One difficulty is to explain why it follows the equator almost perfectly. The moons of Saturn are typically thought to have formed through Iapetus has been imaged multiple times from moderate distances by the The monolith featured at the climax of Arthur C. Clarke's 1968 novel Congratulations on this excellent venture… what a great idea!I use WIKI 2 every day and almost forgot how the original Wikipedia looks like. The puzzle is compounded by the fact that the dividing line between the two sides is inexplicably sharp.On the last day of 2004, Cassini made its first close encounter with Iapetus. Iapetus is the 3rd largest moon of planet Saturn, and has a massive equatorial ridge running three-quarters of the way around the moon, giving it the appearance of a walnut.Iapetus also has a striking two-tone coloration, with one hemisphere showing a bright water ice surface and the other hemisphere showing a dark color, possibly due to sublimation effects. This difference is so striking that Cassini noted that he could see Iapetus only on one side of Saturn and not on the other.One explanation of this is that the leading hemisphere is dusted with a coating of material knocked off of Phoebe or some other Saturnian body. The redder color of the leading hemisphere can be seen in bright areas in a lower contrast image (left), and in dark areas in higher contrast images (right).Close-up of 10-kilometer-high (6 mi) mountains within the Computer simulation of the appearance of Saturn from Iapetus when it is at the "highest" point in its inclined orbit. For the mythological figure, see View of Cassini Regio. Saturn's rings are clearly visible (from the other large moons they can only be seen edge-on).Side view of Iapetus's orbit (red) compared to the other large moons, showing its unusually high inclinationPolar view of Iapetus's orbit (red) compared to the other large moons of SaturnThe source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. (2018) The moons more massive than Iapetus are: the Moon, the 4 Van Helden, A., "Saturn through the telescope: A brief historical survey", And as in the image to the left, along the edge of the dark area there are many craters where only one side is covered by the dark material; the boundary between the two regions isn’t so sharp after all. Iapetus is a large moon of Saturn.It was discovered by Giovanni Domenico Cassini in 1671.. Iapetus is unusual: one side is very bright and the other side is very dark. Iapetus (eye-ap'-ə-təs, IPA /aɪˈæpətəs/ , Greek Ιαπετός) is the third-largest moon of Saturn, discovered by Giovanni Domenico Cassini in 1671. Iapetus is inclined almost 15 degrees.The Nine Planets has been online since 1994 and was one of the first multimedia websites that appeared on the World Wide Web.Take an interactive tour of the solar system, or browse the site to find fascinating information, facts, and data about our planets, the solar system, and beyond. Iapetus is a Moon that orbits round the planet Saturn.Its mass is estimated/calculated at being 1,805,952,411,282,580,000,000 … What we do. This is because one half of the moon is covered in ice and the other side is coated in black, dusty carbon deposits. The third largest moon of Saturn An ancient ocean which existed between 600 and 400 million years ago. The albedo of most of the leading hemisphere is about .04, as dark as lampblack, whereas the trailing hemisphere’s albedo is .6, as bright as Europa. There are at least four current hypotheses, but none of them explains why the ridge is confined to Cassini Regio. Roncevaux Terra is at the top (north); Saragossa Terra with its prominent basin Engelier, Iapetus's second largest, is at the bottom.Close-up of north polar region, with the large impact crater Falsaron near bottomThe color dichotomy of Iapetus.


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