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<p><BR/>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'> <font color="#ff0000">Stresses in a rotating sphere are not distributed uniformly. Stresses are higher farther away from the axis of rotation.The only particular advantage that I see to a sphere is that it has maximum volume for a fixed surface area. There are advantages to other shapes if you wish to simulate gravite by imparting a rotaion. <br />Posted by DrRocket</font></DIV></p><p><font size="2"><strong>V</strong></font><strong><font size="2">ery true DrRocket, hence the giant outer planets being oblate spheroids, particularly Saturn & Uranus where their equators are approx 10% greater than their polar diameters.</font></strong></p><p><strong><font size="2"><br />Below: Saturn Ring Plane crossing Hubble Space Telescope. The oblateness of Saturn's form is very apparent here due to the low density & fast rotation.<br /></font></strong></p><p><strong><font size="2">Titan is the large moon on the left. </font></strong><br /><img src="http://sitelife.space.com/ver1.0/Content/images/store/0/5/d05fe2e4-e62a-4ce5-b573-98c19aa4da7d.Medium.jpg" alt="" /></p><p><br /><font size="2"><strong>Uranus also at ring plane crossing Hubble Space Telescope (poles are left & right owing to the extreme axial tilt of Uranus). Like Saturn above, Uranus is clearly oblate due to the low density & fast rotation.</strong></font> <br /><img src="http://sitelife.space.com/ver1.0/Content/images/store/5/4/756be68d-36ae-4937-8475-465678d9bcdf.Medium.jpg" alt="" /><br /> </p><p><font size="2"><strong>This is a most interesting thread. Something I know absolutely nothing about, but is most interesting to read about. </strong></font></p><p><font size="2"><strong>My guess is that a spherical space station / spacecraft if spinning to create lets say 1 G internally at the equator would have to have internal ribs that are thicker at the 'equator' than at the 'poles' but each 'pole' would have to have some sort of reinforcing ring to precent the structure from spinning apart???<br /></strong></font></p><p><font size="2"><strong>Andrew Brown. </strong></font></p> <div class="Discussion_UserSignature"> <p><font color="#000080">"I suddenly noticed an anomaly to the left of Io, just off the rim of that world. It was extremely large with respect to the overall size of Io and crescent shaped. It seemed unbelievable that something that big had not been visible before".</font> <em><strong><font color="#000000">Linda Morabito </font></strong><font color="#800000">on discovering that the Jupiter moon Io was volcanically active. Friday 9th March 1979.</font></em></p><p><font size="1" color="#000080">http://www.launchphotography.com/</font><br /><br /><font size="1" color="#000080">http://anthmartian.googlepages.com/thisislandearth</font></p><p><font size="1" color="#000080">http://web.me.com/meridianijournal</font></p> </div>