Want this question answered?
1) It must orbit the sun directly, and not another solar system body. (This lets out Ganymede, for example, which orbits Jupiter.)2) It must have sufficient mass to have reached hydrostatic equilibrium: a near-round shape. (This removes most asteroids, which are too small for gravity to have rounded them off.)3) It must have cleared the neighborhood around its orbit. (This eliminates Ceres, because it hasn't cleared its neighborhood of other asteroids; and Pluto, because it's locked into a resonance orbit with the much-larger Neptune.)
1) It must orbit the sun directly, and not another solar system body. (This lets out Ganymede, for example, which orbits Jupiter.)2) It must have sufficient mass to have reached hydrostatic equilibrium: a near-round shape. (This removes most asteroids, which are too small for gravity to have rounded them off.)3) It must have cleared the neighborhood around its orbit. (This eliminates Ceres, because it hasn't cleared its neighborhood of other asteroids; and Pluto, because it's locked into a resonance orbit with the much-larger Neptune.)
Within the solar system, the mass of the orbiting bodies ... whether planets, asteroids, comets etc. ... has no effect on the dimensions of their orbits.
Planets are celestial bodies orbiting a star. Other things can orbit a star, so long as it has mass and the proper inertia.
The solar system has three classified dwarf planets. They are Pluto, Ceres, and Eris. A dwarf planet has sufficient mass, has not cleared the neighborhood around its orbit, and is in orbit around a star.
Orbits a star and has enough mass to have cleared its orbit of debris.
Galaxies form groups called galaxy clusters, so they would orbit the center of mass of the galaxy clusters, just as our Solar System orbits the center of mass of our galaxy.Galaxies form groups called galaxy clusters, so they would orbit the center of mass of the galaxy clusters, just as our Solar System orbits the center of mass of our galaxy.Galaxies form groups called galaxy clusters, so they would orbit the center of mass of the galaxy clusters, just as our Solar System orbits the center of mass of our galaxy.Galaxies form groups called galaxy clusters, so they would orbit the center of mass of the galaxy clusters, just as our Solar System orbits the center of mass of our galaxy.
Comet
Two objects of the same mass will also move in elliptical orbits. Whether the two bodies are of the same mass or different, one focus of the elliptical orbit is the center of mass (barycenter).
Meteors are in orbit round the Sun and they follow Kepler's 3 laws of planetary motion, which apply to anything that orbits the Sun, of any size and mass.
1) It must orbit the sun directly, and not another solar system body. (This lets out Ganymede, for example, which orbits Jupiter.)2) It must have sufficient mass to have reached hydrostatic equilibrium: a near-round shape. (This removes most asteroids, which are too small for gravity to have rounded them off.)3) It must have cleared the neighborhood around its orbit. (This eliminates Ceres, because it hasn't cleared its neighborhood of other asteroids; and Pluto, because it's locked into a resonance orbit with the much-larger Neptune.)
1) It must orbit the sun directly, and not another solar system body. (This lets out Ganymede, for example, which orbits Jupiter.)2) It must have sufficient mass to have reached hydrostatic equilibrium: a near-round shape. (This removes most asteroids, which are too small for gravity to have rounded them off.)3) It must have cleared the neighborhood around its orbit. (This eliminates Ceres, because it hasn't cleared its neighborhood of other asteroids; and Pluto, because it's locked into a resonance orbit with the much-larger Neptune.)
The gravity that keeps the planets in orbit is the sun's gravity, which is a product of the sun's mass.
The gravitational influence of mass contained within an orbit of a particular size determines the speed (and therefore period) of that orbit. So by measuring the period and size of the orbit, we can determine the mass inside the orbit. This concept works equally well for the orbits of stars and gas within spiral galaxies. By looking at the mass inside the orbit of stars or gas at different distances from the center of the galaxy, the mass of a galaxy as a function of radial distance from the center the mass of a galaxy inside radius r obtained from the rotation curve of the galaxy. What have we learned? In discussing the orbits of planets around a star, or the orbits of stars around the center of the galaxy, the mass inside the orbit determines, via gravity, the properties of the orbit. The difference here is that if you look at a bigger orbit (farther from the center), the mass inside that orbit is bigger than the mass inside the smaller orbit. We have to remember that the mass of the planets is insignificant compared to the mass of the star. I as well learned the expression for the mass enclosed within an orbit of radius r is M = v2r/G, where G is Newton's gravitational constant (and v is the orbital speed of a star at distance r. This formula is essentially another way of writing Kepler's Law Porb2 = constant * r3.)
Within the solar system, the mass of the orbiting bodies ... whether planets, asteroids, comets etc. ... has no effect on the dimensions of their orbits.
Ummmm.... No. The Moon orbits the Earth. The Earth orbits the Sun. The Sun orbits the center of the galaxy. Light things in orbit, heavier things in the center of the orbit. Well not exactly, they revolve around their common center of mass. This may or may not be at the exact center as far as distance. The common center of mass of the Moon and the Earth is located inside the earth, but not at the center of the Earth.
Planets are celestial bodies orbiting a star. Other things can orbit a star, so long as it has mass and the proper inertia.