It was Kepler. It's Kepler's 3rd Law of Planetary motion.
Planets closer to the Sun, like Mercury and Venus, have shorter revolution periods because they have shorter distances to travel around the Sun. Outer planets, such as Neptune and Pluto, have longer revolution periods due to their larger orbits.
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The gas giants in our solar system—Jupiter, Saturn, Uranus, and Neptune—exhibit significant differences between their periods of rotation and revolution. Generally, gas giants have short rotation periods; for example, Jupiter completes a rotation in about 10 hours, while their revolution periods around the Sun are much longer, with Jupiter taking about 12 Earth years. This disparity is due to their large distances from the Sun and the gravitational forces involved, resulting in slower orbital speeds compared to their rapid spins. Thus, while they rotate quickly, their orbits take much longer to complete.
The relationship is described by Kepler's Third Law.
By squaring the period of revolution (earth years) in Kepler's third law, the equation balances the relationship between the orbit's distance and the time taken to complete it. This allows for a direct comparison between different planets' orbital periods and distances from the sun.
Planets closer to the Sun, like Mercury and Venus, have shorter revolution periods because they have shorter distances to travel around the Sun. Outer planets, such as Neptune and Pluto, have longer revolution periods due to their larger orbits.
The cubes of the average distances of the planets from the sun is proportional to the squares of their periods.
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The planets are not all the same distance from the Sun, which determines how far they have to travel, and how fast they are moving. Planets farther from the Sun have much longer orbits and are not moving as quickly. So their period of revolution (year) is longer.
no they are not
The gas giants in our solar system—Jupiter, Saturn, Uranus, and Neptune—exhibit significant differences between their periods of rotation and revolution. Generally, gas giants have short rotation periods; for example, Jupiter completes a rotation in about 10 hours, while their revolution periods around the Sun are much longer, with Jupiter taking about 12 Earth years. This disparity is due to their large distances from the Sun and the gravitational forces involved, resulting in slower orbital speeds compared to their rapid spins. Thus, while they rotate quickly, their orbits take much longer to complete.
The relationship is described by Kepler's Third Law.
They are the same. The Moon rotates once for each revolution around the Earth.
yes
The comets with long periods of revolution around the Sun.
Women living with each other for a prolonged periods of time tend to have periods that coincide with each other. It is proposed that pheromones are the cause of that.
Period of rotation on its axis: 23 hours 56 minutesPeriod of revolution around the sun: 365.25 days