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mikeemmert
Guest
Another thing I would like to know is, when will Eris pass in front of a star? Occultation will give a good diameter and if we're lucky, we can get Dysnomia, too! There are a couple of asteroids whose shape has been very exactly characterized this way.<br /><br />I don't expect an atmosphere around Eris, but, you never know. If somebody gave me strong odds, say, 10 - 1 or so, I would bet there was an atmosphere around 2003 EL61.<br /><br />My reasoning here is that Santa (provisional name) is covered, not with methane, but with crystalline water ice. Water ice should gradually lose it's crystalline structure under relentless ultraviolet radiation. So the crystalline structure implies the surface is new. How can this be?<br /><br />The best conjecture I can make is that 2003 EL61 has an elongated ellipsoidal shape about twice as long as it is wide. It spins very rapidly, every 3.9 hours, and has two moons. The moons are fairly large, 170 km and 350 km in diameter, and their orbits are fairly close to each other. It's possible that the moons get a tidal beating; thus perhaps their cores are heated. Which might lead to Enceladus-style geysers on the moons.<br /><br />If either Eris or Santa have moons with geysers, this should slightly reduce starlight as they pass in front of a star.<br /><br />That would be intriguing if it happens to be the case. If it does, then it would bolster the case for sending a probe to Saturn rather than Jupiter, for newbies here I have had a couple of freindly debates with 3488 over this ( a true gentleman who does not use logical fallacies or misleading arguments - and never appears in Free Space). <br /><br />Below is a picture of the Eris system, which is posted elsewhere on this thread. I have "enhanced" it, but frankly I don't know what I'm doing, I just played with contrast and brightness and color. What is that object at about the ten o'clock position? Star? Artificial guide star? Moon? Static? Any experts care to comment on t