<?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="HR 8799 - Page 10 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=HR_8799&amp;p=9">1.Previous</a><br />
<a accesskey="3" href="page.php?w=HR_8799&amp;p=11">3.Next</a>
</p>
<p>reveals that it has a slight overabundance of <a href="page.php?w=carbon">carbon</a> and <a href="page.php?w=oxygen">oxygen</a> compared to the Sun (by approximately 30% and 10% respectively). While some Lambda Boötis stars have <a href="page.php?w=sulfur">sulfur</a> abundances similar to that of the Sun, this is not the case for HR 8799; the sulfur abundance is only around 35% of the solar level. The star is also poor in elements heavier than <a href="page.php?w=sodium">sodium</a>: for example, the iron abundance is only 28% of the solar iron</p><p>
<a accesskey="1" href="page.php?w=HR_8799&amp;p=9">1.Previous</a><br />
<a accesskey="3" href="page.php?w=HR_8799&amp;p=11">3.Next</a>
</p>

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

</card>
</wml>
