mirror: 初始快照

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+<tei-ms:entry>
+<tei-ms:orth><h1 align="center" >Saturn</h1></tei-ms:orth>
+</tei-ms:entry>
+<br />
+<div align="center" title="Saturn's great rings are impressive clouds of dirt."><img src="saturn.jpg"  /></div>
+
+<p ><b class="first" >S</b>aturn's rings make it one of the most familiar, and
+spectacular images of astronomy, not to mention science fiction. When Galileo
+trained a primitive telescope on the planet for the first time in 1610, he was
+misled. From the poorly resolved image in his viewfinder, he believed Saturn to
+be a triple-system, with a large body in the center and smaller ones on each
+side.</p>
+
+<p >The rings may be much younger than the planet itself, and great
+mathematicians have found them worthy of contemplation. Laplace and James Clerk
+Maxwell calculated that Saturn's rings must consist of many smaller objects.</p>
+
+<p >Although the planet is almost the size of <a href="jupiter.htm">Jupiter</a>, its mass is but one third
+as great, giving Saturn the lowest mean density of any solar system object.</p>
+
+<p >As a gas giant, the planet has no single rotation period but rather a variety
+depending on latitude. Upper atmosphere clouds travel around the equator in as
+little as 10 hours and 10 minutes; clouds in high latitudes may take half and
+hour longer to pass across the planet.</p>
+
+<p >Based on gravitational field data, Saturn appears to have a solid core with a
+mass equivalent to up to 20 <a href="earth.htm">Earths</a>. As the most oblate planet, the pull of
+gravity at its equator is less than three quarters of that at the poles.</p>
+
+</body>
+</html>