<?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="Radar astronomy - Page 8 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=radar_astronomy&amp;p=7">1.Previous</a><br />
<a accesskey="3" href="page.php?w=radar_astronomy&amp;p=9">3.Next</a>
</p>
<p>dependence of echo strength. Radar could detect something ~1&nbsp;km across a large fraction of an AU away, but at 8-10 AU, the distance to Saturn, we need targets at least hundreds of kilometers wide. It is also necessary to have a relatively good <a href="page.php?w=ephemeris">ephemeris</a> of the target before observing it.</p>

<p><big> History </big></p>
<p>The <a href="page.php?w=Moon">Moon</a> is comparatively close and was detected by radar soon after the invention of the technique in 1946. Measurements included surface roughness and later mapping</p><p>
<a accesskey="1" href="page.php?w=radar_astronomy&amp;p=7">1.Previous</a><br />
<a accesskey="3" href="page.php?w=radar_astronomy&amp;p=9">3.Next</a>
</p>

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

</card>
</wml>
