Ceres' mean orbital velocity is about 17.9 kilometers per second.
The escape velocity of Ceres is approximately 2,650 miles per hour (mph). This value reflects the minimum speed an object must reach to break free from Ceres' gravitational pull without any additional propulsion. Due to its relatively small size and mass compared to larger celestial bodies, Ceres has a lower escape velocity.
The diameter of Ceres is 2,232 miles.
The Sun is vastly larger than Ceres. The Sun's diameter is about 1.39 million kilometers, while Ceres, the largest object in the asteroid belt, has a diameter of about 940 kilometers. This means the Sun is roughly 1,480 times wider than Ceres. In terms of volume, the Sun is about 1.3 million times larger than Ceres.
The Axial tilt of the dwarf planet Ceres is about 3°
Ceres, the largest object in the asteroid belt, has an orbital eccentricity of approximately 0.08. This value indicates that its orbit is slightly elliptical, but not highly elongated. Compared to other celestial bodies, this eccentricity is relatively low, meaning Ceres' orbit is close to being circular.
4 years 220 days
Ceres has a rotation period of 0.3781 days, and an orbital period of 4.6 years.
The escape velocity of Ceres is approximately 2,650 miles per hour (mph). This value reflects the minimum speed an object must reach to break free from Ceres' gravitational pull without any additional propulsion. Due to its relatively small size and mass compared to larger celestial bodies, Ceres has a lower escape velocity.
471 kilometers.
The diameter of Ceres is 2,232 miles.
The Sun is vastly larger than Ceres. The Sun's diameter is about 1.39 million kilometers, while Ceres, the largest object in the asteroid belt, has a diameter of about 940 kilometers. This means the Sun is roughly 1,480 times wider than Ceres. In terms of volume, the Sun is about 1.3 million times larger than Ceres.
Ceres has an average radius of about 470 kilometers; Earth's radius is about 6371 kilometers.
Yes, Ceres orbits the sun, but at 10% off axis and a slightly more elliptical orbit than normal for planets (It is a dwarf planet). Orbital revolution takes 4.6 years.
The gravitational field at the surface is: For Ceres: 0.28 meters per second squared For Earth: 9.8 meters per second squared
The Axial tilt of the dwarf planet Ceres is about 3°
Ceres, the largest object in the asteroid belt, has an orbital eccentricity of approximately 0.08. This value indicates that its orbit is slightly elliptical, but not highly elongated. Compared to other celestial bodies, this eccentricity is relatively low, meaning Ceres' orbit is close to being circular.
The disk-shaped belt of icy particles in Pluto's orbital neighborhood is called the Kuiper Belt.