The observation of the zodiacal light has established some of the properties of interplanetary dust present between 0.1AU and 1AU from the Sun, such as their spatial distribution, color and polarization. It has been established that the powder was more sensitive to gravitational forces and electromagnetic forces. The amount of dust was observed up to 10 times around the Earth. Heterogeneous distribution was generally expected due to the passage of comets, but observations have not confirmed this. The probe instruments detected dust near the Sun showing that, despite the sunshine is still present in distance 0.09 AU.