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In responce to the Aproaching Iapetus thread (which I have found fascinating & Vogon13 has made it more so with his / her insights & knowledge, I would like to start something on the two largest moons of Uranus.<br /><br />Please note that the Uranian system at the time was observed Pole On by the Voyager 2 spacecraft, as the tipped over Uranus system was close to a 'solstice'.<br /><br />This is really for those interested in Planetary Science.<br /><br />1). Does anyone think that Titania may have or have had a subsurface ocean??<br /><br />2). I think that it may have had in the past due to a generally smooth surface & large tectonic faults. Subsurface ocean or tidal stresses or cryovolanic activity? <br /><br />Cryovocanoes erupt slushy ice which then freezes solid, not molten rock as on Earth, Io, Venus, etc.<br /><br />3). Does anyone think that Oberon has displayed evidence of Cryovolcanic activity? <br /><br />4). Both Titania & Oberon are very similar in size to the Saturn moons Rhea & Iapetus, yet all four are very different. Rhea I think is the least interesting as it seems to be nothing more than a giant cratered iceball.<br /><br />In size order largest first (diameter).<br /><br />Titania: 1,578 KM / 980 miles. Uranus system.<br />Rhea: 1,530 KM / 950 miles. Saturn system.<br />Oberon: 1,522 KM / 945 miles. Uranus system.<br />Iapetus: 1,440 KM / 895 miles. Saturn system.<br /><br />Iapetus on the other hand is fascinating, will not say more here as we already have a great Iapetus thread.<br /><br />Titania & Oberon have clearly seen more geological activity than Rhea. Titania appears to have seen the most out of the four.<br /><br />4). Oberon clearly has a rougher surface than its slightly larger sibling Titania, has tall mountains, hilly & large dark floored craters.<br /><br />I will start something on Miranda & Ariel when I have time. I have different questions for these.<br /><br />It was a shame that New Horizons 2 did not happen, as <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>