what is saturns size?
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See the "physical characteristics" section on:\n\nhttp://en.wikipedia.org/wiki/Saturn_(planet)
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Name Distance from Saturn's center (km) Width (km) Named after \nD Ring 66,900 - 74,510 7,500   \nC Ring 74,658 - 92,000 17,500   \nColombo Gap 77,800 ? (2) 100 Giuseppe "Bepi" Colombo \nTitan Ringlet 77,800 ? (2)  ? Titan moon of Saturn \nMaxwell Gap 87,491 (2) 270 James Clerk Maxwell \nB Ring 92,000 - 117,580 25,500   \nCassini Division 117,580 - 122,170 4,700 Giovanni Cassini \nHuygens Gap 117,680 ? (2) 285-440 Christiaan Huygens \nA Ring 122,170 - 136,775 14,600   \nEncke Division 133,589 (2) 325 Johann Encke \nKeeler Gap 136,530 (2) 35 James Keeler \nR/2004 S 1(1) 137,630 (2)  ?   \nR/2004 S 2(1) 138,900 (2)  ?   \nF Ring 140,180 (2) 30-500   \nG Ring 170,000 - 175,000 5,000   \nE Ring 181,000 - 483,000 302,000   \n\nNote:\n(1) temporary designation\n(2) distance is to centre of gaps, rings and ringlets that are narrower than 1000 km\n\n\n\n\nD Ring\nThe D Ring is the innermost ring. It is located inward of the C Ring, and is very faint. In 1980, Voyager 1 detected within this ring three ringlets designated D73, D72 and D68, with D68 being the discrete ringlet nearest to Saturn. Some 25 years later Cassini images showed that D72 had become significantly fainter and moved planetward by 200 kilometres. Present in the gap between the C ring and D73 is finescale structure with waves 30 kilometres apart.\n\n\nC Ring\n \nIn this image of Saturn's rings, the C Ring is the faint ring below the two brighter onesThe C Ring is a wide but faint ring located inward of the B Ring, and was discovered in 1850 by William and George Bond when it was termed the 'Crepe Ring' because it seemed to be composed of darker material than the brighter A and B Rings.\n\nIts thickness is estimated as 5 metres, its mass as 1.1e18 kilogram, and its optical depth varies from 0.05 to 0.12.[1]\n\n\nColombo Gap\nThe Colombo Gap lies in the middle of the C Ring, and contains the bright and narrow Titan Ringlet (also called the Colombo Ringlet) centred at 77,883 kilometres from Saturn's centre.\n\n\nTitan Ringlet\nThe Titan Ringlet (also called the Colombo Ringlet) is centred at 77,883 kilometres from Saturn's centre and is within the Colombo Gap. This ringlet is eccentric; that is, it is slightly elliptical rather than circular. The Titan Ringlet is so named because it is in a resonance with Titan.[2] In this case, the time period of a ring particle's apsidal precession is equal to the time period of Titan's orbital motion, so that the outer end of this eccentric ringlet always points towards Titan.\n\n\nMaxwell Gap\nThe Maxwell Gap lies within the C Ring.\n\n\nB Ring\n \nIn this image of Saturn, the B Ring is the inner of the two wide rings, the Cassini Division is the gap between the two widest rings, and the A Ring is the outer of the two wide ringsThe B Ring is the innermost of the two largest, brightest rings. Unlike the A Ring, it is made of innumerable ringlets, some of which have eccentric orbits. There are also spoke-like features running across it, which are made of suspended dust particles.\n\nIts thickness is estimated as 5 to 10 metres, its mass as 2.8e19 kilogram (about three-quarters of Mimas), and its optical depth varies from 0.4 to 2.5.[3]\n\nThe outer edge of the B Ring is maintained by a 2:1 resonance with the moon Mimas. Ring particles at this location orbit twice for every one orbits of Mimas. The resonance causes Mimas' pulls on these ring particles to accumulate, destabilizing their orbits and leading to a sharp cutoff in ring density.\n\n\nHuygens Gap\nThe Huygens Gap separates the B Ring from the Cassini Division.\n\n\nCassini Division\nThe Cassini Division is a 4,800 km (2,980 mile) region between the A Ring and B Ring. It was discovered in 1675 by Giovanni Cassini. From Earth it appears as a thin black gap in the rings. However, during the Voyager flybys, it was discovered that the gap is full of tiny rings.\n\n\nA Ring\nThe A Ring is the outermost of the two largest, brightest rings.
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Saturn is 9.54 AU from the earth, an astronomical unit is equal to 93 million miles.  At the average speed of a car of 70 miles per hour hahahaha it will take you\n about 1,328,571.4 hours or 55, 357,141 days or 151,663.4 yrs  or some such thing...good luck
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Saturn is a gas giant, so it has no surface.
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http://www.nineplanets.org/saturn.html\nhttp://en.wikipedia.org/wiki/Saturn_(planet)\nhttp://saturn.jpl.nasa.gov/\nhttp://pds.jpl.nasa.gov/planets/welcome/saturn.htm\nhttp://www.windows.ucar.edu/tour/link=/saturn/saturn.html\nhttp://www.spds.nasa.gov/planetary/factsheet/saturnfact.html\n\nHow is that.... Happy reading! lol
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I don't know what it means, but it's also the name of a character in The Tempest by Shakepeare. I believe it's also the moon of some gas giant. Saturn?
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Saturn is the 6th planet from the sun.
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Saturn has 31 known moons.
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Size and connection to the planet(under the water) but mainly size
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below freezing point of water.\n\nThe average temperature on Saturn (at the cloud tops) is -185° C. (88 degrees Kelvin)
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SUN\n        diameter:    1,390,000 km.\n        mass:        1.989e30 kg\n        temperature: 5800 K (surface)\n                     15,600,000 K (core)\n\nMercury \n        orbit:    57,910,000 km (0.38 AU) from Sun\n        diameter: 4,880 km\n        mass:     3.30e23 kg\n\nVenus \n        orbit:    108,200,000 km (0.72 AU) from Sun\n        diameter: 12,103.6 km\n        mass:     4.869e24 kg\n\nEarth \n        orbit:    149,600,000 km (1.00 AU) from Sun\n        diameter: 12,756.3 km\n        mass:     5.972e24 kg\nMars \n      orbit: 227,940,000 km (1.52 AU) from Sun\n      diameter: 6,794 km\n      mass: 6.4219e23 kg\n\nJupiter \n        orbit:    778,330,000 km (5.20 AU) from Sun\n        diameter: 142,984 km (equatorial)\n        mass:     1.900e27 kg\n\nSaturn\n        orbit:    1,429,400,000 km (9.54 AU) from Sun\n        diameter: 120,536 km (equatorial)\n        mass:     5.68e26 kg\n\nUranus \n        orbit:    2,870,990,000 km (19.218 AU) from Sun\n        diameter: 51,118 km (equatorial)\n        mass:     8.683e25 kg\n\nNeptune \n        orbit:    4,504,000,000 km (30.06 AU) from Sun\n        diameter: 49,532 km (equatorial)\n        mass:     1.0247e26 kg\n\nPluto \n        orbit:    5,913,520,000 km (39.5 AU) from the Sun (average)\n        diameter: 2274 km\n        mass:     1.27e22 kg\n --------------------------------------------------\n............ Distance... ..Radius. ..Mass.\n.Name....... (000 km)... .(km).... .(kg)..\n------------- ----------- ---------- -------\nSun............0..... .697000. .1.99e30\nMercury.......57910.. ...2439. .3.30e23 +\nVenus........108200.. ...6052. .4.87e24\nEarth........149600.. ...6378. .5.98e24\nMars.........227940.. ...3398. .6.42e23\nJupiter......778000.. ..71492. .1.90e27\nSaturn......1429000.. ..60268. .5.69e26\nUranus......2870990.. ..25559. .8.69e25 *\nNeptune.....4504300.. ..24764. .1.02e26 *\nPluto.......5913520.. ...1160. .1.32e22
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Saturn has a large number of moons. The precise figure will never be certain as the orbiting chunks of ice in Saturn's rings are all technically moons, and it is difficult to draw a distinction between a large ring particle and a tiny moon. Seven of the moons are massive enough to have collapsed into a spheroid under their own gravitation. These are compared to Earth's moon in the table below. Saturn's most noteworthy moon is Titan, the only moon in the solar system to have a dense atmosphere.\n\nThough it has 47 confirmed satellites.
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Since Saturn does not rotate on its axis at a uniform rate, two rotation periods have been assigned to it (as in Jupiter's case): System I has a period of 10 h 14 min 00 s (844.3°/d) and encompasses the Equatorial Zone, which extends from the northern edge of the South Equatorial Belt to the southern edge of the North Equatorial Belt. All other Saturnian latitudes have been assigned a rotation period of 10 h 39 min 24 s (810.76°/d), which is System II. System III, based on radio emissions from the planet, has a period of 10 h 39 min 22.4 s (810.8°/d); because it is very close to System II, it has largely superseded it.\n\nWhile approaching Saturn in 2004, the Cassini spacecraft found that the radio rotation period of Saturn had increased slightly, to approximately 10 h 45 m 45 s (± 36 s).  The cause of the change is unknown — however, it is thought that this is due to a movement of the radio source to a different latitude inside Saturn, with a different rotational period, rather than an actual change in Saturn's rotation.
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As of right now we don't know sizes of other planets outside our solar system.\n\n But, Jupiter is the largest planet in the Solar System. With an equatorial diameter of 143,884 km, (89,405 miles), it is as wide as more than 11 Earths stacked side by side. The planet also has the shortest period of rotation - Jupiter days last just under ten hours.
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Pluto, being both much smaller than Earth and less dense would have lower gravity.\n\nMars is also less dense, and is also considerably smaller, giving it a lower gravity.\n\nThe gas giants are (on average) less dense than Earth, but much much much bigger, and so have much higher gravity.  Saturn's average density is actually lower than that of water, but because there's so much of Saturn there, its gravity is quite high.  There's some sort of rule in schoolbooks about the solar system that they have to mention that Saturn could float in a bathtub, and that's what they mean.\n\nThe gravity of a planet is directly corellated to both its diameter and its density.\n\nFor example, the Earth is about 8000 miles across, and has a density of 5.5 (g/cc).  On Earth, acceleration due to gravity is 9.8 m/s2, also known as 1 G.  \n\nSaturn has a density of 0.7 (g/cc), but a diameter of 74500 miles.   Multiplying these together, and comparing to Earth's numbers, we discover that Saturn has about 1.185 times the acceleration due to gravity that Earth does.\n\nMars is 4200 miles across, and a density of 3.9 g/cc.  This comes out to a gravity 0.38 that of Earth.
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A typical grain of sand is about 2mm in size and a typical atom is a few angstroms (10^(-10) meters). So if an atom 2 angstrom units big is scaled up to 2mm, thats a scaling factor of 10000000. So, if you scale a 6' man the same number of times, he would be 18288000 meters tall which is 60000000' tall. This means that the man's head will almost reach the midpoint between earth and moon(if his feet were on earth)!!
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How many moons does Saturn have? There you go- good question.