Kuiper belt
thats all i know
Comets are classified based on the length of their orbital period and their origin. Short-period comets have orbital periods less than 200 years, while long-period comets have longer orbital periods. Comets can also be classified based on their composition and physical characteristics, such as size and brightness.
Comets with short orbital periods are typically located in the inner solar system, closer to the Sun. These comets may have originated in the Kuiper Belt or the scattered disc and have been deflected into shorter, more frequent orbits due to gravitational interactions with the outer planets.
Long-period comets have periods of over 200 years.The longest would probably be somewhere around a million years (comparable to the orbital periods of objects in the Oort cloud); much longer than that, and it will go away far enough to be captured by the gravitational field of other stars.
No. At the extremity of a comet's orbit (farthest point from the sun) it is moving very slowly (for an interstellar object). But it cannot quite escape the sun's gravity, so it begins to fall back in toward the sun. It is accelerating constantly from that point on until it swings around the sun, when it is moving at it's fastest. Then, as it heads back out into space on it's orbit, it is slowly and steadily slowing down, and the whole cycle repeats.
It's almost impossible to give a definitive answer. Some comets only have short orbital periods (less than 300 years), while others have been calculated to take thousands of years to return close to the Earth ! As an example, Halley's comet returns roughly every 76 years (last time was in 1986, the next time will be around 2062). At the other end of the scale, comet McNaught is estimated to take around 92,000 years to travel once around the sun !
Comets are classified based on the length of their orbital period and their origin. Short-period comets have orbital periods less than 200 years, while long-period comets have longer orbital periods. Comets can also be classified based on their composition and physical characteristics, such as size and brightness.
Comets with short orbital periods are typically located in the inner solar system, closer to the Sun. These comets may have originated in the Kuiper Belt or the scattered disc and have been deflected into shorter, more frequent orbits due to gravitational interactions with the outer planets.
Long-period comets have periods of over 200 years.The longest would probably be somewhere around a million years (comparable to the orbital periods of objects in the Oort cloud); much longer than that, and it will go away far enough to be captured by the gravitational field of other stars.
short period comets
Comets with a return period less than 200 years are arbitrarily called short period comets.No comets are currently known with an orbital eccentricity significantly greater than 1, so they are all considered to be solar system visitors.Some from the Kuiper belt, and some from further out called the Oort Cloud.The longest period comets may have return periods of greater than 1 million years, but maybe their orbits become so perturbed by other masses in their lifetime, that they never return to Sol.
Short period comets have a period of less than 200 years Long period comets have a period of more than 200 years.
No. At the extremity of a comet's orbit (farthest point from the sun) it is moving very slowly (for an interstellar object). But it cannot quite escape the sun's gravity, so it begins to fall back in toward the sun. It is accelerating constantly from that point on until it swings around the sun, when it is moving at it's fastest. Then, as it heads back out into space on it's orbit, it is slowly and steadily slowing down, and the whole cycle repeats.
A short-term comet is typically defined as a comet with an orbital period of less than 200 years, meaning it travels around the Sun and returns relatively quickly compared to long-period comets. These comets often originate from the Kuiper Belt, a region of the solar system beyond Neptune filled with icy bodies. Their orbits can be influenced by gravitational interactions with planets, causing them to become visible from Earth more frequently. Examples of short-term comets include Comet Halley and Comet Swift-Tuttle.
It's almost impossible to give a definitive answer. Some comets only have short orbital periods (less than 300 years), while others have been calculated to take thousands of years to return close to the Earth ! As an example, Halley's comet returns roughly every 76 years (last time was in 1986, the next time will be around 2062). At the other end of the scale, comet McNaught is estimated to take around 92,000 years to travel once around the sun !
Comets can travel varying distances depending on their orbits. Some comets have orbits that take them far out into the outer solar system, while others have short-period orbits that keep them closer to the sun. Some comets can travel billions of miles during their journey through the solar system.
-- Despite where they come from, some comets have different mass qualities. While some are long-term comets, some are short-term. Short-term period comets originate in the Kuiper belt or it's "shattered disc", which is around the orbit of Neptune. Long-term period comets originate in Oort cloud, which is a cloud of icy bodies in space.
Short-period comets originate from the Kuiper Belt, a region beyond Neptune filled with icy debris, or from the scattered disk, which is a distant region beyond the Kuiper Belt. These comets have orbits that last less than 200 years and are affected by the gravity of the outer planets.