, the star starts to fuse different elements, and eventually throws off its layers as a planetary nebula, leaving behind a white dwarf made of carbon and oxygen.

A red dwarf that is too small to become a red giant will not turn into a planetary nebula: its fusion processes will eventually cease and it will probably produce a white [dwarf made](http://en.wikipedia.org/wiki/White_dwarf) mostly of helium. But the main-sequence lifetime of these very small stars is longer than the age of the universe, so this has never actually happened yet. The helium white dwarfs that do exist were formed in binary star systems (and were formed during their complex dynamics).

Red dwarfs are small main sequence stars - the smallest and dimmest that are still able to fuse hydrogen in their core. [Brown dwarfs](https://en.wikipedia.org/wiki/Brown_dwarf) are even smaller (in terms of mass), but cannot even fuse hydrogen - they are thought to be able to fuse deuterium and lithium. Stars smaller than a brown dwarf turn out to be gas giants like our Jupiter, Saturn, Uranus and Neptune.


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