Moons of Saturn - Jet Propulsion Laboratory Aeronautics and Space Administration Moons of Saturn...

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www.nasa.gov Moons of Saturn National Aeronautics and Space Administration 300,000,000 900,000,000 1,500,000,000 2,100,000,000 2,700,000,000 3,300,000,000 3,900,000,000 4,500,000,000 5,100,000,000 5,700,000,000 kilometers 0

Transcript of Moons of Saturn - Jet Propulsion Laboratory Aeronautics and Space Administration Moons of Saturn...

National Aeronautics and Space Administration

www.nasa.gov

Moons of Saturn

National Aeronautics and Space Administration

300,000,000 900,000,000 1,500,000,000 2,100,000,000 2,700,000,000 3,300,000,000 3,900,000,000 4,500,000,000 5,100,000,000 5,700,000,000 kilometers0

LG-2009-09-576-HQ — JPL 400-1344O 09/09

Saturn, the sixth planet from the Sun, is home to a vast array ofintriguinganduniquesatellites—53plus9awaitingofficialconfirmation.ChristiaanHuygensdiscoveredthefirstknownmoonofSaturn.Theyearwas1655andthemoonisTitan.Jean-DominiqueCassinimadethenextfourdiscoveries:Iapetus(1671),Rhea(1672),Dione(1684),andTethys(1684).MimasandEnceladuswerebothdiscoveredbyWilliamHerschelin1789.The next two discoveries came at intervals of 50 or more years —Hyperion(1848)andPhoebe(1898).

As telescopic resolving power improved, Saturn’s family of knownmoonsgrew.EpimetheusandJanuswerediscovered in1966.BythetimeCassini–Huygenswaslaunchedin1997,high-resolutionimagingtechniquesusedonEarth-basedtele-scopes had added to the moon count. Cassini has discovered sixmoonsandmayfindmoreduringitsmission.CassinifocusesitscamerasmainlyonobjectsrelativelyclosetoSaturn;thebrightringscomplicatemoon-huntingefforts.Earth-basedtele-scopes focus on the outer part of the Saturn system, and have foundanumberofmoonsintheouterregions.

EachofSaturn’smoonsbearsauniquestory.Twoofthemoonsorbitwithingapsinthemainrings.Some,suchasPrometheusandPandora,interactwithringmaterial,shepherdingtheringinitsorbit.SomesmallmoonsaretrappedinthesameorbitsasTethysorDione.JanusandEpimetheusoccasionallypassclosetoeachother,causingthemtoperiodicallyexchangeorbits.In2006,Cassinifoundevidenceforanewclassof“moonlets”re-siding within Saturn’s rings, sweeping out small gaps in the ring particles.Theremaybeasmanyas10millionmoonletswithinjust one of the rings.

Here’sasamplingofsomeoftheuniqueaspectsofthemoons:

•Titan—At5,150kilometers(3,200miles)across,Titanisthesolar system’s second-largest moon. Titan hides its surface beneathathick,nitrogen-richatmosphere,butCassini’sinstru-ments have revealed that Titan possesses many parallels to Earth—clouds,dunes,mountains,lakes,andrivers.Titan’satmosphereisapproximately95 percent nitrogen with traces of methane.WhileEarth’satmosphereextendsabout60kilome-ters(37miles)intospace,Titan’sextendsnearly600kilometers(10timesthatofEarth’satmosphere)intospace.

•Iapetushasonesideasbrightassnowandonesideasdarkasblackvelvet,withahugeridgerunningaroundmostofitsdark-sideequator.

•PhoebeorbitstheplanetinadirectionoppositethatofSaturn’slarger moons, as do several of the recently discovered moons.

•Mimashasanenormouscraterononeside,theresultofanimpact that nearly split the moon apart.

•Enceladusdisplaysevidenceofactiveicevolcanism:Cassiniobservedwarmfractureswhereevaporatingiceevidentlyes-capes and forms a huge cloud of water vapor over the south pole.

•Hyperionhasanoddflattenedshapeandrotateschaotically,probablyduetoarecentcollision.

•PanorbitswithinthemainringsandhelpssweepmaterialsoutofanarrowspaceknownastheEnckeGap.

•TethyshasahugeriftzonecalledIthacaChasmathatrunsnearly three-quarters of the way around the moon.

•FourmoonsorbitinstableplacesaroundSaturncalledLagran-gianpoints.Theseplaceslie60degreesaheadoforbehindalargermoonandinthesameorbit.TelestoandCalypsooccupythetwoLagrangianpointsofTethysinitsorbit;HeleneandPoly-deucesoccupythecorrespondingLagrangianpointsofDione.

•SixteenofSaturn’smoonskeepthesamefacetowardtheplanetastheyorbit.Called“tidallocking,”thisisthesamephe-nomenonthatkeepsourMoonalwaysfacingtowardEarth.

In addition to studies of Titan, Cassini continues to gather data aboutmanyoftheothersatellitesinanefforttofullyunderstandthe nature, formation, and dynamics of Saturn’s many intriguing moons.

FAST FACTS

•LargestMoonofSaturn Titan Titan’sDiameter 5,150km(3,200mi)

•ClosestMoontoSaturn Pan Pan’sDistancefromSaturn 133,583km(83,022mi)

•FastestOrbit Pan Pan’sOrbitAroundSaturn 13.8hours

•NumberofMoonsDiscoveredbyVoyager 3 (Atlas,Prometheus,andPandora)

•NumberofMoonsDiscoveredbyCassini 6 (Methone,Pallene,Polydeuces,Daphnis,Anthe,andAegaeon)

ABOUT THE IMAGES

1 2 3

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6 7 8

Cassini’1 s visual and infrared mapping spectrometer can view different layers of Titan’s atmosphere simultaneously.

2 Falsecolor(blue)emphasizesicywalls offracturesonEnceladus.

3 TheHerschelcrateronMimasisarelicofalargeimpactthat nearly destroyed this moon.

4 ThisisthelandscapeseenbytheHuygensprobeonitsdescent to the surface of Titan.

A false-color view pr5 ocessed to enhance the individual jets spurting ice particles on Enceladus.

6 ThisimageisamosaicofimagesofPhoebetakenbyCassini during its historic close encounter in June 2004.

This image of Iapetus, the two-toned moon, shows the 7

brighttrailinghemisphere.

Cassini’8 s false-color image of Rhea enhances the slight dif-ferences in natural color across the moon’s face.

FOR MORE INFORMATION

solarsystem.nasa.gov/saturn

ForthemostrecentSaturnmooncount,visit: solarsystem.nasa.gov/planets/profile.cfm?Object= Saturn&Display=Moons

Some of Saturn’s moons are shown at relative distances to the planet.