European involvement in the Juno mission
June 29, 2016

European involvement in the Juno mission (Europlanet 2020 Press Release EPN PR16/6)
29 June 2016

NASA’s Juno mission will arrive at Jupiter and begin its orbit insertion manoeuvre at 4:18 am BST (5:18 am CEST) on the morning of 5th July 2016. Juno’s goals are to study Jupiter’s gravitational field, inner structure, deep atmospheric composition and magnetic environment in order to understand the origin and evolution of the giant planet. Europe has provided instrumentation for the mission and European scientists from Italy, France, Belgium, the UK and Denmark are part of the team of co-investigators that will help analyse data sent back by Juno. Amateur and professional scientists from across Europe are also involved in campaigns using ground- and space-based telescopes that will study Jupiter at a range of wavelengths to put Juno’s close-up observations into context.

The Italian contribution to Juno includes the JIRAM (Jovian InfraRed Auroral Mapper) instrument, which will study Jupiter’s atmosphere in and around the planet’s auroras, and the KaTS (Ka-Band Translator System) instrument, which will allow the acquisition of highly precise velocity measurements for Juno’s Gravity Science experiments.  France contributed to the construction of three particle spectrometers for Juno’s JADE experiment, which will help to characterise the speed and energy of populations of particles in the electrically charged plasma that fills the Jovian magnetosphere and ultimately produce its strong aurora. Belgium provided the scan mirror mechanism for Juno’s Ultraviolet Imaging Spectrograph (UVS) instrument, which will enable UVS to investigate specific features in Jupiter’s auroras. Denmark has provided star trackers that enable Juno’s magnetometer to determine its orientation in space.

Italian scientists will help to understand Jupiter’s magnetosphere and its interaction with the planet, and in particular to study the infrared auroras. They will also participate in gravity experiments to determine the wind depth and the mass of Jupiter’s core that is made up by heavy elements.

French astronomers are involved in the study of Jupiter’s magnetosphere, atmosphere and interior. French scientists also coordinate, on behalf of Juno’s magnetospheric working group, world-wide ground-based observations of Jupiter’s intense and complex radio emissions.

Belgian scientists are collaborating on ultraviolet and infrared observations of Jupiter and will be coordinating an international team that will use the Hubble Space Telescope (HST) to observe Jupiter’s ultraviolet auroras during the one-year life of the Juno mission. This is one of the biggest HST observation programmes of a Solar System object ever granted.

UK astronomers are involved in studies of Jupiter’s magnetosphere, dynamic atmosphere and its polar auroras. They have coordinated HST observations of the effect of the solar wind on Jupiter’s auroras during Juno’s cruise phase to the giant planet.

Full details of the European involvement in the Juno mission and ground support campaign can be found at:

http://www.europlanet-eu.org/juno-europe/

About Juno

JPL manages the Juno mission for the principal investigator, Dr. Scott Bolton, of Southwest Research Institute in San Antonio. The Juno mission is part of the New Frontiers Program managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama for the agency’s Science Mission Directorate. Lockheed Martin Space Systems, in Denver, built the spacecraft. JPL is a division of the California Institute of Technology in Pasadena.

More information about the Juno mission is available at: http://www.nasa.gov/juno

Juno Orbit Insertion Online Press Kit: http://www.jpl.nasa.gov/news/press_kits/juno/

Events

Details of European public events relating to the arrival of Juno at Jupiter can be found here:

http://www.europlanet-eu.org/news/juno-outreach-events/

Links:

JIRAM Instrument:

http://www.iaps.inaf.it/solarsystem/jiram/

Radio Science Laboratory, Sapienza University of Rome: http://radioscience.dima.uniroma1.it/about.php

CNRS Article on Juno: https://news.cnrs.fr/articles/juno-to-unlock-jupiters-secrets

IRAP: http://www.irap.omp.eu/en/actualites/tir-juno

Juno-Ground-Radio website:

http://maser.lesia.obspm.fr/tools-services/juno-ground-radio/juno-decametric-observations.html

Centre Spatial de Liège Juno webpage: http://www.csl.ulg.ac.be/jcms/c_8374/en/juno

University of Liège’s Laboratory for Planetary and Atmospheric Physics (LPAP) Juno webpage: http://www.lpap.ulg.ac.be/Juno

University of Leicester Jupiter webpage: http://www2.le.ac.uk/offices/press/for-journalists/juno

Leicester to Jupiter: The Juno Mission: http://staffblogs.le.ac.uk/leicester-to-jupiter/

DTU Space, Technical University of Denmark: http://www.space.dtu.dk/english/Research/Instruments_Systems_Methods/Stellar_navigation

Animation

Trailer for upcoming Europlanet animation on ‘Jupiter and its Icy Moons’, featuring the Juno and JUICE missions:

https://www.youtube.com/watch?v=ILtXyvqyBFc&index=2&list=PLPXeplhp1d00cvLIkYDoJpMalCD4jQSEJ

Media Contacts

Anita Heward
Europlanet Media Centre
Tel: +44 7756 034243
anita.heward@europlanet-eu.org

Italy
Francesco Rea
Agenzia Spaziale Italiana (ASI)
Rome, Italy
francesco.rea@asi.it

Marco Galliani
Istituto Nazionale Di Astrofisica
Rome, Italy
marco.galliani@inaf.it

Livia Giacomini
Istituto Nazionale Di Astrofisica
Rome, Italy
livia.giacomini@iaps.inaf.it

Alessandra Bomben
Sapienza University of Rome
alessandra.bomben@uniroma1.it

France

Marc Fulconis
Observatoire de la Côte d’Azur
+33 06 89 66 65 56
marc.fulconis@oca.eu

Frédérique Auffret
Observatoire de Paris
+33 (0)6 22 70 16 44
presse.communication@obspm.fr

CNRS press office
+33 (0)1 44 96 51 51
presse@cnrs.fr

Belgium

Marie Liégeois
Université de Liège
+32 (0)4 366 52 11
+32 (0)494 16 09 83
marie.liegeois@ulg.ac.be

UK

Peter Thorley
University of Leicester
+44 (0)116 252 2415
pt91@le.ac.uk
www.le.ac.uk

Denmark

Morten Garly Andersen
DTU SPACE
National Space Institute
+45 29 62 23 05 (mobile)
mga@space.dtu.dk