Université de Liège
STAR Institute

Quartier Agora
Allée du six août, 19C
B-4000 Liège

Tel.: +32(0)4.366.9774

Juno Mission

LPAP is actively involved in the NASA Juno mission

The Centre Spatial de Liege (CSL) contributed to the UVS spectrograph on board Juno

Juno spinning around Jupiter (NASA Eyes). Juno is shown with its actual spin rate (2 rotations per minute)
Higher resolution movie (8.3 Mb mov)
The steerable scan mirror of the UVS spectrograph (SwRI) developed and tested at CSL (credit: CSL/Université de Liège)

Link to the current HST campaign supporting Juno observations.

Prof Denis GRODENT is co-Investigator of the ultraviolet spectrograph UVS on board Juno. He is taking part to the analysis of the hyperspectral images of the auroral emissions of Jupiter. D. Grodent is also the Principal Investigator of the large size HST observation campaign in support to the Juno prime mission (HST GO-14634). The scientific description of this HST campaign may be found in this white paper.
Dr Bertrand BONFOND is a Juno science Team Member and assists the Principal Investigator in the detailed planning of the auroral observations. In addition, B. Bonfond is directly involved in the processing and interpretation of the data of the supporting HST campaign.
Prof Jean-Claude GERARD is co-Investigator of UVS and of the Juno InfraRed Auroral Mapper (JIRAM). In that regard, J.-C. Gérard leads the comparison of ultraviolet and infrared imaging and spectroscopy from the UVS and JIRAM instruments.

The slit of the UVS spectrograph is able to scan the auroral region by taking advantage of Jupiter's rotation, Juno's spin and orbital motion, as well as of the steerable pickup mirror of UVS, built and tested at CSL. This simulation (credit: B. Bonfond, ULg) shows how the field of view (green lines) is very rapidly changing with time. In this simulation, the northern aurora is continuously observed for almost three hours prior to perijove.
Reconstruction of an image of Jupiter's aurora obtained by scanning the UVS slit across the pole (credit: D. Grodent, ULg). This simulation uses a long sequence of HST images (movie) previously obtained with the STIS camera. The simulation is combining the data obtained from 5 consecutive rotations of Juno (5 times 30 sec).
University of Liège > Faculty of Sciences > AGO Department > Laboratory for Planetary and Atmospheric Physics: D. Grodent, November 2016.