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Uranus and Neptune Uranus – The Discovery Discovered in 1781 by William Herschel. He wanted to name the planet “Sidus Georgium” after the king of England. Thankfully, another astronomer talked him out of it and he went with a name from Greco-Roman mythology. Where can you see it? Barely visible to the naked eye, if you know where to look. Few people see it without a telescope. Uranus: Physical Properties Radius: 4.0 x that of Earth Mass: 14.5 x that of Earth Rotation: 17.2 hours Revolution: 84 years Distance: 19 AU Experiences differential rotation Axis of rotation: 98˚ - appears to “roll” around the sun – sometimes its axis is pointed toward the sun No internal heat source. Strange times on Uranus During summer in the northern hemisphere, an observer would see the sun make circles in the sky As summer turned into fall and then into winter, eventually the sun would “fail” to rise! The Discovery of Neptune Discovered because it “perturbed” Uranus’ orbit. Its position was mathematically calculated by two people before it was discovered. The person who first found it did not get credit for its discovered – the two mathematicians that calculated it did. Actually, according to his notes, Galileo may have seen it first – he just didn’t know what it was at the time. Neptune: Physical Properties Period of revolution: 163.7 years (has not made a complete orbit since its discovery – it will in two years!) Distance from sun: 30.1 AU Cannot be seen with the naked eye. You must have a telescope. Radius: 3.9 x that of Earth Mass: 17.1 x that of Earth Neptune: Physical Properties, cont. Experiences differential rotation – atmosphere rotates more slowly than the planet. Rotational period: 16.1 hours. Tilt of axis: 29.6˚ Radiates 2.7 times more heat than it receives from the sun – scientists are not sure why. Atmospheres of Uranus and Neptune Similar to Jupiter and Saturn. Made up of hydrogen, helium, and methane; contains very little ammonia. The more methane, the bluer the planet. Uranus is bluish green, while Neptune is blue. Neptune had the “Great Dark Spot” – located near the equator and about the size of Earth. It has now vanished. Overall, both have stormy weather. Uranian Clouds Neptune’s Great Dark Spot Magnetospheres and Interiors Both planets have a magnetosphere. Both have large rocky cores about the size of Earth, perhaps 10 times more massive. Uranus’s Moons Current count: 27 Largest two were discovered by Herschel: Titania and Oberon Others include Arial, Umbrial, Miranda. They are darker than Saturn’s moons. Miranda has many geological features: faults, ridges, valleys, etc. It is considered to be a tortured world. Miranda Titania Neptune’s Moons Current count: 13 Only two can be seen from Earth – Triton and Nereid. Most have retrograde orbits. Neptune’s Moon Triton 6th largest moon in the solar system. Has a retrograde orbit. Has an atmosphere of nitrogen (100 times thinner than Earth). Contains very few craters, which may be a sign of tectonic activity. Contains large fissures. Contains frozen lakes of water. Voyager 2 detected possible nitrogenspewing geysers. Neptune and Triton More of Triton It may be a “captured” moon. Is actually spiraling toward Neptune. Will eventually be torn apart by Neptune’s gravity. Triton Rings Both Uranus and Neptune have rings. Uranus’s were discovered during a “stellar occultation” – a star passed behind them. They are different from those of Saturn. They are dark, narrow, and widely spaced. Some of Uranus’s moons act as shepherd satellites. Neptune’s rings have “clumped” areas.