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JUICE – mission to the icy moons of Jupiter

The Jupiter Mission JUICE
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JUICE-Mission zu den Eismonden des Jupiters
22 February 2013

Mission involvement for the German Aerospace Center

Last week, the European Space Agency (ESA) announced its choice of scientific experiments for the JUICE Mission (JUpiter ICy moons Explorer) . The decision taken involved two experiments developed by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) Institute of Planetary Research.

As the first big mission in the ESA Cosmic Vision 2015-2025 programme, JUICE is scheduled to spend three years exploring the Jovian system. The launch is scheduled for 2022, and the spacecraft should reach its destination in 2030, where it will make detailed observations of the largest planet in the Solar System and the Galilean satellites Io, Ganymede, Callisto and Europa. The focus here is on the oceans of water below the thick, ice-encrusted surfaces of the individual moons, accurate measurements of these satellites and their interaction with the giant 'particle accelerator' that is Jupiter and its magnetic field.

En route to the gas giant with JANUS and GALA

The payload of the JUICE spacecraft will include a total of 11 instruments, including cameras, a spectrometer, a laser altimeter and a ground radar for ice. Fifteen ESA member states as well as the United States and Japan are involved in this project. DLR will play a key role on this mission with its JANUS camera system (an acronym for Jovis, Amorum ac Natorum Undique Scrutator) and GALA (GAnymede Laser Altimeter). "This selection showcases great technological performance capability as well as recognition of DLR's outstanding international scientific standing," said Tilman Spohn, Director of the DLR Institute of Planetary Research in Berlin, as he welcomed the decision by ESA.

The JANUS camera system is being developed in a collaborative venture with Italian scientists. This camera, developed jointly by Ralf Jaumann from the DLR Institute of Planetary Research and Pasquale Palumbo, of the Università degli Studi di Napoli 'Parthenope' in Naples, will map the surface of the icy moons of Jupiter and, in the case of Ganymede, will perform a full global mapping. "In this way, we can investigate local regions of these moons that either recently were, or perhaps still may be geologically active, and can do so to a resolution of just a few metres," announced Jaumann. Recordings will also be made of changes in Jupiter's atmosphere and of possible volcanic eruptions on Io.

The second experiment, GALA, is a laser altimeter which will be used to measure the topography of Ganymede, and is capable of height readings accurate to within 15 centimetres. DLR planetary researchers, under the direction of Hauke Hussmann, with some Japanese involvement, are developing GALA. This height-measuring instrument precisely determines topographical height from elapsed time; that is, the time for a laser pulse to be transmitted to the surface of the satellite and reflected back to the spacecraft. When the flight path of the spacecraft is known, hundreds of millions of these individual measurements enable a very accurate topographic model of the moon to be built up. "This will be the first time we will have managed to produce a detailed terrain map, not an easy task given the relative absence of physical relief on Europa, Ganymede and Callisto," explained Hussmann. "Furthermore, from this data we can extrapolate information about the internal structure and the rotational characteristics of the Jovian satellites."

Admittedly, the probe's two flybys of Europa and its 12 flybys of Callisto will not be sufficient to provide complete global coverage, but nonetheless some extremely accurate topographical profiles of these satellites can be obtained. The combination of the laser altimeter, the JANUS camera and the 3GM radio wave experiment constitutes a geophysical-geodetic package that can help determine the nature of these moons, their geological activity and their internal structure.

Jupiter – an archetype among gas giants

With an equatorial diameter of approximately 143,000 kilometres, Jupiter is the largest planet in the Solar System and is therefore your typical gas giant. With its four large Galilean moons, Jupiter is a small planetary system in its own right. Below the surface of Ganymede, Europa and Callisto, scientists believe there are giant oceans of liquid water that might conceivably harbour life, as we know it. The JUICE Mission aims to gain a comprehensive understanding of the Jovian system and decipher its history and origins. As well as the conditions for planetary formation, this mission will explore the fundamental question of how the Solar System really functions. By exploring the gas giant, located almost 800 million kilometres from the Sun, and by finding out more about its satellites, scientists hope to be able to draw conclusions about the origin and development of life. These insights can, in turn, help to track down life in systems similar to Jupiter beyond the Solar System.

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