The first images from the Webb telescope reveal the Universe as it has never been seen before.
@NASA, ESA, CSA, and STScI
The dawn of a new era in astronomy has begun as the world discovers for the first time the full capabilities of the NASA/ESA/CSA James Webb Space Telescope (JWST). The telescope's first color images and spectroscopic data, which reveal a spectacular array of previously elusive cosmic features, were released on July 12, 2022.
Stars and planets are formed from interstellar matter in galaxies. The densest parts of interstellar clouds collapse to form protostars surrounded by disks. These « protoplanetary disks » are the nurseries for planetary systems. The dynamics, density structure, temperature, chemical composition, dust-to-gas ratio in interstellar clouds and disks are key ingredients to determine the initial conditions of stars and planets, and the evolution of the new protostars and protoplanets in their native disk. The unprecedented performances and instrumental capabilities of the JWST will allow an incredible jump in the observations from the interstellar medium to disks and exoplanets.
MIRI during ambient temperature alignment testing in RAL Space's clean rooms at STFC's Rutherford Appleton Laboratory. Credit: Science and Technology Facilities Council (STFC, UK)
A suite of 4 instruments is located at the focal plane of the telescope:
Two astrophysical laboratories members of the P2IO LabEx, Irfu-DAp and IAS, are members of the MIRI consortium. MIRI offers a suite of versatile observing capabilities including imaging, low and moderate resolution spectroscopy and coronagraph.The French participation in MIRI is focused on the imager, under the technical and scientific management of Irfu-DAp. CNES is responsible to ESA for the French contribution.
Paris-Saclay teams working on extraterrestrial matter (from Irfu-Dap, IAS and IJCLab in the P2IO Labex, and also ISMO and Maison de la Simulation) have come together to propose a project in order to prepare for the interpretation of the JWST observations. The goal is to bring a complete understanding of the different physical processes, at micro and macro scales and in relation with the dynamics and the physical and chemical properties, which are acting in the evolutionary sequence from the interstellar medium to the formation of planets.
The project is organized in three scientific work packages: