Jupiter Icy Moons Explorer
The JUpiter ICy moons Explorer (JUICE) is an interplanetary spacecraft in development by the European Space Agency (ESA) with Airbus Defence and Space as the main contractor. The mission is being developed to visit the Jovian system and is focused on studying three of Jupiter's Galilean moons: Ganymede, Callisto, and Europa (excluding the more volcanically active Io) all of which are thought to have significant bodies of liquid water beneath their surfaces, making them potentially habitable environments. The spacecraft is set for launch in June 2022 and would reach Jupiter in October 2029 after five gravity assists and 88 months of travel. By 2033 the spacecraft should enter orbit around Ganymede for its close up science mission and becoming the first spacecraft to orbit a moon other than the moon of Earth. The selection of this mission for the L1 launch slot of ESA's Cosmic Vision science programme was announced on 2 May 2012. Its period of operations will overlap with NASA's Europa Clipper mission, also launching in 2022.
Artist's impression of the JUICE spacecraft.
|Mission type||Planetary science|
|Mission duration||7.6 years cruise;|
3.5 years in the Jovian system.
|Manufacturer||Airbus Defence and Space|
|Power||Solar array ~100 m2 (1,100 sq ft) 820 watts|
|Start of mission|
|Launch date||June 2022|
|Rocket||Ariane 5 ECA|
|Launch site||Guiana Space Centre ELA-3|
ESA solar system insignia for JUICE
The mission started as a reformulation of the Jupiter Ganymede Orbiter proposal, which was to be ESA's component of the cancelled Europa Jupiter System Mission—Laplace (EJSM-Laplace). It became a candidate for the first L-class mission (L1) of the ESA Cosmic Vision Programme, and its selection was announced on 2 May 2012. In April 2012 JUICE was recommended over the proposed ATHENA X-ray telescope and a gravitational wave observatory (New Gravitational wave Observatory (NGO)). In July 2015, Airbus Defence and Space was selected as the Prime Contractor to design and build the probe.
Launch and trajectoryEdit
The proposed timeline envisions a launch in June 2022 on an Ariane 5 carrier rocket, a sequence of five gravity assist maneuvers over several orbits meeting Earth, Venus, Earth, Mars, and again Earth, and an arrival at the Jupiter system in October 2029 after 88 months of travel. By 2033 the spacecraft should enter orbit around Ganymede, after completing various maneuvers around Jupiter and the other moons. Proposed instruments include cameras, spectrometers, magnetometers, and an ice-penetrating radar.
The Jupiter Icy moons Explorer will perform detailed investigations on Ganymede as a planetary body and evaluate its potential to support life. Investigations of Europa and Callisto will complete a comparative picture of these Galilean moons. The three moons are thought to harbour internal liquid-water oceans, and so are central to understanding the habitability of icy worlds.
The main science objectives for Ganymede, and to a lesser extent for Callisto, are:
- Characterisation of the ocean layers and detection of putative subsurface water reservoirs;
- Topographical, geological and compositional mapping of the surface;
- Study of the physical properties of the icy crusts;
- Characterisation of the internal mass distribution, dynamics and evolution of the interiors;
- Investigation of Ganymede's tenuous atmosphere;
- Study of Ganymede's intrinsic magnetic field and its interactions with the Jovian magnetosphere.
For Europa, the focus is on the chemistry essential to life, including organic molecules, and on understanding the formation of surface features and the composition of the non-water-ice material. Furthermore, JUICE will provide the first subsurface sounding of the moon, including the first determination of the minimal thickness of the icy crust over the most recently active regions.
More distant spatially resolved observations will also be carried for several minor irregular satellites and volcanic moon Io.
Mission conditions and designEdit
The main spacecraft design drivers are related to the large distance to the Sun, the use of solar power, and Jupiter's harsh radiation environment. The orbit insertions at Jupiter and Ganymede and the large number of flyby manoeuvres (more than 25 gravity assists, and two Europa flybys) requires the spacecraft to carry about 3,000 kg (6,600 lb) of chemical propellant.
Gravity assists include:
- Interplanetary transfer (Earth, Venus, Earth, Mars, Earth)
- Jupiter orbit insertion and apocentre reduction with multiple Ganymede gravity assists
- Reduction of velocity with Ganymede–Callisto assists
- Increase inclination with 10–12 Callisto gravity assists
The Russian Space Research Institute is currently evaluating a Ganymede lander mission called Laplace-P, with emphasis in astrobiology. Cooperation and a possible synergy with JUICE Ganymede orbital mission is being discussed between ESA and Roscosmos. Russia had also proposed to power the JUICE spacecraft with a Russian-built radioisotope thermoelectric generator (RTG), replacing solar panels that would be vulnerable to Jupiter's radiation.
On 21 February 2013, after a competition, 11 science instruments were selected by ESA, which will be developed by scientific and engineering teams from all over Europe, with participation from the US and Japan: 
The Jovis, Amorum ac Natorum Undique Scrutator (JANUS) camera system will image Ganymede and interesting parts of the surface of Callisto at better than 400 m/pixel (resolution limited by mission data volume). Selected targets will be investigated in high-resolution with a spatial resolution from 25 m/pixel down to 2.4 m/pixel with a 1.3 degree field of view. The camera system has 13 panchromatic, broad and narrow-band filters in the 0.36 µm to 1.1 µm range, and provides stereo imaging capabilities. JANUS will also allow relating spectral, laser and radar measurements to geomorphology and thus will provide the overall geological context.
- Principal investigator: P. Palumbo, Parthenope University of Naples, Italy
- Lead Funding Agency: ASI, Italy
Moons And Jupiter Imaging Spectrometer (MAJIS) is a visible and infrared imaging spectrograph operating from 500 nm to 5.50 um, with spectral resolution of 3–7 nm, that will observe tropospheric cloud features and minor gas species on Jupiter and will investigate the composition of ices and minerals on the surfaces of the icy moons. The spatial resolution will be down to 75 m (246.1 ft) on Ganymede and about 100 km (62.1 mi) on Jupiter.
- Principal investigator: Y. Langevin, Institut d'Astrophysique Spatiale, France
- Lead Funding Agency: CNES, France
UV imaging Spectrograph (UVS) is an imaging spectrograph operating in the wavelength range 55–210 nm with spectral resolution of < 0.6 nm that will characterise exospheres and aurorae of the icy moons, including plume searches on Europa, and study the Jovian upper atmosphere and aurorae. It will reach a resolution of 0.5 km (0.3 mi) observing Ganymede and up to 250 km (155.3 mi) observing Jupiter.
- Principal investigator: R. Gladstone, Southwest Research Institute, USA
- Lead Funding Agency: NASA, USA
The Sub-millimeter Wave Instrument (SWI) is a spectrometer using a 30 cm (11.8 in) antenna and working in 1080–1275 GHz and 530–601 GHz with spectral resolving power of ~107 that will study Jupiter's stratosphere and troposphere, and the exospheres and surfaces of the icy moons.
- Principal investigator: P. Hartogh, Max Planck Institute for Solar System Research, Germany
- Lead Funding Agency: DLR, Germany
The GAnymede Laser Altimeter (GALA) is a laser altimeter with a 20 m (65.6 ft) spot size and 0.1 m (3.9 in.) vertical resolution at 200 km (124.3 mi) intended for studying topography of icy moons and tidal deformations of Ganymede.
- Principal investigator: H. Hussmann, DLR, Institute for Planetary Research, Germany
- Lead Funding Agency: DLR, Germany
The Radar for Icy Moons Exploration (RIME) is an ice-penetrating radar working at frequency of 9 MHz (1 and 3 MHz bandwidth) emitted by a 16 m (52.5 ft) antenna that will be used to study the subsurface structure of Jovian moons down to 9 km (5.6 mi) depth with vertical resolution up to 30 m (98.4 ft) in ice.
- Principal investigator: Michele Dougherty, Imperial College London, United Kingdom
- Lead Funding Agency: UKSA, United Kingdom
The Particle Environment Package (PEP) is a suite of six sensors to study the magnetosphere of Jupiter and its interactions with the Jovian moons. PEP will measure positive and negative ions, electrons, exospheric neutral gas, thermal plasma and energetic neutral atoms present in all domains of the Jupiter system from 1 meV to 1 MeV energy.
- Principal investigator: S. Barabash, Swedish Institute of Space Physics, Sweden
- Lead Funding Agency: SNSA, Sweden
The Radio & Plasma Wave Investigation (RPWI) will characterise the plasma environment and radio emissions around the spacecraft, it is composed of four experiments: GANDALF, MIME, FRODO and JENRAGE. RPWI will use four Langmuir probes, each one mounted at the end of its own dedicated boom, and sensitive up to 1.6 MHz to characterize plasma and receivers in the frequency range 80 kHz – 45 MHz to measure radio emissions.
- Principal investigator: J.-E. Wahlund, Swedish Institute of Space Physics, Sweden
- Lead Funding Agency: SNSA, Sweden
The Gravity & Geophysics of jupiter and Galilean Moons (3GM) is a radio science package comprising a Ka transponder and an ultrastable oscillator. 3GM will be used to study the gravity field - up to degree 10 - at Ganymede and the extent of internal oceans on the icy moons, and to investigate the structure of the neutral atmospheres and ionospheres of Jupiter (0.1 - 800 mbar) and its moons.
The Planetary Radio Interferometer & Doppler Experiment (PRIDE) experiment will generate specific signals transmitted by JUICE antenna and received by Very Long Baseline Interferometry to perform precision measurements of the gravity fields and of Jupiter and the icy moons.
Jupiter Icy Moons Explorer in popular mediaEdit
In the internet multimedia fiction project 17776, a sentient JUICE is one of the main characters.
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- An Ultra Stable Oscillator for the 3GM experiment of the JUICE mission