<p>The sun is a big ball of hydrogen atoms, that get compressed together due to a huge gravitational force.  We start off with 4 H atoms:</p>

<p>P-e, P-e, P-e, P-e (note: P=proton, e=electron)</p>

<p>Now, when a proton (P) and electron (e) fuse together, they simply combine into a neutron (note: neutron=N). So, if two of those P-e pairs fuse into a neutron, we now have:</p>

<p>N, N, P-e, P-e</p>

<p>Two neutrons, two protons, two electrons. The 4 hydrogen atoms have become a single helium atom. But wait... the mass went on a diet! If we "weighed" the 4 hydrogen atoms, their total mass was = 4(1.004u) = 4.016u. But the end result, a single helium atom, is only 4.003u.</p>

<p>So, from 4 hydrogens to 1 helium, some "weight" was lost, or more exactly, some of the mass converted into energy. How much energy? This much energy:</p>

<p>e=mc^2</p>

CC BY-SA 4.0
2019-03-24T04:13:16.073Z
This answer is a little misleading. The [p-p chain](https://en.wikipedia.org/wiki/Proton–proton_chain_reaction) doesn't quite work that way. Eg, the Sun doesn't fuse protons & electrons to produce free neutrons.
PM 2Ring
CC BY-SA 3.0
2017-05-25T03:44:18.973Z
2017-05-25T03:44:18.973Z
Courtney McFarren
<p>The gravitational pull of the Sun is so big, that it fuses hydrogen to helium-2. Helium-2 is unstable and decays to H-2 through the weak interaction. This releases energy in form of heat. Now again the gravitational pull of the sun is so big that it fuses H-2 to He-4 through the strong interaction. This releases energy in form of heat. </p>

CC BY-SA 4.0
2019-07-01T12:47:15.343Z
2019-07-01T13:16:46.033Z
2019-07-01T13:16:46.033Z
Warrior
<p>As you are suspecting, the sun burns in a different sense, not by chemical reaction with oxygen.</p>

<p><a href="http://en.wikipedia.org/wiki/Atom">Atoms</a> consist of a tiny, heavy <a href="http://en.wikipedia.org/wiki/Atomic_nucleus">nucleus</a>, surrounded by an almost empty space, populated by <a href="http://en.wikipedia.org/wiki/Electrons">electrons</a>. Burning by chemical reaction with oxygen doesn't change the nucleus of atoms, but takes place in the hull of atoms: Atoms may assemble to form <a href="http://en.wikipedia.org/wiki/Molecule">molecules</a>; electrons change their <a href="http://en.wikipedia.org/wiki/Molecular_orbital">orbitals</a> (the way they surround the nucleus), and release some energy as heat.</p>

<p>Atomic nuclei are (positively) electrically charged, and repell each other.
But if small nuclei, like those of hydrogen atoms, come close together, they can <a href="http://en.wikipedia.org/wiki/Nuclear_fusion">fuse</a> and form a larger nucleus. This nuclear fusion of hydrogen to helium (in this case) releases much energy, more even than <a href="http://en.wikipedia.org/wiki/Nuclear_fission">fission</a> of uranium in a <a href="http://en.wikipedia.org/wiki/Nuclear_power_plant">nuclear power plant</a>. The notion "burning" is used sometimes for reactions of atomic nuclei, too, if they release energy as heat.</p>

<p>To overcome the <a href="http://en.wikipedia.org/wiki/Coulomb%27s_law">electrostatic repulsion</a> of <a href="http://en.wikipedia.org/wiki/Hydrogen_atom">hydrogen</a> nuclei, high pressure and temperature are needed. <a href="http://en.wikipedia.org/wiki/Proton-proton_chain">These conditions</a> occur in the <a href="http://en.wikipedia.org/wiki/Solar_core">core of the Sun</a>.</p>

CC BY-SA 3.0
2014-04-29T16:56:17.310Z
2014-04-29T16:56:17.310Z
Gerald
<p>How does the Sun burn without oxygen?</p>

<p>It might not be burning but a big part of the society speaks of it as burning.</p>

<p>So how does it work?</p>

CC BY-SA 3.0
2014-04-29T20:44:32.683Z
I share your view of the universe and the more I learn the more it increases my amazement!
Itumac
CC BY-SA 3.0
2014-04-29T21:48:16.637Z
[This question](http://physics.stackexchange.com/q/26628/5646) on the Physics site is similar. (I think it was originally posted on the old Astronomy site, which was shut down and merged into Physics before this new Astronomy site was created).
Keith Thompson
<the-sun><nucleosynthesis>
How can the Sun burn without oxygen?
NullReference
# How can the Sun burn without oxygen?

(Asked by: username_0 on 2014-04-29)

How does the Sun burn without oxygen?

It might not be burning but a big part of the society speaks of it as burning.

So how does it work?

**Tags:** the-sun, nucleosynthesis
> **Comments:**
> **username_1**: I share your view of the universe and the more I learn the more it increases my amazement!  
> **username_2**: [This question](http://physics.stackexchange.com/q/26628/5646) on the Physics site is similar. (I think it was originally posted on the old Astronomy site, which was shut down and merged into Physics before this new Astronomy site was created).  

---

## 3 answers

### Answer by username_6 on 2014-04-29. Score: 16 | Accepted answer

As you are suspecting, the sun burns in a different sense, not by chemical reaction with oxygen.

[Atoms](http://en.wikipedia.org/wiki/Atom) consist of a tiny, heavy [nucleus](http://en.wikipedia.org/wiki/Atomic_nucleus), surrounded by an almost empty space, populated by [electrons](http://en.wikipedia.org/wiki/Electrons). Burning by chemical reaction with oxygen doesn't change the nucleus of atoms, but takes place in the hull of atoms: Atoms may assemble to form [molecules](http://en.wikipedia.org/wiki/Molecule); electrons change their [orbitals](http://en.wikipedia.org/wiki/Molecular_orbital) (the way they surround the nucleus), and release some energy as heat.

Atomic nuclei are (positively) electrically charged, and repell each other.
But if small nuclei, like those of hydrogen atoms, come close together, they can [fuse](http://en.wikipedia.org/wiki/Nuclear_fusion) and form a larger nucleus. This nuclear fusion of hydrogen to helium (in this case) releases much energy, more even than [fission](http://en.wikipedia.org/wiki/Nuclear_fission) of uranium in a [nuclear power plant](http://en.wikipedia.org/wiki/Nuclear_power_plant). The notion "burning" is used sometimes for reactions of atomic nuclei, too, if they release energy as heat.

To overcome the [electrostatic repulsion](http://en.wikipedia.org/wiki/Coulomb%27s_law) of [hydrogen](http://en.wikipedia.org/wiki/Hydrogen_atom) nuclei, high pressure and temperature are needed. [These conditions](http://en.wikipedia.org/wiki/Proton-proton_chain) occur in the [core of the Sun](http://en.wikipedia.org/wiki/Solar_core).


---

### Answer by username_3 on 2017-05-25. Score: 2

The sun is a big ball of hydrogen atoms, that get compressed together due to a huge gravitational force. We start off with 4 H atoms:

P-e, P-e, P-e, P-e (note: P=proton, e=electron)

Now, when a proton (P) and electron (e) fuse together, they simply combine into a neutron (note: neutron=N). So, if two of those P-e pairs fuse into a neutron, we now have:

N, N, P-e, P-e

Two neutrons, two protons, two electrons. The 4 hydrogen atoms have become a single helium atom. But wait... the mass went on a diet! If we "weighed" the 4 hydrogen atoms, their total mass was = 4(1.004u) = 4.016u. But the end result, a single helium atom, is only 4.003u.

So, from 4 hydrogens to 1 helium, some "weight" was lost, or more exactly, some of the mass converted into energy. How much energy? This much energy:

e=mc^2

> **Comments:**
> **username_4**: This answer is a little misleading. The [p-p chain](https://en.wikipedia.org/wiki/Proton–proton_chain_reaction) doesn't quite work that way. Eg, the Sun doesn't fuse protons & electrons to produce free neutrons.  

---

### Answer by username_5 on 2019-07-01. Score: 1

The gravitational pull of the Sun is so big, that it fuses hydrogen to helium-2. Helium-2 is unstable and decays to H-2 through the weak interaction. This releases energy in form of heat. Now again the gravitational pull of the sun is so big that it fuses H-2 to He-4 through the strong interaction. This releases energy in form of heat.


---

