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Yes, spot on, good guess . .
That's Kepler's third law. He derived it empirically from Tycho's observational data, and it can be derived from Newton's law of universal gravitation.
5.2 Earth yearsExplanation: Kepler's third law, shown below, relates a planet's orbital period to its orbital radius. T is the planet's orbital period and r is its orbital radius. k is a constant that depends upon the mass of the star at the center of the solar system.soT2 = kr3When AU are used in our solar system, k is 1. To solve, cube the orbital radius, so 33 is 27. Then take the square root of the result. The square root of 27 is close to 5.2, so the period of a typical asteroid is close to 5.2 Earth years.
19.2 rE
pluto
Pluto is the planet that has the lowest orbital velocity relative to that of the earth. The orbital velocity of Pluto is 0.159.
a planet's orbital period. based off kepler's 3rd law (Wrong.)The planet's orbital radius. (Correct.)
Yes, spot on, good guess . .
That's Kepler's third law. He derived it empirically from Tycho's observational data, and it can be derived from Newton's law of universal gravitation.
Yes. T = (2pi / sqroot of GM) multiplied by the radius^3/2. A planets mass DOES NOT affect its orbital period. A planets radius DOES affect its orbital period.
5.2 Earth yearsExplanation: Kepler's third law, shown below, relates a planet's orbital period to its orbital radius. T is the planet's orbital period and r is its orbital radius. k is a constant that depends upon the mass of the star at the center of the solar system.soT2 = kr3When AU are used in our solar system, k is 1. To solve, cube the orbital radius, so 33 is 27. Then take the square root of the result. The square root of 27 is close to 5.2, so the period of a typical asteroid is close to 5.2 Earth years.
In the solar system, Mars is the 4th planet from the Sun, following right after the Earth.
You can determine the mass of any planet by astronomically determining the planet's orbital radius and period. Then calculate the required centripetal force and equate this force to the force predicted by the law of universal gravitation using the sun's mass
19.2 rE
A planet's orbital period is also known as its year.
Kepler's Second Law: The planet moves faster when it is closer to the Sun.
pluto