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What effect has distance of a planet to the sun to its orbital period?
The distance of a planet from the sun affects its orbital period. Generally, the farther a planet is from the sun, the longer its orbital period will be. This relationship is described by Kepler's third law of planetary motion, which states that the square of a planet's orbital period is directly proportional to the cube of its average distance from the sun.
What trend can you see between the time for one complete orbit and the distance from the sun?
There is a direct relationship between the time for one complete orbit (orbital period) and the distance from the sun (orbital radius). This relationship is described by Kepler's third law of planetary motion, which states that the square of the orbital period of a planet is proportional to the cube of its average distance from the sun. In simple terms, planets farther from the sun take longer to complete their orbits.
What is the relationship between a planet's distance from the sun and the planet's period of revolution?
The relationship between the planet's SPEED and its distance from the Sun is given by Kepler's Third Law.From there, it is fairly easy to derive a relationship between the period of revolution, and the distance.
Who stated that the square of the period of revolution of a planet is proportional to the cube of its mean distance from the sun?
Johannes Kepler stated the relationship in his third law of planetary motion. This law, formulated in the early 17th century, describes the relationship between a planet's orbital period and its average distance from the sun.
What is the relationship between distance from the sun and period of revolution?
the planets
Is the square of the orbital period of a planet proportional to the cube of the average distance of the planet from the Sun?
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.
The relationship between the average distance of a planet from the sun and the planets orbital period is described by what?
Kepler's third law of planetary motion states that the square of a planet's orbital period is directly proportional to the cube of its average distance from the sun. This relationship allows us to predict the orbital period of a planet based on its distance from the sun, and vice versa.
What effect has distance of a planet to the sun to its orbital period?
The distance of a planet from the sun affects its orbital period. Generally, the farther a planet is from the sun, the longer its orbital period will be. This relationship is described by Kepler's third law of planetary motion, which states that the square of a planet's orbital period is directly proportional to the cube of its average distance from the sun.
What trend can you see between the time for one complete orbit and the distance from the sun?
There is a direct relationship between the time for one complete orbit (orbital period) and the distance from the sun (orbital radius). This relationship is described by Kepler's third law of planetary motion, which states that the square of the orbital period of a planet is proportional to the cube of its average distance from the sun. In simple terms, planets farther from the sun take longer to complete their orbits.
What is the relationship between a planet's distance from the sun and the planet's period of revolution?
The relationship between the planet's SPEED and its distance from the Sun is given by Kepler's Third Law.From there, it is fairly easy to derive a relationship between the period of revolution, and the distance.
What is the relationship between distance from the sun and period of rotation or distance from the sun and eccentricity?
The relationship between distance from the Sun and the period of rotation is 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. As for eccentricity, there isn't a direct relationship with distance; eccentricity measures the shape of an orbit, which can vary among planets at similar distances from the Sun. However, generally, planets further from the Sun tend to have more circular orbits, resulting in lower eccentricities.
Who stated that the square of the period of revolution of a planet is proportional to the cube of its mean distance from the sun?
Johannes Kepler stated the relationship in his third law of planetary motion. This law, formulated in the early 17th century, describes the relationship between a planet's orbital period and its average distance from the sun.
What does the distance between the sun and a planet determine?
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.
What is the relationship between distance from the sun and period of revolution?
the planets
At what distance from the Sun would a planets orbital period be 3 million years?
A planet's orbital period is related to its distance from the Sun by Kepler's third law, which states that the square of the orbital period is proportional to the cube of the semi-major axis of the orbit. For an orbital period of 3 million years, the planet would need to be located at a distance of approximately 367 AU from the Sun.
What relationship exists between a planet's distance from the sun and its period of revolution?
The relationship that exists between a planet's distance from the Sun and its period of revolution is that the closer the planet is from the Sun, the less amount of time it takes for the planet to complete its period of revolution.
Who figured out that the orbital period of a planet is related to its distance from the sun?
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.
