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How to fill out 1 keplers third law

01
Understand the equation for Kepler's third law: T^2 = k*a^3, where T is the period of the orbiting object, a is the semimajor axis of the orbit, and k is a constant.
02
Measure the period of the orbiting object (T) in seconds.
03
Determine the semimajor axis of the orbit (a) in meters.
04
Square the period (T) and cube the semimajor axis (a).
05
Set up the equation T^2 = k*a^3 and solve for the constant k.
06
Fill in the values of T, a, and k to complete Kepler's third law.

Who needs 1 keplers third law?

01
Astronomers and physicists who study the motion of celestial bodies in our solar system and beyond.
02
Students learning about the laws of planetary motion in science classes.
03
Anyone interested in understanding the relationship between the period and distance of objects in orbit around a central body.
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Kepler's third law states that the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
1 Kepler's third law is a scientific principle and does not require filing.
There is no specific form to fill out for Kepler's third law as it is a mathematical principle.
The purpose of Kepler's third law is to describe the relationship between the orbital period and distance of a planet from the sun.
Kepler's third law does not involve reporting any information, but it is used to calculate the orbital period of planets.
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