It takes 140 days more for the earth to go around the sun than Venus!
The period of a planet's revolution can be used to calculate its orbital radius or distance from the sun using Kepler's third law of planetary motion. It can also be used to determine the planet's orbital speed or velocity if its mass is known. Additionally, the period of revolution helps in predicting future positions of the planet along its orbit.
The primary factors affecting orbital time are the mass of the objects involved, the distance between them, and the gravitational force between them. Orbital time increases with greater mass or distance, and decreases with stronger gravitational forces. The velocity of the objects also plays a role in determining the orbital time.
The temperature of a planet generally decreases with increasing distance from the Sun due to the inverse square law of radiation, where the intensity of sunlight diminishes with distance. Additionally, a planet's period of revolution, or orbital period, increases with distance from the Sun as described by Kepler's Third Law, which states that the square of a planet's orbital period is proportional to the cube of its average distance from the Sun. Therefore, planets that are farther from the Sun tend to have longer orbital periods and, on average, cooler temperatures.
uranus does a full revolution every 84.016846 julian years
The revolution of asteroids in the asteroid belt is typically between 2 to 6 years, depending on the specific asteroid's distance from the Sun and its orbital speed. The average distance of the asteroid belt from the Sun is about 2.2 to 3.3 astronomical units (AU), with one AU being the average distance between the Earth and the Sun.
gravity is that keeping the orbital speed from falling or breaking loose. and the distance away = time
A planets period or revolution, the time taken to orbit its star, is dependant on its mass, the stars mass and the distance between the two. See Kepler's laws of planetary motion for further information.
The period of a planet's revolution can be used to calculate its orbital radius or distance from the sun using Kepler's third law of planetary motion. It can also be used to determine the planet's orbital speed or velocity if its mass is known. Additionally, the period of revolution helps in predicting future positions of the planet along its orbit.
The primary factors affecting orbital time are the mass of the objects involved, the distance between them, and the gravitational force between them. Orbital time increases with greater mass or distance, and decreases with stronger gravitational forces. The velocity of the objects also plays a role in determining the orbital time.
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.
The temperature of a planet generally decreases with increasing distance from the Sun due to the inverse square law of radiation, where the intensity of sunlight diminishes with distance. Additionally, a planet's period of revolution, or orbital period, increases with distance from the Sun as described by Kepler's Third Law, which states that the square of a planet's orbital period is proportional to the cube of its average distance from the Sun. Therefore, planets that are farther from the Sun tend to have longer orbital periods and, on average, cooler temperatures.
The two factors that affect orbital motion are the mass of the objects involved and the distance between them. Gravitational force is stronger with larger masses and decreases as distance between objects increases.
uranus does a full revolution every 84.016846 julian years
Because it has an orbital speed of 47.87 km/s and a distance of 363,837,382.6 km to cover in one revolution.
The revolution of asteroids in the asteroid belt is typically between 2 to 6 years, depending on the specific asteroid's distance from the Sun and its orbital speed. The average distance of the asteroid belt from the Sun is about 2.2 to 3.3 astronomical units (AU), with one AU being the average distance between the Earth and the Sun.
The relationship between the distance from the sun and the speed of revolution of the planets is described by Kepler's laws of planetary motion. Specifically, the further a planet is from the sun, the slower its orbital speed tends to be. This is because gravitational force weakens with distance, resulting in a longer orbital period and reduced speed for planets farther out in the solar system. Thus, inner planets like Mercury and Venus revolve around the sun much faster than outer planets like Neptune and Pluto.
There is no real relationship, a planets spin depends on collisions it may have had in the past, rather than on its distance from the sun (which governs its orbital rotation time around the sun).