Remote sensing for cosmic dust and other celestial bodies

The solar system is full of various small bodies such as planetary moons, main belt asteroids, Jupiter Trojans, Centaurs, trans-Neptunian objects and comets. To study them, scientists typically analyse the radiation they reflect, which is referred to as polarimetry. Scientists not only focus on the intensity of the scattered radiation, but also on how photons oscillate in the plane perpendicular to their direction of propagation – that is, their polarisation. Combining these two aspects yields significantly better descriptions than data obtained from the intensity alone.