<?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="Wide Field and Planetary Camera 2 - Page 6 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=Wide_Field_and_Planetary_Camera_2&amp;p=5">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Wide_Field_and_Planetary_Camera_2&amp;p=7">3.Next</a>
</p>
<p>detectors, each 800x800 <a href="page.php?w=pixel">pixel</a>s. Three of these, arranged in an L-formation, comprise Hubble's Wide Field Camera (WFC). Adjacent to them is the Planetary Camera (PC), a fourth CCD with different (narrower-focused) optics. This afforded a more detailed view over a smaller region of the visual field. WFC and PC images are typically combined, producing the WFPC2's characteristic stairstep image. When distributed as non-scientific <a href="page.php?w=JPEG">JPEG</a> files the PC portion of the image is shown with the</p><p>
<a accesskey="1" href="page.php?w=Wide_Field_and_Planetary_Camera_2&amp;p=5">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Wide_Field_and_Planetary_Camera_2&amp;p=7">3.Next</a>
</p>

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

</card>
</wml>
