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JupiterandSaturnRevisitedDaveStevenson
Caltech
InsightCruises,January28,2018
Exploration of the Giant Planets:Pioneer, Voyager, Galileo, Cassini & Juno
Io Europa
Ganymede Callisto
Juno JupiterMass 318 MEarth
Radius 11 REarth
TheFacts
• Moremassivethanalltheotherplanetsputtogether• Mostlyhydrogen&helium;bottomlessatmosphere• Mostofthishydrogenismetallic,probablythemostabundantmetalintheuniverse
• Emits2.5timestheenergyreceivedfromtheSun• Internalheatsourceismostlycooling,partlyheliumrain
• Strongestradiosourceinthenightsky• Largemagneticfield,generatedbyadynamo
Jupitersendsstuffourway
TheQuestions
• Doesithaveacore?• Acentralconcentrationofheavyelements,maybe~10Earthmasses
• Howmuchwater?• Onlymeasurementthusfargaveverylittlewater
• Whatdrivesthewinds?• Andhowdeepdotheygo
• DidJupiterdictatethearchitectureofthesolarsystem?• IncludingplanetEarth
Gravityfield
MagneticField
WaterAbundance
NatureandextentofheavyelementenrichmentinJupiter’score
Whathappenedwhenourplanetsformed?
+poleposition
Gas giant planets formed beyond the frost line where hydrogen gas
captured onto ice & rock core
WhymightaPlanethaveaCore?
BottomUp
Accreteouterlayer
TopDown
Differentiate
WhymightaPlanethaveaCore?
BottomUp
Accretegas
TopDown
Differentiate
PopularGiantPlanetPicture
WellestablishedTerrestrialPlanetPicture
Water H2O
NH4SH
km
AmmoniaNH3
Temperature (Kelvin)
Ammonia cloudscolored by ??phosphine??sulfur compounds, ??
WindsonJupiter
HowtoGetaBillionDollarMissionYourtaxpayer’smoneyatwork
• Collectabunchofcleverscientists• Includinginternationalpartners(ItalyforJuno).
• Talktoabunchofcleverengineers• Writeaproposal• Winthecompetition• Startspendingthemoney• Lotsofmeetings• ConvinceNASAHQthatyouknowwhatyou’redoing.• Makeitwork…..
Spacecraft & Payload
WavesRadio & plasma
MWRMicrowaves
SPACECRAFT DIAMETER: 20 m POWER: ~500 W SPIN PERIOD: 30 s
JEDIHigh-energy particles
JADELow-energy particles
Magnetometer
JIRAMIR spectrometer
Gravity Science
JunoCamcamera
UVSUV spectrometer
Earth Flyby
DeepSpace
Maneuvers
Jupiter Orbit Insertion
Juno Launch 5 Aug 2011
TheOrbit: Keyto theWholeMission
Duck under radiation belts… Skim above clouds…
~32polarorbits
2 Hours pole-to-pole!
Juno Science Instruments OffJupiter
Orbit Insertion
4th July 2016
Juno Science Instruments On!Perijoves 1-10
Aug. 2016– Jan. 2018
Map Gravity & Magnetic Field32 orbits ~evenly spaced in longitude
4 orbits->90°8 orbits->45°16 orbits->23°32 orbits->11°
Measuring Jupiter’s Magnetic Field
Juno
Juno Science Presentation 47Juno Site Visit – Use or disclosure of any of the information of this package is subject to the
• Ioejects 1 ton per secondvolcanic gases
• Europa
• Ganymede• Callisto
Jupiter’s magnetic field extends beyond orbits of the 4 big moons
Hubble Space Telescope
Molecular state
Plasma state
•At Plasma Phase Transition Hydrogen is conducting• Jupiter spins every 10 hours• Internal heat drives convection➢ strong magnetic dynamo
~2.5 Mbar phase transition
R ~ 0.8- 0.95 RJ
Jupiter
Heimpel& Aurnou
Juno Modeling Jupiter's Interior to Match Juno Gravity Data
• No distinct core
• Heavy elements partially mixed
• Helium raining out of outer layer
• All boundaries fuzzy?!
Incomingplanetesimalsencounterenoughgastobreakupwhenthecoreisonly~1ME
AtmosphericbasalTis~4000Kwhencoreis1ME,sufficienttodissolvealltheincomingmaterial
We would like to know the structure at early time (end of accretion)
The structure we see now is not necessarily the same
Smaller core
Enriched envelope
Partialdissolutionofthecore
“Ohthatthistootoosolidfleshwouldmelt,Thawandresolveitselfintoadew!”
-Shakespeare,Hamlet
Wilson&Militzer,2011,2012
Juno Microwave Radiometry
Infrared Image
Mic
row
ave Infra
red
Juno'sobservationsofmicrowavescomingfrom the interiorshow absorption by ammoniain a deep circulation pattern
First hints of deepcirculation.....
JIRAM’s5MicronImager
JIRAM’s IR Poles at 5 μ
North Pole
South Pole
Public voteswhich images JunoCAM takes– and submits their own images
http://missionjuno.swri.educlick on “Junocam”
JunoCAM – The People’s Camera
Composite ofmultiple images
•62
NASA Cassini Maksim Kakitsev
Saturn's polar vortex& hexagon
MassSaturn
~1/3 MassJupiter
Clouds deeper
PJ8
PJ6 –May19th
Juno passed over the Great Red Spot
July 10th!
Voyager image
CassiniatSaturn
CassiniatSaturn
Cassini’slastlook
HowisSaturnsimilartoJupiter?
• Similarradii• Bothmostlyhydrogen• Mostofthathydrogenismetallic• Roughlytenhourspinperiods• StrongEast-Westwinds• CoreofaroundtenorsoEarthmasses• Magneticfields• Extensivesatellitesystems• Rings
HowisSaturndifferentfromJupiter?
• Saturnhasamuchsmallermassandsolowerinternalpressures• WindsonSaturnarefourtimesstronger(upto400m/s)andextendthreeorfourtimesdeeper(to12000km)
• CoreonSaturniswelldefinedwhereasonJupiteritisfuzzy?• SaturnmagneticfieldismuchsmallerandmuchsimplerthanJupiter’sfield
• Saturn’sringsaremuchmoremajestic… butthey’reprobablyyoung!
What’sNext?
• Certain• Europaclipper(mid20’s)• EuropeanmissionJUICEtotheJovianmoons,especiallyGanymede.(2030)
• 50%Likely• Missiontothelakes&seasofTitan
• Possible• Probes?EspeciallyforSaturn.• Seismology… theonlyrealwaytounderstandtheinterior• Enceladus… thelittlemoonthatcould
Questions?
WhyistheCoreanInterestingIssue?
• Presenceofcorecouldtellusabouttheformationprocess• ThiswasamajorpartofthejustificationforJuno• Jupitermaydefinesolarsystemarchitecture
• PersistenceofacoremaytellusthermodynamicsofmixtureswithinJupiter&theconvectivestate
• Relevanttotheheatflow• Possiblyrelevanttothedynamo
SomeDefinitions
• By“core”ImeanacentralconcentrationofelementsheavierthatHandHe
• Thiscoredoesnothavetobesolid(itprobablyisnot)• Thiscoredoesnothavetoberock&iron(itcouldalsocontainice)• Thiscoreneednothaveasharpboundary(itprobablydoesnot)- inthisrespectitisfundamentally differentfromearth’score
• ThiscorecouldcontainsomeHandHemixedintoit(andIwillarguethatitdoes)
"JusttheplaceforaSnark!Ihavesaidittwice:Thataloneshouldencouragethecrew.JusttheplaceforaSnark!Ihavesaiditthrice:WhatItellyouthreetimesistrue.
-LewisCarroll
JunoarrivedatJupiteronJuly4,2016&isspendingoverayearinorbitcollectingdata
Conclusions
• WewillbeabletotellwhetherJupiterhasacoreandevenestablishthemassofthatcoreprovidedwedefinethecoretobetheexcessofheavyelements
• Assumesgoodunderstandingofhydrogenequationofstate
• Wemayhavedifficultyestablishingthenatureofthatcorewithanyconfidence(i.e.,theextenttowhichitisdispersedratherthanconcentrated)by“conventional”techniques(gravitymoments)
• Precession(ifaccurateenough)• Unconventionalincludestidalresponse,normalmodesandperhapsmagneticfield
GreatRedSpot
NASA /JPL/MSSS /Gerald Eichstadt/Sean Doran
NASA /JPL/SwRI/MSSS /Gerald Eichstadt/Sean Doran
Perijove 9 – October
NASA /JPL/SwRI/MSSS /Peitho-54
Not bad for a "public outreach" camera, eh?
Jupiter's aurora is structured & dynamic•75
Juno UVS
NASA /JPL/MSSS /Gerald Eichstadt/Sean Doran
2017-10-24 17:24
South Temperate Zone
NASA /JPL/MSSS /Gerald Eichstadt/Sean DoranAltitude: 15306 km Spatialscale: 10.3 km/pixelSubs/clatitude: -32.4 2017-10-24 17:59
SouthTemperateZone:String of Pearls whiteoval
NASA /JPL/MSSS /Gerald Eichstädt/Sean Doran2017-10-24 17:59
NASA /JPL/MSSS /Gerald Eichstadt /Sean Doran
2017-10-24 18:03
Altitude: 20742 kmSpatial scale: 14 km/pixelSubs/c latitude: -40
WhiteOval inString of Pearls
Southern hemisphere Oval- zoom
NASA /JPL/MSSS /Gerald Eichstadt /Sean Doran2017-10-24 18:03
SouthernHemisphere
Altitude: 33115 km Spatialscale: 22.3 km/pixelSubs/c latitude: -53
2017-10-24 18:11
NASA /JPL/MSSS /Gerald Eichstadt/Sean Doran
Southern Hemisphere Coverage
2017-10-24 18:11 NASA /JPL/MSSS /Gerald Eichstädt/Sean Doran
StackingflybysPJ6
PJ8
PJ9
NorthernStorms
NASA /JPL/MSSS /Gerald Eichstadt /Sean Doran
True Color
NASA /JPL/MSSS /Bjorn Jonsson
2017-09-01 22:03Altitude: 12143 km
Juno
Where’s the water?
What drives the winds?
Jupiter’sAtmosphere