<p>The nebula from which the sun and the solar system formed contained mostly hydrogen and helium, but also small amounts of heavier elements, including "dust". </p>

<p>Any dust that ended up in the centre of the accretion disc became part of the sun. The sun contains 0.01% silicon, for example. This is only a small proportion, but is still about $2\times10^{26}kg$, 100 times the mass of the Earth. When you add in the Iron, Nickel, Oxygen, Carbon and other elements that make up the rocks, you find that there is enough matter in the sun to make up thousands of rocky planets. (<a href="http://www.space.com/17170-what-is-the-sun-made-of.html" rel="nofollow noreferrer">http://www.space.com/17170-what-is-the-sun-made-of.html</a>)</p>

<p>So it is only that part of the dust that happens not to fall into the sun that goes on to form rocky planets.</p>

<p>The details of the process of planetary formation are complex (and not completely understood) however after the formation of the sun, solar wind cleared out the inner solar system of gas and volatiles, leaving only the rocky planets which were too small to hold on a large hydrogen-helium envelope. Further out, beyond the ice-line, water and other volatiles are solid, and much larger planets can form, that gravitationally attract hydrogen and helium mantles.</p>

<p>see <a href="https://astronomy.stackexchange.com/questions/16140/how-did-the-earth-come-to-be-in-orbit-around-the-sun">How did the Earth come to be in orbit around the sun?</a> for more on planetary formation.</p>

CC BY-SA 3.0
2017-03-21T01:56:39.730Z
Thanks for that, and for the link. It's fascinating. TV programs don't go into nearly enough detail, even programs like The Sky at Night.
Mick
CC BY-SA 3.0
2017-03-21T05:18:19.737Z
The formation of our solar system is even more fascinating than you have described. The elements heavier than hydrogen in our solar system weren't created in the Big Bang, but by a previous supernova.
MaxW
CC BY-SA 3.0
2017-03-21T06:47:43.190Z
@MaxW Hydrogen and helium, I thought?
Charles
CC BY-SA 3.0
2017-03-21T18:58:15.473Z
@MaxW That is not correct. Helium was produced shortly after the big bang. Elements with mass less than iron were mostly formed in the cores of stars, and while some or the heaviest elements were formed by the r-process in supernovae, more were made by the s-process of neutron capture in the cores of large stars. They were distributed to the interstellar medium by supernovae.
James K
CC BY-SA 3.0
2017-03-21T20:03:24.577Z
Yes the big bang created more than just hydrogen. He, Li, and Be in particular.  https://en.wikipedia.org/wiki/Big_Bang_nucleosynthesis
MaxW
CC BY-SA 3.0
2017-03-21T01:37:48.950Z
2017-03-21T01:55:15.510Z
2017-04-13T12:59:06.910Z
James K
<p>When a star system forms from a cloud of gas and dust, why doesn't the dust migrate towards the centre of gravity with the gas to form a star? Why does dust in the accretion disk aggregate to form rocky planets, rather than fall into the proto-star?</p>

CC BY-SA 3.0
2017-03-21T01:15:00.137Z
Can you say why you think the dust is more likely to migrate to the star than gas in the accretion disc?
James K
CC BY-SA 3.0
2017-03-21T01:21:18.373Z
I didn't say that or mean to imply it. I've always wondered why the gas migrates but the dust doesn't, since they are both under the influence of gravity.
Mick
<planetary-formation>
Why do rocky planets form?
Mick
# Why do rocky planets form?

(Asked by: username_0 on 2017-03-21)

When a star system forms from a cloud of gas and dust, why doesn't the dust migrate towards the centre of gravity with the gas to form a star? Why does dust in the accretion disk aggregate to form rocky planets, rather than fall into the proto-star?

**Tags:** planetary-formation
> **Comments:**
> **username_1**: Can you say why you think the dust is more likely to migrate to the star than gas in the accretion disc?  
> **username_0**: I didn't say that or mean to imply it. I've always wondered why the gas migrates but the dust doesn't, since they are both under the influence of gravity.  

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## 1 answers

### Answer by username_1 on 2017-03-21. Score: 8 | Accepted answer

The nebula from which the sun and the solar system formed contained mostly hydrogen and helium, but also small amounts of heavier elements, including "dust".

Any dust that ended up in the centre of the accretion disc became part of the sun. The sun contains 0.01% silicon, for example. This is only a small proportion, but is still about $2\times10^{26}kg$, 100 times the mass of the Earth. When you add in the Iron, Nickel, Oxygen, Carbon and other elements that make up the rocks, you find that there is enough matter in the sun to make up thousands of rocky planets. (<http://www.space.com/17170-what-is-the-sun-made-of.html>)

So it is only that part of the dust that happens not to fall into the sun that goes on to form rocky planets.

The details of the process of planetary formation are complex (and not completely understood) however after the formation of the sun, solar wind cleared out the inner solar system of gas and volatiles, leaving only the rocky planets which were too small to hold on a large hydrogen-helium envelope. Further out, beyond the ice-line, water and other volatiles are solid, and much larger planets can form, that gravitationally attract hydrogen and helium mantles.

see [How did the Earth come to be in orbit around the sun?](https://astronomy.stackexchange.com/questions/16140/how-did-the-earth-come-to-be-in-orbit-around-the-sun) for more on planetary formation.

> **Comments:**
> **username_0**: Thanks for that, and for the link. It's fascinating. TV programs don't go into nearly enough detail, even programs like The Sky at Night.  
> **username_2**: The formation of our solar system is even more fascinating than you have described. The elements heavier than hydrogen in our solar system weren't created in the Big Bang, but by a previous supernova.  
> **username_3**: @MaxW Hydrogen and helium, I thought?  
> **username_1**: @MaxW That is not correct. Helium was produced shortly after the big bang. Elements with mass less than iron were mostly formed in the cores of stars, and while some or the heaviest elements were formed by the r-process in supernovae, more were made by the s-process of neutron capture in the cores of large stars. They were distributed to the interstellar medium by supernovae.  
> **username_2**: Yes the big bang created more than just hydrogen. He, Li, and Be in particular.  https://en.wikipedia.org/wiki/Big_Bang_nucleosynthesis  

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