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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).<ref>[http://meetingorganizer.copernicus.org/EPSC-DPS2011/EPSC-DPS2011-1343-1.pdf JUICE (JUpiter ICy moons Explorer): a European-led mission to the Jupiter system]</ref> 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.<ref name='selection'/>
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).<ref>[http://meetingorganizer.copernicus.org/EPSC-DPS2011/EPSC-DPS2011-1343-1.pdf JUICE (JUpiter ICy moons Explorer): a European-led mission to the Jupiter system]</ref> 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.<ref name='selection'/>


In April 2012, JUICE was recommended over the proposed [[Advanced Telescope for High Energy Astrophysics|ATHENA]] X-ray telescope and a [[gravitational wave]] observatory ([[New Gravitational wave Observatory]] (NGO)).<ref>{{cite news|work=Emily Lakdawalla|url=http://www.planetary.org/blogs/emily-lakdawalla/2012/3458.html|title=JUICE: Europe's next mission to Jupiter?|date=18 April 2012|publisher=[[The Planetary Society]]}}</ref>·<ref>{{cite news|work=Jonathan Amos|title=Disappointed astronomers battle on|date=19 April 2012|url=https://www.bbc.co.uk/news/science-environment-17773383|publisher= BBC News Online|accessdate=2012-04-20}}</ref> In July 2015, Airbus Defence and Space was selected as the prime contractor to design and build the probe.<ref>{{cite news|work=ESA|url= http://sci.esa.int/juice/56165-preparing-to-build-esas-jupiter-mission/|title=Preparing to build ESA's Jupiter mission|date= 17 July 2015|publisher=[[ESA]]}}</ref>
In April 2012, JUICE was recommended over the proposed [[Advanced Telescope for High Energy Astrophysics|ATHENA]] X-ray telescope and a [[gravitational wave]] observatory ([[New Gravitational wave Observatory]] (NGO)).<ref>{{cite news|work=Emily Lakdawalla|url=http://www.planetary.org/blogs/emily-lakdawalla/2012/3458.html|title=JUICE: Europe's next mission to Jupiter?|date=18 April 2012|publisher=[[The Planetary Society]]}}</ref>·<ref>{{cite news|work=Jonathan Amos|title=Disappointed astronomers battle on|date=19 April 2012|url=https://www.bbc.co.uk/news/science-environment-17773383|publisher= BBC News Online}}</ref> In July 2015, Airbus Defence and Space was selected as the prime contractor to design and build the probe.<ref>{{cite news|work=ESA|url=http://sci.esa.int/juice/56165-preparing-to-build-esas-jupiter-mission/|title=Preparing to build ESA's Jupiter mission|date= 17 July 2015|publisher=[[ESA]]}}</ref>


== Timeline ==
== Timeline ==

Revision as of 05:23, 4 March 2020

For the similarly-named cancelled NASA concept, see Jupiter Icy Moons Orbiter.

Jupiter Icy Moons Explorer
File:JUICE spacecraft.png
Artist's impression of the JUICE spacecraft
Mission typePlanetary science
OperatorESA
COSPAR ID2023-053A Edit this at Wikidata
SATCAT no.56176Edit this on Wikidata
Mission durationCruise phase: 7.6 years
Science phase: 3.5 years
Spacecraft properties
ManufacturerAirbus Defence and Space
Launch mass4,800 kg (10,600 lb) [1]
Dry mass1,900 kg (4,200 lb) [1]
Power820 watts[2] from a Solar array ~100 m2 (1,100 sq ft)[3]
Start of mission
Launch dateJune 2022 (planned) [4]
RocketAriane 5 ECA
Launch siteCentre Spatial Guyanais, ELA-3
ContractorArianespace
Flyby of Earth
Closest approachMay 2023
Distance12,700 km (7,900 mi)
Flyby of Venus
Closest approachOctober 2023
Distance9,500 km (5,900 mi)
Flyby of Earth
Closest approachSeptember 2024
Distance1,950 km (1,210 mi)
Flyby of Mars
Closest approachFebruary 2025
Distance1,100 km (680 mi)
Flyby of Earth
Closest approachNovember 2026
Distance3,700 km (2,300 mi)
Jupiter orbiter
Orbital insertionPlanned: October 2029
Orbital departureSeptember 2032
Ganymede orbiter
Orbital insertionPlanned: September 2032
JUICE mission logo
JUICE mission insignia
← Euclid
SMILE →

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 will study 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.[5]

The spacecraft is set for launch in June 2022 and will reach Jupiter in October 2029 after five gravity assists and 88 months of travel. By September 2032 the spacecraft will 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.[6] Its period of operations will overlap with NASA's Europa Clipper mission, launching in 2024.

History

Concept art for the Jupiter Ganymede Orbiter, the ESA component of the proposed Europa Jupiter System Mission – Laplace.

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).[7] 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.[6]

In April 2012, JUICE was recommended over the proposed ATHENA X-ray telescope and a gravitational wave observatory (New Gravitational wave Observatory (NGO)).[8]·[9] In July 2015, Airbus Defence and Space was selected as the prime contractor to design and build the probe.[10]

Timeline

Launch and trajectory

JUICE will be launched in June 2022 by an Ariane 5 rocket. Following the launch, there is a planned first flyby of Earth in May 2023, Venus in October 2023, second flyby of Earth in September 2024, Mars in February 2025 and a final third flyby of Earth in November 2026, to put the JUICE on a trajectory to Jupiter.

Arrival to the Jovian system

In October 2029, when it arrives in Jupiter's system, JUICE will first perform a flyby of Ganymede in preparation for orbital insertion ≈7.5 hours later. The first orbit will be elongated, with the first Jupiter closest approach taking place in May 2030. After that, the orbits will be gradually closer to Jupiter, resulting in a circular orbit.

The first Europa flyby will take place in October 2030. JUICE will enter a high inclination orbit to allow exploration of Jupiter's polar regions. JUICE will study Jupiter's magnetosphere. Then a Callisto flyby in April 2031 will put JUICE on a normal equatorial orbit. Also, there is a transit of Europa and Io that will occur on January 27, 2032.

Orbital insertion on Ganymede

In September 2032, JUICE will enter an elliptical orbit around Ganymede, becoming the first spacecraft to orbit a moon other than Earth's. The first orbit will be at a distance of 5,000 km. In February 2033 JUICE will enter a circular orbit 500 km above the surface of Ganymede. JUICE will study Ganymede's composition and magnetosphere among other things.

Planned deorbit on Ganymede

When the spacecraft consumes its propellant, JUICE is planned to be deorbited and impact Ganymede in February 2034.[citation needed]

Science objectives

Ganymede view by Galileo
Section of Europa's icy surface

The Jupiter Icy moons Explorer orbiter will perform detailed investigations on Ganymede and evaluate its potential to support life. Investigations of Europa and Callisto will complete a comparative picture of these Galilean moons.[11] 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:[11]

  • 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 out for several minor irregular satellites and the volcanically active moon Io.

Spacecraft

Design drivers

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.[12]

Gravity assists include:[1]

  • 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

Ganymede Lander

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.[13] 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.[13]

Science instruments

On 21 February 2013, after a competition, 11 science instruments were selected by ESA, which are being developed by science and engineering teams from all over Europe, with participation from the US.[14][15][16][17] Japan will also contribute several components for SWI, RPWI, GALA, PEP, JANUS and J-MAG instruments, and will facilitate testing.[18][19]

Instrument name Abbr. Description and scientific objectives
Jovis, Amorum ac Natorum Undique Scrutator JANUS A camera system to 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.
Moons And Jupiter Imaging Spectrometer MAJIS 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 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. Resolution up to 0.5 km (0.3 mi) observing Ganymede and up to 250 km (155.3 mi) observing Jupiter.
Sub-millimeter Wave Instrument SWI 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.
GAnymede Laser Altimeter GALA 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.
Radar for Icy Moons Exploration RIME An ice-penetrating radar working at frequency of 9 MHz (1 and 3 MHz bandwidth) emitted by a 16 m (52.5 ft) antenna; 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.
JUICE MAGnetometer J-MAG Will study the subsurface oceans of the icy moons and the interaction of Jovian magnetic field with the magnetic field of Ganymede using a sensitive magnetometer.
Particle Environment Package PEP 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.
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.
Gravity & Geophysics of jupiter and Galilean Moons 3GM 3GM is a radio science package comprising a Ka transponder and an ultrastable oscillator.[20] 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.
Planetary Radio Interferometer & Doppler Experiment PRIDE The experiment will generate specific signals transmitted by JUICE's antenna and received by Very Long Baseline Interferometry to perform precision measurements of the gravity fields of Jupiter and its icy moons.

Targets

See also

References

  1. ^ a b c "JUICE (JUpiter ICy moons Explorer)" (PDF). European Space Agency. March 2012. Retrieved 18 July 2013.
  2. ^ Pultarova, Tereza (24 March 2017). "Europe's Jupiter explorer mission moves to prototype production". SpaceNews. Retrieved 25 March 2017.
  3. ^ Amos, Jonathan (9 December 2015). "Juice mission: Deal signed to build Jupiter probe". BBC News.
  4. ^ "JUICE's journey to Jupiter". ESA. 16 February 2017.
  5. ^ "ESA—Selection of the L1 mission" (PDF). 17 April 2012.
  6. ^ a b "Esa selects 1bn-euro Juice probe to Jupiter". Jonathan Amos. BBC News Online. 2 May 2012.
  7. ^ JUICE (JUpiter ICy moons Explorer): a European-led mission to the Jupiter system
  8. ^ "JUICE: Europe's next mission to Jupiter?". Emily Lakdawalla. The Planetary Society. 18 April 2012.
  9. ^ "Disappointed astronomers battle on". Jonathan Amos. BBC News Online. 19 April 2012.
  10. ^ "Preparing to build ESA's Jupiter mission". ESA. ESA. 17 July 2015.
  11. ^ a b "JUICE—Science objectives". European Space Agency. 16 March 2012. Retrieved 20 April 2012.
  12. ^ "JUICE—Spacecraft". European Space Agency. 16 March 2012. Retrieved 20 April 2012.
  13. ^ a b "Russia funds a proposal to land on Jupiter's moon Ganymede". Russianspaceweb. Archived from the original on 30 July 2015. Retrieved 25 August 2015.
  14. ^ "ESA chooses instruments for its Jupiter Icy Moon Explorer". CSW. ESA. 21 February 2013. Retrieved 17 June 2013.
  15. ^ "JUICE science payload". ESA. 7 March 2013. Retrieved 24 March 2014.
  16. ^ "The JUICE Instruments". CNES. 11 November 2013. Retrieved 24 March 2014.
  17. ^ "Jupiter Icy Moons Explorer (JUICE): Science objectives, mission and instruments" (PDF). 45th Lunar and Planetary Science Conference (2014). Retrieved 24 March 2014.
  18. ^ Current Status of Japanese Participation to Jupiter Icy Moons Explorer "JUICE". Saito, Y.; Sasaki, S.; Kimura, J.; Tohara, K.; Fujimoto, M.; Sekine, Y. AGU Fall Meeting Abstracts. Published on December 2015. Bibcode: 2015AGUFM.P11B2074S
  19. ^ [1] and [2] - Japan's contributions to JUICE instruments (in Japanese).
  20. ^ Shapira, Aviv; Stern, Avinoam; Prazot, Shemi; Mann, Rony; Barash, Yefim; Detoma, Edoardo; Levy, Benny (2016). "An Ultra Stable Oscillator for the 3GM experiment of the JUICE mission". 2016 European Frequency and Time Forum (EFTF). pp. 1–5. doi:10.1109/EFTF.2016.7477766. ISBN 978-1-5090-0720-2.
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