International audienceThe analysis of light scattered by dust in planetary and cometary atmospheres, by interplanetary dust and by regolith on small body surfaces, can provide some information on the physical properties of the grains, mainly their nature, size and porosity. Many remote sensing observations of these bodies have been conducted from telescopes on the ground and from space. A laboratory data base is needed to interpret such measurements, for various kinds of irregularly shaped dust grains. This is the aim of the PROGRA2 project, for deposited and free-floating particles. The PROGRA2 concept encompasses a suite of five instruments carrying out measurements at different wavelengths between 540 and 1500 nm: PROGRA2-VIS (visible do...