juno opag report · 2020. 8. 31. · juno status. • launched 2011 and arrived 2016 • prime...
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Scott BoltonOPAGSeptember 2020
NASA/JPL-Caltech/SwRI/MSSS, Image processing by Kevin M. Gill © CC BY Clyde Foster
Juno OPAG REPORT
Clyde’s Spot
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Juno Status
• Launched 2011 and arrived 2016• Prime mission operations ends July 2021• 53 day polar orbiter; 34 orbits• Extended mission proposal due 9/30/2020• EM decision expected ~12/2020• EM extends to orbits 34 – 76• EM last orbit completes September, 2025
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Gravity X/Ka band DopplerMAG Dual high-accuracy vector fluxgatesASC Visible star cameras for MAGMWR Six channel microwave sounding (1-50 cm)JEDI Energetic particles JADE PlasmaWaves Radio-plasma E/M wavesUVS Ultraviolet spectral imagerJIRAM Infrared spectral imagerJunoCam Visible color imager w/methane filterSRU Main star camera
Juno EM Science Payload
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Juno Extended Mission Proposal
Juno evolves to a full Jovian system explorer with close flybys of satellites and rings.
Juno EM provides a diverse OPAG community with data from 2021 to 2025.
The final selection of science objectives & measurements may be limited by NASA budget.
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A Sampling of EM Science Objectives Addresses discoveries and new targets
Jupiter’s northern hemisphere and poleThe shearing of magnetic featuresCharacterizing the dilute coreProbing the polar magnetopauseIn-situ exploration of the Io-Europa TorusMultiple flybys of Io, Europa and GanymedeDetailed characterization of the ring system
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The EM investigates the northern hemisphere and probes the low altitude acceleration region above Jupiter’s polar cap aurora
The migration of Juno’s perijove northward
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The northern progression of perijove enables Satellite flybys and penetrates Jupiter’s ring halo
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Orbit planet projection: EM orbits reach deep into the southern magnetosphere
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High-resolution views “fill the gap” between the halo and Jupiter
Waves dust impacts through PJ21 (color), future observations are shown in purple
Juno will search for clumps throughout the rings as seen in this image near Adrastea
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The EM provides 3D maps probing the depths of Jupiter’s polar cyclones
Example microwave mapping coverage over Jupiter’s poles during the EM. Colored swath is JIRAM data showing Jupiter’s polar cyclones
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Characterizing the Dilute Core
• The discovery of a dilute core was completed unexpected and is critical to understanding the formation and evolution of Jupiter.
• Juno’s EM will help characterize the dilute core via – tidal response– global water abundance– MOI – zonal field – tesseral harmonics.
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The EM bisects Prime mission longitudes to create a magnetic map with ever-increasing spatial resolution; appropriate to sources that we now know are more shallow than anticipated.
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The EM performs a high-resolution magnetic survey above the Great Blue Spot (GBS) to characterize the distortion (shear) of the GBS due to zonal winds at few 1,000 km depths.
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First radio occultations to cover a wide range of latitude and longitude
Probing upper atmosphere and ionosphere along the Io Flux Tube footprint, polar auroral oval, and mid-latitudes
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Clipper-JUICE Radiation Environment
Dissecting the Io-Europa-Ganymede Torus:– In-situ F&P– Update radiation – Coverage of – low & high latitudes
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Juno’s Satellite Encounters– Ganymede
• Surface composition, space weathering maps, ,magnetospheric interaction (thru wake)
– Europa• Ice shell, plume search, organics maps, surface
sputtering
– Io• Magma ocean, polar volcanoes & SO2 maps,
magnetospheric interaction– Semi-major axis of each moon to compare with
astrometry from other missions (LaPlace resonance)
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Moon ~Alt (km) YR
Ganymede 1000 mid 2021
Ganymede 50000 mid 2021
Europa 88000 late 2021
Europa 47000 early 2022
Io 85000 mid 2022
Europa 320 late 2022
Io 63000 late 2022
Io 51000 early 2023
Io 35000 mid 2023
Io 22000 mid 2023
Io 11000 late 2023
Io 1500 early 2024
Io 1500 early 2024
Io 18000 early 2024
Io 83000 late 2024
Io 94000 mid 2025
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Ganymede Science
• Investigate the 3-D structure of Ganymede’s magnetosphere
• Surface composition,role of radiolytic processes in surface weathering• Investigate surface changes since Voyager and Galileo
JIRAM Ganymede map at 23km resolution
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Juno Europa Science
Ice shell characterization:– Identify regions where ice is thick, thin or has
subsurface liquid– Map surface with MWR∼120-200 km resolution
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Europa ScienceSurface Composition and Sputtering
– Map water ice, CO2 and organics (10 km res)– Ions/ion cyclotron waves infer chlorine– F&P constrain surface sputtering– Juno’s plasma instrument represents a significant
advancement for constraining sputtering
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Juno Europa SciencePlume Search:
– Search for surface changes (1-2 km resolution)– JunoCam, SRU (High phase forward scattering )– In-situ F&P to characterize mag field, wave
emissions, electron densities and dust environment
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Io Science • Juno will constrain k2 to help
clarify the physical origin of Io’s volcanism
• Juno will monitor Io volcanic activity, including the polar region. Global mapping addresses where internal dissipation of tidal heating occurs.
Io at ~300,000 km
JunoCam SRU
JIRAM