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Japetus - Übersetzung nach russisch
![The bright regions of Iapetus. [[Roncevaux Terra]] is at the top (north); [[Saragossa Terra]] with its prominent basin [[Engelier]], Iapetus's second largest, is at the bottom.](https://commons.wikimedia.org/wiki/Special:FilePath/Color hemispheres map of Iapetus PIA18436 Nov. 2014 (Cropped).png?width=200 "The bright regions of Iapetus. [[Roncevaux Terra]] is at the top (north); [[Saragossa Terra]] with its prominent basin [[Engelier]], Iapetus's second largest, is at the bottom.")
![Turgis]] (above and right of center) and Ganelon (lower right)](https://commons.wikimedia.org/wiki/Special:FilePath/Iapetus Spins and Tilts.jpg?width=200 "Turgis]] (above and right of center) and Ganelon (lower right)")
.jpg?width=200 "Side view of Iapetus's orbit (red) compared to the other large moons, showing its unusually high inclination")
общая лексика
Япет (спутник Сатурна)
Wikipedia
Iapetus () is a moon of Saturn. It is the 24th of Saturn’s 83 known moons. With an estimated diameter of 1,469 km, it is the third-largest moon of Saturn and the eleventh-largest in the Solar System. Named after the Titan Iapetus, the moon was discovered in 1671 by Giovanni Domenico Cassini.
A relatively low-density body made up mostly of ice, Iapetus is home to several distinctive and unusual features, such as a striking difference in coloration between its leading hemisphere, which is dark, and its trailing hemisphere, which is bright, as well as a massive equatorial ridge running three-quarters of the way around the moon.
