1. The Juno New Frontiers Mission Rosalyn A. Pertzborn Director, OSSE Juno E/PO Lead Madison, WI May 9th, 2006 Office of Space Science Education Space Science & Engineering Center University of WI-Madison rosep@ssec.wisc.edu

2. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 2 Mission Overview Dr. Scott Bolton of SwRI, in San Antonio, TX is Principal Investigator for Juno, the second mission in NASA’s New Frontiers Program Scheduled for Launch in August, 2011 Upon arrival in 2016, the simple spinning solar-powered spacecraft will go into a highly elliptical pole to pole orbit, avoiding the bulk of Jupiter’s radiation Operations are repeatable, cyclic and designed to reduce overall cost

3. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 3 Mission Overview, continued… Juno will help reveal the answers to the remaining mysteries of Jupiter and our solar system by investigating Jupiter’s core, water, upper atmosphere, and magnetosphere Suite of eight instruments will collect data on: –Jupiter’s Gravity Field –Aurora –Deep Atmospheric Structure –Magnetosphere JunoCam will enable students to capture the first images of Jupiter’s North Pole!

4. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 4 Juno Project Organization Telecom PEM Anthony Mittskus (JPL) NASA New Frontiers Program Office Principal Investigator Dr. Scott Bolton, SwRI Deputy Principal Investigator Dr. Jack Connerney, GSFC Deputy Project Scientist Dr. Steve Levin, JPL Science Investigation Office Mgr. Bill Gibson (SwRI) Science Team Education & Public Outreach Rosalyn Pertzborn (U. WI) CTM for LM Contract Rick Nybakken Business Manager Cindy Cornish (JPL) PRA(JPL) Scott Johnston Payload Mgmt. Office Phil Morton (JPL) Flight System Office Al Herzl (LM) Mission Systems Mgmt. Office Steve Matousek (JPL) Science Ops & Data Center Mgr. Bill Gibson (SwRI) Advisory Board PI, Chair Chris Jones (Dir, SSED, JPL) Jim Crocker (VP, LM) Jim Burch (VP, SwRI) Project Manager Rick Grammier (JPL) Deputy Project Manager Rick Nybakken (JPL) MA Manager Sammy Kayali (JPL) Radiation Env. Engineer Mag Control & EMC Engineer System Safety Engineer Project System Engineer Dr. Doug Bernard (JPL) Radiation System Engineer (JPL) Flight Sys. Insight-Oversight Team (JPL) Launch Vehicle (KSC) MWR (JPL) MAG SHM (JPL) Gravity Science (JPL) MAG Flux Gate (GSFC) JADE (SwRI) UVS (SwRI) WAVES (UnivofIowa) EPD (APL) Camera (Malin) * * Note: Telecom PEM reports directly to PM/DPM For cost, schedule, and technical performance; and to LM FSM for technical and schedule delivery

5. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 5 Presentation Overview The Mythology Why Juno? Science Mission Spacecraft Payload Operations Education Conclusion-DVD

6. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 6 The Mythology Juno, the god-sister-wife of Jupiter, maintained a constant, jealous vigil over her god-husband’s dalliances from Mount Olympus. When Jupiter had his tryst with Io, he spread a veil of clouds around the entire planet to conceal his activities. Upon observing the cloud- cloaked planet, Juno immediately suspected Jupiter of concealing activities that would not bear the light. Hence, Juno came down from Mount Olympus and employed her special powers to penetrate the clouds and reveal the true nature of Jupiter….

7. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 7 Why Juno? Peering down through the clouds and deep into Jupiter’s atmosphere, Juno will reveal fundamental processes of the formation and early evolution of our solar system

8. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 8 The Giant Planet Story Solar systems containing Giant Planets such as our own, may be required for life to originate The history of our solar system truly is found in the formation of the planet Jupiter!

9. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 9 Juno Science Objectives Origin Determine Oxygen/Hydrogen ratio (water abundance) and constrain core mass to decide among alternative theories of origin. Interior Understand Jupiter's interior structure and dynamical properties by mapping its gravitational and magnetic fields Atmosphere Map variations in atmospheric composition, temperature, cloud opacity and dynamics to depths greater than 100 bars at all latitudes. Magnetosphere Characterize and explore the three- dimensional structure of Jupiter's polar magnetosphere and auroras.

10. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 10 Origin Juno’s Oxygen measurements discriminate among Jupiter’s formation scenarios. Ar, Kr, Xe, C, and S abundances are well determined, however Oxygen is not yet determined. Juno will determine both the N and O abundances essential for understanding the environment in which Jupiter’s originated.

11. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 11 Jupiter’s Interior Thick atmosphere - Galileo probe reached at least ~ 23 bars Liquid layer under high pressure Metallic hydrogen - under extreme pressure the electrons move freely, creating a conducting layer, and leading to a dynamo and radio emissions Rocky core at center

12. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 12 Interior Juno will investigate the structure and convection of Jupiter’s interior by reaching through the meteorological layer. Gravity sounding explores the mass distribution and core inside of the planet. A possible inner “rock” core is shown, surrounded by a “blue” metallic hydrogen envelope and “yellow” outer envelope of molecular H, all hidden beneath the visible cloud deck.

13. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 13 Interior Juno will measure variations of the magnetic field to determine flow patterns on the core surface. The figure shows a plausible Jovian dynamo with columnar structures in the flow organized about a putative (assumed) core.

14. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 14 Atmosphere The depth of Jupiter’s wind zones, belts, and other features remains one of the most outstanding fundamental questions regarding Jovian atmospheric dynamics.

15. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 15 Atmosphere - Two Possible Scenarios Juno provides three- dimensional views of the atmosphere to depths greater than 100 bars to resolve the basic question of the circulation depth. Top Panel (Scenario 1): Large- scale flow dominates and the belt-zone structure penetrates to depth > 200 bars. Bottom Panel (Scenario 2): small-scale convection dominates and belt zone structure disappears below the water cloud base at 6 bars.

16. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 16 Magnetosphere Jupiter’s powerful magnetospheric dynamics create the brightest aurora in our solar system, as electrons and ions precipitate down into its atmosphere. The three auroral types in this HST UV image are signatures of Jupiter’s momentum transfer processes.

17. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 17 Magnetosphere Juno’s measurements will target each critical path in this closed circuit that transfers angular momentum from Jupiter to its nebula. Juno measures the distinct signatures of different auroral processes as it traverses the poles to greatly improve our understanding of one of the solar systems most remarkable phenomena.

18. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 18 Mission In August, 2011 Juno will be launched from Cape Canaveral using an Atlas 551 rocket. ~ 2 years after launch an Earth flyby will give the spacecraft an additional energy assist to reach Jupiter ~ 5 years after launch.

19. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 19 Jupiter Orbit After orbital insertion (October 2016), Juno will spend most of the mission away from Jupiter’s high radiation environment. The line of apsides (furthest distance from planet) moves southward over mission lifetime.

20. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 20 Spacecraft The solar powered, Spinning Spacecraft built by Lockheed-Martin, provides stability, accurate pointing and simple operations.

21. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 21 Spacecraft Detail (1) Roomy upper deck easily accommodates instruments.

22. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 22 Spacecraft Detail (2) All components are balanced to facilitate spacecraft spin

23. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 23 Payload (1) Spacecraft design fully accommodates all science instruments.

24. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 24 Payload(2)

25. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 25 Operations Juno wraps Jupiter in a uniform net, enabling observations that constrain Jupiter’s core and characterize it’s Dynamo. The one year nominal mission will include 32 orbits of ~ 11days/orbit.

26. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 26 Jupiter Orbit Geometry 100 000 km Inbound Trajectory Callisto 26.3 Rj Io 5.9 Rj Europa 9.4 Rj Ganymede 15.0 Rj Line of apsides at start of mission (2.1º) Line of apsides at EOM (32.5º)

27. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 27 Operations (1) The mission requires only two Spacecraft attitudes during science perijove (nearest Jupiter) passages, thereby simplifying operations.

28. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 28 Operations (2)

29. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 29 Education Juno’s Educational Mission reaches out to communities with historically limited access to NASA resources, facilities and people, particularly: –Rural America –Native American Communities –Young Women –Communities with substantial minority populations

30. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 30 JunoCam JunoCam is an Educational Instrument that will allow students to take the mission’s first visible images of Jupiter’s poles! Juno engages the public and students in the its eleven year journey to discover the “Giant Planet Story”

31. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 31 Juno.wisc.edu

32. Juno Rosalyn Pertzborn – UW Space Place, 9 May 2006 32