Jet Propulsion Laboratory California Institute of Technology. Juno Update

Similar documents
Scott Bolton OPAG February 1, 2016

Juno Update for OPAG. Steve Levin Juno Project Scien8st September 7, 2017

Juno Status and Earth Flyby Plans. C. J. Hansen

Radiation: Lessons Learned

Supplemental info for MCR : Change Science Orbit Period from 11 Days to 14 Days

Juno. Fran Bagenal University of Colorado

Last Class. Jupiter. Today s Class

Tilts and Obliquities!

JUNO: sopravvivere alle radiazioni

Last Class. Today s Class 11/28/2017

Juno UV, Optical, & IR Remote Sensing

Launch Period Development for the Juno Mission to Jupiter

How Amateur Astronomers Can Support the Juno Mission

Outline. Characteristics of Jupiter. Exploration of Jupiter. Data and Images from JUNO spacecraft

The Juno Mission. B S.J. Bolton

Feasible Mission Designs for Solar Probe Plus to Launch in 2015, 2016, 2017, or November 19, 2008

Rosetta Mission Status Update. Hal Weaver (JHU/APL) CoI on Rosetta-Alice UV Spectrograph (with help from Art Chmielewski, JPL)

JUpiter Icy Moons Explorer (JUICE) Status report for OPAG. N. Altobelli (on behalf of O. Witasse) JUICE artist impression (Credits ESA, AOES)

Science Scenario Modeling

JUpiter Icy Moons Explorer (JUICE) Status report for OPAG. O. Witasse and N. Altobelli. JUICE artist impression (Credits ESA, AOES)

Post-Cassini Saturn Exploration. Saturn (shallow) Probes. Sushil Atreya NRC Decadal / Outer Planets Irvine, CA, 26 October 2009

Overview of the Jovian Exploration Technology Reference Studies

Planetary Protection Trajectory Analysis for the Juno Mission

NASA Future Magnetospheric Missions. J. Slavin & T. Moore Laboratory for Solar & Space Physics NASA GSFC

ESA s Juice: Mission Summary and Fact Sheet

BepiColombo Mission to Mercury

Titan Saturn System Mission: Jonathan Lunine Co Chair, TSSM JSDT

Exploring the Mysteries of the Cosmos on the MOST Microsatellite Mission

STATUS OF THE JUICE MISSION

The Interior of Giant Planets. Cyrill Milkau

JUICE/Laplace Mission Summary & Status

Jovian Orbiters Like THEMIS (JOLT)

Venus Express: Results, Status and Future Plans

12. Jovian Planet Systems Pearson Education Inc., publishing as Addison Wesley

JUICE: A European Mission to Jupiter and its Icy Moons. Claire Vallat Prague, 15 th November 2018

MAE 180A: Spacecraft Guidance I, Summer 2009 Homework 4 Due Thursday, July 30.

Radiation Environment. Efforts at JPL. Dr. Henry Garrett. Jet Propulsion Laboratory 4800 Oak Grove Dr. Pasadena, CA 91109

Accepted Manuscript. Europa Planetary Protection for Juno Jupiter Orbiter

ESA UNCLASSIFIED For Official Use. BepiColombo à Exploring Mercury

A Concept of Nanosatellite Small Fleet for Earth Observation

Jupiter Science and Capabilities on the Europa Jupiter System Mission

Resource Allocation Planning and Scheduling Office. Deep Space Station-15 Out-of-Service Assessment Report. April 11, 2003

Orbiter Element Brian Cooke

S E C T I O N 7 P R O B E S C I E N C E R E S U L T S

S E C T I O N 8 T H E T O U R

Solar System Exploration

SPRITE: Saturn PRobe Interior and atmosphere Explorer

OPAG Aug. 24, Europa Mission Science Overview

BepiColombo Mission to Mercury - コロンボ. October Jan van Casteren, Mauro Novara.

COVE OVER STORY SUSHEELA SRINIVAS

Lecture #27: Saturn. The Main Point. The Jovian Planets. Basic Properties of Saturn. Saturn:

12a. Jupiter. Jupiter Data (Table 12-1) Jupiter Data: Numbers

Earth 110 Exploration of the Solar System Assignment 4: Jovian Planets Due in class Tuesday, Feb. 23, 2016

Solar Sailing as an Enabling Technology

PHYSICS 3300 Case Study - Falling through Jupiter

Chapter 8 Geospace 1

Design of Orbits and Spacecraft Systems Engineering. Scott Schoneman 13 November 03

PLANET-C: Venus Climate Orbiter mission -Updates- Takehiko Satoh (Kumamoto Univ / JAXA) George Hashimoto (Kobe Univ) PLANET-C team

Spectroscopy for planetary upper atmospheres きょくたん

Jupiter: Giant of the Solar System

Aeolus. A Mission to Map the Winds of Mars. Anthony Colaprete Amanda Cook NASA Ames Research Center

Lecture 23: Jupiter. Solar System. Jupiter s Orbit. The semi-major axis of Jupiter s orbit is a = 5.2 AU

DIN EN : (E)

Jupiter and Saturn: Lords of the Planets

Team X Study Summary for ASMCS Theia. Jet Propulsion Laboratory, California Institute of Technology. with contributions from the Theia Team

VLBA Astrometry of Planetary Orbiters

New Horizons Pluto Kuiper Belt mission: design and simulation of the Pluto Charon encounter

NASA Planetary Science Programs

Outer Solar System. Jupiter. PHY outer-solar-system - J. Hedberg

Júpiter. Authors: Nelly Janchuk (teacher) Victoria Intrieri (15 years old) Sofia Silva (15 years old) Priscila Valdéz (16 years old)

BepiColombo MPO Science Operations Planning Drivers IWPSS-2013

10/6/16. Observing the Universe with Gravitational Waves

The 2013 MAVEN Mission To Mars. Bruce Jakosky MAVEN Principal Investigator University of Colorado

Lecture 11 The Structure and Atmospheres of the Outer Planets October 9, 2017

Status of Outer Planet Flagship Mission Studies. Curt Niebur June 8, 2007 Planetary Science Subcommittee Mtg

CASE/ARIEL & FINESSE Briefing

Technology Reference Studies

An Overview of BepiColombo Thermal Analysis

Linking the Planetary Ephemeris to the ICRF. W. M. Folkner

Planetary Magnetic Fields: Planetary Interiors and Habitability

JAXA s Venus Climate Orbiter (PLANET-C) overview. Launch: Jun 2010 Arrival: Dec 2010 Mission life: 2 years

LEARNING ABOUT THE OUTER PLANETS. NASA's Cassini spacecraft. Io Above Jupiter s Clouds on New Year's Day, Credit: NASA/JPL/University of Arizona

Lecture Outlines. Chapter 11. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Review III. ASTR 371, Fall Jovian Planets and Rings (Lecture Notes 9; Chap 12, 14)

Sun Earth Connection Missions

The Jovian Planets (Gas Giants)

THE VOYAGER-2 NEPTUNE ENCOUNTER

Cassini s Grand Finale Science Highlights & End of Mission

Electromagnetic Radiation

PSWS meeting Multi-wavelength observations of Jupiter's aurora during Juno s cruise phase T. Kimura (RIKEN)

Pre-Decadal study summary European Geophysical Union, 24 April Kim Reh 1, Mark Hofstadter 1, John Elliott 1, Amy Simon 2

LRO Lunar Reconnaissance Orbiter

Jupiter. Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by Spacecrafts

Discovery and Surprise from Entry Probes to Giant Planets

Topside interactions with the Titan atmosphere. Anne Wellbrock

Synergistic observations of the giant planets with HST and JWST: Jupiter's auroral emissions

Space Weather Awareness in the Arctic. Torsten Neubert Head of Section for Solar System Physics

Using This Flip Chart

Chapter 11 Jovian Planet Systems. Jovian Planet Composition. Are jovian planets all alike? Density Differences. Density Differences

Tracking Solar Eruptions to Their Impact on Earth Carl Luetzelschwab K9LA September 2016 Bonus

Transcription:

Juno Update

Juno Status Launched August 2011 Earth flyby October 2013 Jupiter arrival July 4, 2016 Spacecraft is healthy and all instruments are working.

Juno s Science Objectives Origin Determine O/H 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. 3

Juno Payload X and Ka Band Gravity Science (JPL/ASI) Magnetometer MAG/ASC (GSFC/DTU) Microwave Radiometers MWR (JPL) Energetic Particle Detectors JEDI(APL) Jovian Auroral Distributions JADE (SwRI) Waves (U of Iowa) UV Spectrograph UVS (SwRI) Visible Camera - JunoCam (Malin) IR Camera/Spectrometer JIRAM (ASI)

Probing the deep interior from orbit Juno maps Jupiter from the deepest interior to the atmosphere using microwaves, magnetic and gravity fields.

Sensing the deep atmosphere Juno s Microwave Radiometer measures thermal radiation from the atmosphere 1000 atmospheres pressure (~500-600km below the visible cloud tops). Determines water and ammonia abundances in the atmosphere all over the planet

Polar Magnetosphere Exploration Location is Key: Juno passes directly through auroral field lines. A suite of instruments are used to understand the physics: JADE, JEDI, MAG, Waves, JIRAM, UVS

Juno Orbit Geometry Geometry of Juno s orbits viewed with the dawn flank on the left, (top) from the Sun with north up, and (bottom) looking down on the system, the Sun below.

Juno Orbit Geometry Three Juno orbits: showing precession of line of apsides relative to Jupiter s geographic equator.

Overview of two 53.5 day orbits and PJ1 1st 53.5-day orbit (actually 53.422 days) 2nd 53.5-day orbit (actually 53.225 days) PJ0+30d AJ0 OTM AJ0 = 7/31/16 19:44 UTC AJ1 = 9/23/16 03:49 UTC PJ0+40d PJ0+20d PJ0+10d PJ0+50d ~ PJ1-3.4d All tick marks are Solar conjunction every 1 day from PJ0 (9/26/16 ~21:40 UTC) JOI cleanup (PJ0+8.6d) PJ0+3d PJ0+2d PJ0+1d PJ0 = 7/5/16 02:47 UTC (JOI starts 02:30 UTC) PJ1 = 8/27/16 12:54 UTC PJ2 = 10/19/16 18:18 UTC (PRM starts 18:00 UTC) (all 3 PJs) PJ1+14d OTM JPE = 90 (9/7/16 ~00:50 UTC ~ PJ0+64d)

Science Orbit Alternate 14-days Advantages: Juno cruise experience and examination of historical databases suggest safe mode recovery times on order 3-5 days (plus instrument turn-on) or longer for unknown root causes. 3 additional days is significant for safe mode recovery 11 day orbit contains 1 day of margin to maintain back-up OTM and further delay progressively degrades planned science at the next perijove 14 days provides 3 days of margin (on average) to maintain back-up OTM and reduces degradation to planned perijove science Longitude build up provides global coverage earlier in the mission builds up in quadrants v. hemispheres. Advantages of operational schedule to syncing up with 7-day week are intuitive and hard to quantify or characterize key to remember that cadence is for duration of 1+ years.

Science Orbit Alternate : 14-days Baseline : 11-day 14-day Design Constraints 11-day period, 30 orbits completes grid Duration from PRM +1 spare : 363d OTM & Deorbit DV: ~116 m/s Longitude Mesh through First Quarter (192 W Lon spacing) 8 6 4 14-day period, 32 orbits completes grid Duration from PRM + 1 spare : 490d OTM & Deorbit DV: ~150 m/s Longitude Mesh through First Quarter (270 W Lon spacing) 2 7 6 Final longitude spacing of 12 degrees or better Longitude map build up retains coarse mapping followed by fine mapping 2 1 3 5 7 Rotation of Orbit (NON-Sun : 35 max) 3 1 8 5 4 Rotation of Orbit (NON-Sun : 44 max) Perijove passes over Goldstone DSN complex (DSS-25 for Ka-Band) NON = Negative Orbit Normal