<p>The escape velocity of <a href="http://en.wikipedia.org/wiki/Mars" rel="nofollow">Mars</a> is about $5.03 \mbox{ km}/\mbox{s}$ , that of Earth about $11.2 \mbox{ km}/\mbox{s}$ , that of <a href="http://en.wikipedia.org/wiki/Moon" rel="nofollow">Moon</a> about $2.38 \mbox{ km}/\mbox{s}.$</p>

<p>The escape velocity is an important ingredient for the stability of a planetary atmosphere.
From this it's not surprising, that the density of the Martian atmosphere is between that of Moon and that of Earth.</p>

<p>The loss of most of the magnetic field of Mars makes its atmosphere less resistant to erosive solar wind.</p>

<p>(Actually things get more complicated, since <a href="http://perso.utinam.cnrs.fr/~mousis/papier91.pdf" rel="nofollow">sequestration and outgassing</a>, meaning an exchange of atmosphere with rock, as well as sublimation, and resublimation of water and carbon dioxide take place. Water vapor is decomposed into hydrogen and oxygen by <a href="http://en.wikipedia.org/wiki/Photodissociation" rel="nofollow">photolysis</a>, hydrogen escapes to space due to its low molecular weight, and oxygen tends to be bound chemically to iron-bearing rocks. On the other hand <a href="http://en.wikipedia.org/wiki/Solar_energetic_particles" rel="nofollow">solar wind provides a steady supply of hydrogen</a>, which is bound by rocks in the top few micrometers; "<a href="http://www.lanl.gov/newsroom/news-releases/2012/August/08.23-chemcam-results.php" rel="nofollow">ChemCam saw peaks of hydrogen and magnesium during the first shots that we didn’t see in subsequent firings</a>.")</p>

<p>The history of the Marsian atmosphere isn't yet known in full detail. NASA's <a href="http://en.wikipedia.org/wiki/MAVEN" rel="nofollow">MAVEN</a> mission is designed to find out more.</p>

CC BY-SA 3.0
2014-04-30T11:09:12.793Z
I would add: most of Mars oxygen were captured by iron-bearing rocks which get oxydized. This is why it is orange-red.
Envite
CC BY-SA 3.0
2014-04-30T13:20:48.363Z
@Envite That's true to some degree, but actually the oxidized layer is very thin, mostly restricted to the dust. So, it's difficult to tell, how prevailing this chemical binding of oxygen at the surface actually is.
Gerald
CC BY-SA 3.0
2014-04-29T22:25:57.280Z
2014-04-30T13:17:31.103Z
2014-04-30T13:17:31.103Z
Gerald
<p>Is it because there isn't life to exhale enough oxygen and carbon dioxide? The size of Mars is about the same as Earth, so isn't there enough gravity to hold enough air?</p>

<mars>
Why is Mars' atmosphere so thin?
ashpool
# Why is Mars' atmosphere so thin?

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

Is it because there isn't life to exhale enough oxygen and carbon dioxide? The size of Mars is about the same as Earth, so isn't there enough gravity to hold enough air?

**Tags:** mars


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## 1 answers

### Answer by username_1 on 2014-04-29. Score: 6 | Accepted answer

The escape velocity of [Mars](http://en.wikipedia.org/wiki/Mars) is about $5.03 \mbox{ km}/\mbox{s}$ , that of Earth about $11.2 \mbox{ km}/\mbox{s}$ , that of [Moon](http://en.wikipedia.org/wiki/Moon) about $2.38 \mbox{ km}/\mbox{s}.$

The escape velocity is an important ingredient for the stability of a planetary atmosphere.
From this it's not surprising, that the density of the Martian atmosphere is between that of Moon and that of Earth.

The loss of most of the magnetic field of Mars makes its atmosphere less resistant to erosive solar wind.

(Actually things get more complicated, since [sequestration and outgassing](http://perso.utinam.cnrs.fr/~mousis/papier91.pdf), meaning an exchange of atmosphere with rock, as well as sublimation, and resublimation of water and carbon dioxide take place. Water vapor is decomposed into hydrogen and oxygen by [photolysis](http://en.wikipedia.org/wiki/Photodissociation), hydrogen escapes to space due to its low molecular weight, and oxygen tends to be bound chemically to iron-bearing rocks. On the other hand [solar wind provides a steady supply of hydrogen](http://en.wikipedia.org/wiki/Solar_energetic_particles), which is bound by rocks in the top few micrometers; "[ChemCam saw peaks of hydrogen and magnesium during the first shots that we didn’t see in subsequent firings](http://www.lanl.gov/newsroom/news-releases/2012/August/08.23-chemcam-results.php).")

The history of the Marsian atmosphere isn't yet known in full detail. NASA's [MAVEN](http://en.wikipedia.org/wiki/MAVEN) mission is designed to find out more.

> **Comments:**
> **username_2**: I would add: most of Mars oxygen were captured by iron-bearing rocks which get oxydized. This is why it is orange-red.  
> **username_1**: @username_2 That's true to some degree, but actually the oxidized layer is very thin, mostly restricted to the dust. So, it's difficult to tell, how prevailing this chemical binding of oxygen at the surface actually is.  

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