Johannes Kepler, working with the detailed observational data compiled by Tycho Brahe, showed that the ratio of (orbital period)2 to (mean distance from the sun)3 is a constant for the earth and the five other visible planets. A generation after Kepler, Sir Isaac newton showed that his law of universal gravitation could predict the shape and periods of the planetary orbits.
Because Venus has less distance to travel than the Earth and is travelling faster. With an orbital speed of 35.02 km/s and an orbital period of 224.70069 days gives an orbital distance of 679,883,169.35km The Earth has an orbital speed of 29.78 km/s (Slower than Venus) and an orbital period of 365.256 days gives an orbital distance of 939,800,765.95km
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The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
5
It would depend on the star it was orbiting. If it were in our solar system, its orbital period would be little more than 30 years. (Saturn is approximately 9.5 AU from the Sun.)
Temperature and orbital period.
Temperature and orbital period.
At what distance from the Sun would a planet's orbital period be 3 million years?
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Because Venus has less distance to travel than the Earth and is travelling faster. With an orbital speed of 35.02 km/s and an orbital period of 224.70069 days gives an orbital distance of 679,883,169.35km The Earth has an orbital speed of 29.78 km/s (Slower than Venus) and an orbital period of 365.256 days gives an orbital distance of 939,800,765.95km
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F is directly porportional to P
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.
Yes, the equation p2 = a3, where p is a planet's orbital period in years and a is the planet's average distance from the Sun in AU. This equation allows us to calculate the mass of a distance object if we can observe another object orbiting it and measure the orbiting object's orbital period and distance.
The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.