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At last, on July 1, 2004, the Cassini spacecraft fired off its breaking rocket, glided into orbit around Saturn, and started taking pictures that left scientists in awe. It wasn't as if they hadn't been prepared for such wonders. The weeks leading up to Cassini's arrival at Saturn had served to intensify their already heated anticipation. It seemed as if each approach-picture taken was more enticing than the one preceding it.
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But small moons like Methone are usually geologically inactive and bereft of an atmosphere. Therefore, they are usually unable to smooth away the scars. Dr. Peter Thomas of Cornell University in Ithaca, New York, explained it this way in the May 17, 2013 New Scientist: "When we look at objects less than 200 kilometers in radius, they are all like potatoes. They have lumps, grooves, craters." This makes Methone's smooth surface a mystery. Dr. Thomas is a Cassini team member.
"We developed new operations methods for INMS for Cassini's final flight through Enceladus' plume. We conducted extensive simulations, data analyses, and laboratory tests to identify background sources of hydrogen, allowing us to quantify just how much molecular hydrogen was truly originating from Enceladus itself," explained Dr. Rebecca Perryman in the April 13, 2017 SwRI Press Release. Dr. Perryman is INMS operations technical lead.
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The very productive Cassini mission might attain some indirect information by analyzing the ring arc material--however, it is unlikely to come close to the little moon again before the mission ends in 2017.
Dr. Thomas and his team also note that electrostatic forces could additionally keep the Space egg delightfully soft. Electrons that haunt Saturn's radiation belt could be charging ice crystals on the surface, causing them to rise, while also rendering them more mobile. However, the team of astronomers say that this is still speculation.
The fact that Enceladus becomes so extremely distorted suggests that it contains quite a bit of water. A watery moon would, of course, be a flexible one. Therefore, for Enceladus to be as flexible as it apparently is, it must hold either an enormous local ocean or one that is global. Parts of that immense ocean may be pleasantly warm--but other portions might be quite hot.