depends on what you mean. The planets revolve by themselves and around the sun so if you mean just a rotation of a planet then no. If you mean around the sun it depends on how your thinking about it. If you're talking about 365 earth days, then no. Each planet moves at a different speed around the sun and the farther from the sun, the slower the rotation.
The mean radius of the asteroid Vesta is about 262.7 kilometers (163.2 miles).
On the off chance that you mean planet Mercury, it has a radius of about 2440 kilometers.
This is nothing to do with planets. It's part of the theory of black holes. Perhaps you mean if the planet's mass were concentrated into a black hole. In that case the answer is Jupiter, because it has the greatest mass.
s-orbital = 2e- (s) orbital can hold 2 electrons, each with opposite spin. p-orbital = 6e- (p) orbital can hold 6 electrons in 3 suborbitals, so 2 electrons in each d-orbital = 10e- (d) orbital can hold 10 electrons in 5 suborbitals, so 2 electrons in each f-orbital = 14e- (f) orbital can hold 14 electrons in 7 suborbitals, so 2 electrons in each
depends on what you mean. The planets revolve by themselves and around the sun so if you mean just a rotation of a planet then no. If you mean around the sun it depends on how your thinking about it. If you're talking about 365 earth days, then no. Each planet moves at a different speed around the sun and the farther from the sun, the slower the rotation.
It is the orbital velocity (speed and direction) or orbital speed (rate of motion). It is usually stated as "average orbital speed" but is actually "mean orbital speed."
Mercury with a mean orbital speed of 47.87 km/s
The velocity a planet travels in it's circle around the Sun
The average radius of Mars is about 3,389.5 kilometers.
An orbit is the path followed by a planet according to Kepler's laws, which are very accurate but not exact. Size, speed and period are all related by simple formulas so that if you know one you can find out the other two. The orbit is an ellipse and the size is usually measured by its mean radius, also called its semi-major axis, which is the average of the maximum and minimum distances. For the Earth that is 149.6 million kilometres. The orbital period is proportional to the mean radius to the power 1.5, while the orbital speed is inversely proportional to the square root of the mean radius.
No. With a mean radius of 2440 kilometers, Mercury is a the smallest planet in the solar system.
The mean radius of the asteroid Vesta is about 262.7 kilometers (163.2 miles).
On the off chance that you mean planet Mercury, it has a radius of about 2440 kilometers.
The square of the time period of revolution is directly proportional to the cube of the mean distance between the planet and its Sun. T2 α R3T = Time Period R = Length of the semi-major axis
This is nothing to do with planets. It's part of the theory of black holes. Perhaps you mean if the planet's mass were concentrated into a black hole. In that case the answer is Jupiter, because it has the greatest mass.
The only planet close in size to the moon is Mercury, the closest planet to the sun. The mean radius of the moon is 1737.10 km The mean radius of Mercury is 2439.7 km There are many dwarf planets that are close in size to the moon, but that would be another question.