What are dispersed disk objects?

dispersed disc objects are among the most distant and colder objects in the solar system. They are located between 35 and 1,000 AU from the Sun. With an eccentricity of up to 55 degrees, some of the "vertical" are traveled due to the plane of the ecliptic, as "horizontal". Unlike most other objects in the solar system, such as planets and most asteroids, these objects have highly inclined and eccentric orbits, while circular orbits are an exception rather than a standard. Eris is classified as a dwarf planet together with Pluto, which exceeds the size and weight and Ceres, previously considered the largest asteroid. Scattered disc objects are considered to be a subgroup of Trans-Neptun objects, a roofing term used to indicate any body as the orbit of the Neptune, including Pluto.

Although the origin of the origin is not fully understood, it is assumed that the dispersion of the disk were previously members of the Kuiper belt that was thrown into the eccentric, scattered circularsH Railways through close meetings with Neptune. They have some of the coldest surfaces in the solar system, with temperatures in the range of 30 hp and 55 K. From the surface of one, the sun would look like a little more than an exceptionally bright star.

Since Pluto is about 32 au far from the Sun, scattered disc objects move from slightly distant to more than 30 times further from the Sun than Pluto. There are no closer to the Sun than 35 AU, as they would fall into the gravitational effect of Neptune and began to normalize their orbit.