<?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="Circumplanetary disk - Page 2 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=Circumplanetary_disk&amp;p=1">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Circumplanetary_disk&amp;p=3">3.Next</a>
</p>
<p>(or <a href="page.php?w=exomoon">exomoon</a>s or <a href="page.php?w=subsatellite">subsatellite</a>s) may form. Such a disk can manifest itself in various ways.</p>

<p><big> Theory </big></p>
<p>A <a href="page.php?w=giant_planet">giant planet</a> will mainly form via <a href="page.php?w=Core-accretion_theory">core accretion</a>. In this scenario a core forms via the accretion of small solids. Once the core is massive enough it might carve a gap onto the <a href="page.php?w=Circumstellar_disc">circumstellar disk</a> around the host <a href="page.php?w=star">star</a>.</p><p>
<a accesskey="1" href="page.php?w=Circumplanetary_disk&amp;p=1">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Circumplanetary_disk&amp;p=3">3.Next</a>
</p>

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

</card>
</wml>
