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Rings of Uranus Figure 7-7 The equatorial diameter of Uranus is about four
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depths It would be gaseous on the outside, then liquid, then slush, and then goo at the core Further missions to Uranus will be necessary to get a better idea of what, exactly, this planet is made of One thing is certain, however: It manages very well to maintain a constant temperature in its outer layers despite the exaggerated seasonal changes in solar irradiation The climatic system that governs the temperatures on Uranus might be called the great thermal equalizer If Earth were tilted on its axis as much as is Uranus, the weather on our planet would be incredibly severe Winters would be brutal everywhere except at the very lowest latitudes The prevailing winds would be fierce as they attempted to equalize the radical annual seesaw of solar energy received at most points on the surface Hurricanes of unimaginable size would prowl the seas and slam into land masses The whole course of the evolution of life on our planet would be much different from what it was We cannot be certain that intelligent life would have evolved at all
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When the Voyager probe visited Uranus in January of 1986, the rings, which exist in the plane of the planet s equator, were seen in detail for the first time Astronomers were not surprised to find them; their existence was known already because, as Uranus passed near distant stars, those stars seemed to blink several times The only possible cause for such blinking was the existence of thin, nearly opaque rings around the planet The fact that Uranus is tipped on its side so that the rings sometimes appear as pronounced ellipses (almost circles when either pole is nearly facing us) was an assist in their discovery prior to the Voyager grand tour The rings of Uranus are much different than those of Saturn; they more resemble the faint rings around Jupiter The albedo (proportion of light reflected) of the rings is only about 1 percent, similar to that of charcoal If you were to visit the Uranian system in a space ship, you would have a hard time seeing the rings even if you passed right through their plane Only if you actually struck one would you notice it easily; this would not be likely because the rings are exceedingly narrow However, the rings consist of good-sized rocks, generally on the order of 70 centimeters (28 inches) or larger in diameter You would not want to navigate your ship through them The narrowness of the Uranian rings seems to run contrary to dynamics The natural tendency, over time, is for the rings to spread out and become
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more flattened, like those of Saturn (although much less prominent) However, small moons orbit near the rings, and the gravitational fields from these moons tends to force and keep the rings into narrow circles Moons of this type have been observed inside the system of Saturn, too, accounting for some of the narrow rings there Because these moons act to confine the ring particles and hold them within specific orbits, they have been termed shepherd moons
Neptune
Neptune, named after the mythical god of the sea, is more than half again as far from the Sun as is Uranus: 4,504 million kilometers (2,799 million miles) This is 3006 AU Neptune receives only about 1/900 as much sunlight per unit area as does the Earth If you re into electronics, acoustics, or physics, you might get some idea of the difference by noting that a ratio of 1:900 is equivalent to approximately 30 decibels (dB) If light were sound and the Sun shining on the Earth were like a loud vacuum cleaner, then the solar illumination on Neptune would be like a small fan running at low speed
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