Oort Cloud


Oort's cloud is actually a belt to which the Milky Way belongs. It was first described by astronomer Jan Oort in 1950. Through the Oort Cloud we can find the limit of the Solar System. That is, the edge of the Oort Cloud is the edge of the Solar System. Most comets form in the Oort Cloud and are thought to have billions of begging bodies. It consists of two regions, which are called: an internal disk-shaped cloud and an Oort outer spherical cloud. So far no one was able to send in the perfect solution, which is not strange. The mass of the Oort outer cloud is approx. 3 × 10 ^ 25 kilograms.