What seasons does Saturn have?
395890
the seasons are just the same as earth but they last longer 1 season lasts 15 earth years
68167
At the temperatures on Saturn, water would be frozen solid below the methane atmosphere, so we can't say anything about water molecules on the planet.\n\nThe Saturn Rings may contain water ice.\n\nWhat can be said with certainty is that both bound hydrogen and bound oxygen can be found on and around Saturn.
919221
Although everyone is saying it, mine has always been saturn. I remember when I first saw saturn through my 5 inch telescope when i was as kid. It was incredible. It was only very small, but i could see the rings and the shadows that they were casting on the planet. It was so beautiful because i was looking at in 3D. It looked so much better that way than even the best photos taken by the voyagers Cassini or the Hubble.
351070
Saturn's rings are always inclined about 30 degrees; the planet's tilt does not change, at least not on any human timescale.  When we see different parts of the ring, as you've surmised, it is a seasonal effect, as the illumination changes over the orbit.  \n\nWhen the rings are edge-on, think of it as being Saturn's equivalent of spring or fall; when they're at full tilt, think of it as summer or winter (depending on the hemisphere).
19950
Saturn has four main groups of rings and three fainter, narrower ring groups. These groups are separated by gaps called divisions. Close up views of Saturn's rings by the Voyager spacecrafts, which flew by them in 1980 and 1981, showed that these seven ring groups are made up of thousands of smaller rings. The exact number is not known.
679895
mercury, mars, venus, earth, jupiter, saturn, uranus, pluto and neptune.
569991
The Sun, Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto.
1075504
Saturn has 31 officially recognized and named satellites\n\nif u want to know their names u can visit at http://www.solarviews.com/eng/saturn.htm
62546
My - Mercury\nVery - Venus\nEntertaining - Earth\nMother - Mars\nJust - Jupiter\nServed - Saturn\nUs - Uranus\nNine - Neptune\nPickles - Pluto
663789
Well it sounds like they all have their very own opinion. I found this wonderful site, it is trust worthy ... it's an on line encyclopedia and was just updated May 30th.\n    Jupiter has at least 63 natural satellites (also called moons!) \n    Saturn has a large number of moons, however no one will ever be certain of the precise number because the floating chunks of ice in Saturn's rings technically count as moons and it is difficult to draw a distinction between a large ring particle and a moon. One cool thing about Saturn is that it has the moon named Titan, which you have probably heard of because it is the only moon in our solar system that has a dense atmosphere. \n   If you decide to check out this site, just scroll down and click on the planet of your choice and it will take you to all the info on that planet, then click on natural satellites. Best of luck to you and search for the truth about these moons!
1045501
Conjunctions between Mars and Saturn occur once every two years.  The last one was on May 23, 2004. If the conjunction occurs when Mars is retrograde, a triple conjunction can take place within a period of a few weeks.\n\nAfter the upcoming M-S conjunction on June 17, the next three will occur on July 8, 2008; July 30, 2010; and August 14, 2012.
236104
Saturn is the 6th planet from the sun.
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Saturn is the sixth planet from the Sun. It is a gas giant (also known as a Jovian planet, after the planet Jupiter), the second-largest planet in the solar system after Jupiter. Saturn has a prominent system of rings, consisting mostly of ice particles with a smaller amount of rocky debris and dust. It was named after the Roman god Saturn. Its symbol is a stylized representation of the god's sickle (Unicode: ♄).
374685
Saturn: The planet Saturn was named after the Roman god of agriculture and the harvest. Saturn is the second largest planet in our solar system (Jupiter is the largest). The planet Saturn is less dense than water - it will float on water. \nFacts:\n\nDiameter: 120,536 km, 9.4 Earth diameters \n\nAverage Distance from Sun: 1.427 billion km, 9.53 AU (astronomical units) \n\nLength of Day: 10 hours 40 minutes \n\nLength of Year: 29.46 Earth Years \n\nNumber of natural satellites: 30 \n\nPlanetary ring system: Yes \n\nAverage temperature: ~134 K (-139 C) Atmospheric composition: Mostly hydrogen and helium. \n\nEccentricity of orbit 0.053\n\nInclination of equator to orbit 26.73°\n\nInclination of orbit to ecliptic 2.48 ° \nGalileo was the first to see Saturn in 1610 through a telescope. 1655- Christian Huygens (Dutch) used a better telescope and suggested that it was surrounded by a thin-flattened ring. Edge on almost impossible to see. Later on discovered that the rings were really system of rings. 1675 Domenico Cassini discovered a dark division in the rings. The Cassini division is a gap about 4500 km wide that separates the outer A ring from the brighter B ring. 1838- Johann Franz Encke discovered a 270 km wide division in the outer A ring\n\nA, B, & C rings are not uniform but consist of hundred upon hundred of closely space bands or ringlets. This is a picture of the F-ring about 100 km wide. Narrowness is due to the gravitational forces exerted by 2 small satellites\n \n\nRings\n\n \n\nThe storm is the white arrowhead shape in the middle of Saturn - pointing to the right. The diameter of this storm is about the diameter of the Earth. \n\n\n\n\n\n\nThe beautiful blue in the photograph is caused by the multiple pictures that have been combined. Blue is not the natural color of Saturn. White in the clouds are white ammonia ice crystals.\nSaturn’s Moons\n1 planet sized satellites\n6 moderate sized satellites\n? tiny satellites\n\nTitan\nA dark cloud band is visible near Titan's north pole, the equator has a wide band of clouds as well. Titan is larger than the planets Mercury and Pluto. The thick haze/atmosphere of Titan. Picture was taken by Voyager 1 in 1980. Titan is the only moon in our solar system with an atmosphere. Titan's atmosphere might even be thicker than the atmosphere of Earth. It consists mainly of nitrogen. \n \n\nTethys: The area on the right hand side of this photo is heavily cratered and brighter/whiter than the rest of Tethys as seen on the left hand side. Tethys has much more craters at the upper half of this picture than at the lower half. The craters at the bottom half were flooded with volcanic lava, making that half smoother. The smallest object you can see on this photograph is about 5 kilometers across.\n\n Tethys\n\n\nRhea: Icy crust. 1600 km in diameter. Along with Iapetus are the largest and most distant from Saturn.\n\n Rhea\n\nMimas: Photograph by Voyager 1 in 1980. Covered with impact craters of all sizes. The largest impact crater on this picture is more than 100 kilometers in diameter. It has a high central peak. \n\n\n Mima\n\nPhoebas: The bright spot in the picture on the left is a mountain. The two bright spots in the photograph on the right are mountain ridges. \n\n\n\n\nJupiter\n\n\nStats\n\nDistance from Sun- 5.203 AU (4.95-5.45AU)\n\nEccentricity of orbit 0.048\n\nOrbital period- 11.86 years\n\nRotational period- equatorial 9 hours 50 min - internal 9 hours 55 min\n\nInclination of equator to orbit 3.12°\n\nInclination of orbit to ecliptic 1.30 °\n\nDiameter 142,984 Km = 11.209 Earth diameters\n\nMass- 1.899 x 1027 = 317.8 Earths\n\nSurface gravity- 2.36\n\nAlbedo- 0.44\n\nAverage temperature -180 °C= -162 °F=165 k\n\nComposition: Largest object in the solar system. Made mostly of lightweight gases. \n\nOpposition: Where and when the best times to see a superior planet. When the planet is on the same side of the sun as Earth. Jupiter is 3x brighter than the brightest st
237709
Saturn travels at an average speed of 21,637 miles per hour or 34,821 kilometers per hour in its orbit around the sun therefore orbiting around the sun once every 29.4 Earth years, or once every 10,755.7 Earth days.
1063562
Saturn.  It's my favorite planet.  I guess because it is so different from the other planets.
856058
http://www.esa.int/SPECIALS/Cassini-Huygens/SEMV75HHZTD_0.html\n\nhttp://www.windows.ucar.edu/tour/link=/saturn/saturn.html&edu=elem\n\nfun facts\nhttp://saturn.jpl.nasa.gov/kids/fun-facts-saturn.cfm