well the belt of rocks and dust past pluto is called the Kupiter belt, where the suns magnetic field weakens and terminal shock occurs and hello pause, where the suns solar wind slows to sub sonic speeds
That would be the "Oort Cloud" of comets.
Comets primarily originate from two regions of the solar system: the Kuiper Belt and the Oort Cloud. The Kuiper Belt is a disc-shaped region beyond Neptune, containing many icy bodies, while the Oort Cloud is a hypothetical, spherical shell of icy objects that surrounds the solar system at a much greater distance. When gravitational perturbations occur, these icy bodies can be nudged inward, leading to their appearance as comets.
Comets originate from the Oort cloud, a spherical shell of icy bodies at the outer edges of our solar system. These comets can be perturbed and sent into the inner solar system where they become visible as they approach the Sun.
The icy cloud surrounding our solar system is known as the Oort Cloud. It is a vast, spherical shell composed of icy bodies and debris, believed to extend from about 2,000 to 100,000 astronomical units from the Sun. This region is thought to be the source of long-period comets that enter the inner solar system. The Oort Cloud remains theoretical, as it has not been directly observed, but its existence is supported by models of solar system formation and dynamics.
The spherical region of comets on the outer edges of the solar system is known as the Oort Cloud. It is believed to be a vast, hypothetical cloud of icy bodies that extends far beyond the orbit of Pluto, serving as a source for long-period comets. The Oort Cloud is thought to contain trillions of comets, which are remnants from the early solar system. Its exact boundaries and composition remain largely theoretical, as it has not been directly observed.
The Oort Cloud of comets.
Oort cloud
The Oort Cloud
This is the Kuiper Belt. It is located just beyond Pluto. There is also the Oort Cloud that surrounds the whole solar system.
That would be the "Oort Cloud" of comets.
Comets primarily originate from two regions of the solar system: the Kuiper Belt and the Oort Cloud. The Kuiper Belt is a disc-shaped region beyond Neptune, containing many icy bodies, while the Oort Cloud is a hypothetical, spherical shell of icy objects that surrounds the solar system at a much greater distance. When gravitational perturbations occur, these icy bodies can be nudged inward, leading to their appearance as comets.
The outer Oort cloud. (The inner Oort cloud is believed to be disk-shaped.)
Comets originate from the Oort cloud, a spherical shell of icy bodies at the outer edges of our solar system. These comets can be perturbed and sent into the inner solar system where they become visible as they approach the Sun.
The icy cloud surrounding our solar system is known as the Oort Cloud. It is a vast, spherical shell composed of icy bodies and debris, believed to extend from about 2,000 to 100,000 astronomical units from the Sun. This region is thought to be the source of long-period comets that enter the inner solar system. The Oort Cloud remains theoretical, as it has not been directly observed, but its existence is supported by models of solar system formation and dynamics.
The spherical region of comets on the outer edges of the solar system is known as the Oort Cloud. It is believed to be a vast, hypothetical cloud of icy bodies that extends far beyond the orbit of Pluto, serving as a source for long-period comets. The Oort Cloud is thought to contain trillions of comets, which are remnants from the early solar system. Its exact boundaries and composition remain largely theoretical, as it has not been directly observed.
The Oort cloud is thought to have formed from leftover material from the early solar system. Gravitational interactions with nearby stars and the giant planets may have scattered these icy bodies to the distant reaches of the solar system, forming the spherical Oort cloud.
The spherical region that surrounds the solar system and extends almost halfway to the nearest star is known as the heliosphere. It is formed by the solar wind, a stream of charged particles released by the Sun, which creates a bubble-like structure in the interstellar medium. The heliosphere acts as a protective barrier against cosmic radiation and interstellar particles. Its boundary, called the heliopause, marks the transition between solar and interstellar space.