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The zodiacal light is a night-glow mostly visible along the plane of theecliptic. It represents the background radiation associated with solar lightscattered by the tenuous flattened interplanetary cloud of dust particlessurrounding the Sun and the planets. It is an interesting subject of study, asthe source of the micrometeoroids falling on Earth, as a link to the activityof the small bodies of the Solar System, but also as a foreground that veilsthe low brightness extrasolar astronomical light sources.  In this review, we summarize the zodiacal light observations that have beendone from the ground and from space in brightness and polarization at variouswavelength ranges. Local properties of the interplanetary dust particles insome given locations can be retrieved from the inversion of the zodiacal lightintegrated along the light-of-sight. We show that the current communityconsensus favors that the majority of the interplanetary dust particlesdetected at 1 au originate from the activity of comets.  Our current understanding of the interplanetary dust particles properties isthen discussed in the context of the recent results from the Rosetta rendezvousspace mission with comet 67P/Churyumov-Gerasimenko.

Zodiacal light observations and its link with cosmic dust: a review