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RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
A Mission to Jupiter – An Introduction to the European Space Agency JUICE Mission.
Ali Zadeh, Renaud Mangeret, Petteri Nieminen, Robert Furnell, Christian poivey, Giovanni Santin, Alessandra Menicucci, Hugh Evans, Torgeir Paulsen, Dave Rodgers, Fabrice Cipriani, Eamonn Daly, Christian Erd, Arno Wielders, Ludovic Duvet, O. Witasse, N. Altobelli + JUICE Study Team
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
COSMIC VISION
• New challenging ESA
missions will see probes
at Mercury and Jupiter
and its moons, studying
exoplanets and
investigating dark matter
and dark energy.
ESA’s long-term scientific programme is based on a vision. The
‘Cosmic Vision’ looks for answers to mankind's fundamental
questions:
• How did we get from the 'Big Bang' to where we are now?
• Where did life come from?
• Are we alone?
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
• LISA Pathfinder (2015) testing technologies for gravity
wave detection
• BepiColombo (2017) a satellite duo exploring Mercury
(with JAXA)
• Cheops (2017) studying exoplanets around nearby bright
stars
• Solar Orbiter (2017) studying the Sun from close range
• James Webb Space Telescope (2018) studying the
very distant Universe (with NASA/CSA)
• Euclid (2020) probing ‘dark matter’, ‘dark energy’ and the
expanding Universe
• JUICE (2022) studying the ocean-bearing moons around
Jupiter
• Plato (2024) searching for planets around distant stars
• Athena (2028) space telescope for studying the energetic
Universe
ESA COSMIC VISION MISSIONS
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
JUICE Mission
• Objective
o JUpiter ICy moons Explorer (JUICE) is the first L-class launch slot in ESA’s Cosmic Vision
Program foreseen in 2022. (L-Class missions constitute ESA’s cornerstone Large-Class missions).
o The objective of the JUICE mission is the investigation of Jupiter and its icy moons, Callisto,
Ganymede and Europa.
o To achieve the scientific goals of the challenging JUICE missions, prior to its selection a
comprehensive set of R&D activities were carried out.
• Mission overview
o Launch in June 2022 with Ariane 5
Interplanetary transfer about 7.5 years ; Multiple fly-bys (Earth, Venus, Mars,
Ganymede)
Scientific measurements around Europa for 35 days
Jupiter high latitudes phase : several Callisto fly-bys during 6 months
Eccentric orbit around Ganymede ; Science performed during 120 days
Circular phase, at 500 km during 160 days before naturally crashing on the moon
• The JUICE mission was awarded to Airbus Defence & Space in 2015.
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
Jupiter System Archetype for gas giants and potential habitats
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
JUICE Mission
JUICE CReMA (ESOC), WP-578
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
Jupiter: Giant magnetosphere
Callisto
Io Plasma torus
Io flux tube
Europa
Ganymede
Callisto
Moon “footprints”
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
Severe radiation environment: Jovian Specification Environment Model (JOSE)
ESA UNCLASSIFIED – For Internal Use
Lethal dose from minutes to hours
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
JUICE electron radiation environment
Earth MEO electron environment
Problem area!
Shielding optimisation
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
JUICE mission radiation dose
Dominated by trapped electrons
For exposed surfaces, the trapped proton contribution also to be considered
But interplanetary cruise phase should not be forgotten…
Galileo SSI camera was blinded by the solar event of 14.7.2000!
SOHO LASCO “Bastille Day Event”
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
JUICE Spacecraft
• Main characteristics of the spacecraft
• The JUICE configuration relies on
telecommunication spacecraft structure
heritage with a central cylinder providing
strength and stiffness, and four external
walls supporting the large appendices.
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
JUICE Spacecraft Configuration
• In particular, the spacecraft configuration features:
Two vaults along the central cylinder gathering most of the
electronic units (platform and instruments)
An optical bench accommodating instruments with stringent
pointing requirements close to the Star Tracker
Optical Heads (STR-OH) to ensure pointing performance
A High Gain Antenna (HGA) to download Gbits/day of science data,
and to ensure TeleMetry (TM)/TeleCommand (TC) links for nominal
operations and safe-mode, and Radio Science
A solar generator with two wings along the Y axis
A bi-propellant main engine aligned with the main thrust axis
A set of bi-propellant thrusters used for attitude control during main
engine boost and a set of bi-propellant thrusters for attitude
control.
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
JUICE System Constraints
• Main system constraint and drivers
To carry a large set of science payloads with various and sometimes
diverging interface and operation requirements to the Jovian system.
Spacecraft design mainly constrained by the ΔV, as for any
interplanetary mission. Almost 2.4 km/s are performed by the
spacecraft, resulting in about 2.7 tons of propellant
Low solar illumination received at Jupiter, that drives both the size and
the technology of the solar arrays
Thermal control, that shall be designed to cope with a hot environment
at Venus and a cold one at Jupiter
Radiations environment around Jupiter is a major mission
driver, calling for a clear shielding strategy of all equipment
and an in-depth screening of electronic components
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
Conclusion
• ESA’s Cosmic Vision programme looks for answers to mankind’s
fundamental questions.
• The Cosmic Vision programme consist of a large number of exiting
missions.
• The JUICE mission will explore Jupiter and its icy moons, Callisto,
Ganymede and Europa.
JUICE is a highly interesting and challenging mission- and in
particular the radiation challenges are unique.
A large number of R&D activities were initiated in the early JUICE
selection phases to identify mission feasibility.
The JUICE payload consist of a large number of state-of-the-art
instruments to realise the JUICE scientific goals.
Special attention is given to the JUICE Radiation Harness Assurance
processes to ensure that the payload and platform perform to their
specification in the Jupiter harsh radiation environment.
RADECS 2016, Bremen, Germany 19 September 2016
European Space Agency
For more information:
• For more information contact:
• Ali Zadeh: [email protected]
• Renaud Mangeret: [email protected]
• For more information on ESA programmes:
• www.esa.int
• For more information on ESA’s Cosmic Vision programmes:
• sci.esa.int/cosmic-vision/
• For more information on the JUICE mission:
• sci.esa.int/juice/