The orbital speed of a planet is the time it takes to cycle around the sun. The spinning speed of a planet is the time it takes for the planet to rotate on it's axis.
There isn't any relatonship between the orbital distance of the planet, and its rotational speed.
The planets rotate around their rotational axes and revolve around the sun.
The distance between the sun and a planet determines its orbital period, its orbital speed, and the amount of insolation. Other factors such as composition and albedo are required to determine other variables.
Rotation period refers to the time it takes for a planet or celestial body to complete one full rotation on its axis, determining the length of a day. On the other hand, the orbital period is the time it takes for a planet or celestial body to complete one full orbit around another body, such as a star. Rotation period is related to the celestial body's own spinning motion, while orbital period is related to its movement around another body.
True. Rotation refers to the spinning motion of a planet around its own axis, while orbital motion refers to the planet's movement around its star. Both types of motion are important to understand when studying celestial bodies in astronomy.
Yes, the square of the orbital period of a planet is proportional to the cube of the average distance of the planet from the Sun. This relationship is known as Kepler's Third Law of Planetary Motion. It describes the mathematical relationship between a planet's orbital period and its average distance from the Sun.
Pluto is the planet that has the lowest orbital velocity relative to that of the earth. The orbital velocity of Pluto is 0.159.
The difference between the rotation and revoulution is that rotation is the spiinning of the planet on its axis and revoulution is the orbiting of the planet around the sun.
A planet spinning on it's axis is called rotation
F is directly porportional to P
A planet's orbital period is also known as its year.
The orbital period is the time it takes for an object to complete one orbit around another object, like a planet around a star. The synodic period is the time it takes for a given object to return to the same position in the sky relative to the Sun as seen from Earth, for example the time between two consecutive similar configurations of a planet as observed from Earth.