<?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="Polaris - Page 10 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=Polaris&amp;p=9">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Polaris&amp;p=11">3.Next</a>
</p>
<p>it was once thought to be a <a href="page.php?w=type_II_Cepheid">type II Cepheid</a> due to its high <a href="page.php?w=galactic_latitude">galactic latitude</a>. Cepheids constitute an important <a href="page.php?w=standard_candle">standard candle</a> for determining distance, so Polaris, as the closest such star, is heavily studied. The <a href="page.php?w=Variable_star">variability</a> of Polaris had been suspected since 1852; this variation was confirmed by <a href="page.php?w=Ejnar_Hertzsprung">Ejnar Hertzsprung</a> in 1911.</p>

<p>The</p><p>
<a accesskey="1" href="page.php?w=Polaris&amp;p=9">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Polaris&amp;p=11">3.Next</a>
</p>

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

</card>
</wml>
