<?xml version="1.0" encoding='utf-8'?>
<!DOCTYPE wml PUBLIC "-//WAPFORUM//DTD WML 1.1//EN" "http://www.wapforum.org/DTD/wml_1.1.xml">
<wml>
<card id="card1" title="Structure formation - Page 19 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=structure_formation&amp;p=18">1.Previous</a><br />
<a accesskey="3" href="page.php?w=structure_formation&amp;p=20">3.Next</a>
</p>
<p>can be used in some cases). While in principle these simulations are quite simple, in practice they are tough to implement, as they require simulating millions or even billions of particles. Moreover, despite the large number of particles, each particle typically weighs 10<sup>9</sup> <a href="page.php?w=solar_mass">solar mass</a>es and <a href="page.php?w=discretization">discretization</a> effects may become significant. The largest such simulation as of 2005 was the <a href="page.php?w=Millennium_simulation">Millennium simulation</a>.</p>

<p>The</p><p>
<a accesskey="1" href="page.php?w=structure_formation&amp;p=18">1.Previous</a><br />
<a accesskey="3" href="page.php?w=structure_formation&amp;p=20">3.Next</a>
</p>

<do type="prev" label="Search">
        <go href="search.wml"/>
</do>

</card>
</wml>
