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Kepler's Third Law definitions
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Kepler's Third Law
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Kepler's Third Law
States that the square of a planet's orbital period is proportional to the cube of the semi-major axis of its orbit.
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Terms in this set (15)
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Kepler's Third Law
States that the square of a planet's orbital period is proportional to the cube of the semi-major axis of its orbit.
Orbital Period
The time it takes for a satellite to complete one full orbit around a central body.
Semi-major Axis
The longest radius of an elliptical orbit, representing half the longest diameter.
Gravitational Constant
A fundamental constant (G) used in the calculation of gravitational forces and orbital mechanics.
Orbital Distance
The average distance from a satellite to the central body it orbits.
Mass of Central Body
The mass of the object being orbited, which influences the orbital characteristics of satellites.
SI Units
The International System of Units, a standardized system of measurement used in scientific calculations.
Proportionality
A relationship where one quantity is a constant multiple of another.
Orbital Radius
The distance from the center of the orbit to the orbiting object.
Satellite
An object that orbits a planet or other celestial body.
Ratio
A relationship between two numbers indicating how many times the first number contains the second.
Exponents
Mathematical notation indicating the number of times a number is multiplied by itself.
Kilometers
A unit of length in the metric system equal to 1,000 meters.
Seconds
The base unit of time in the International System of Units.
Rounding Errors
Small discrepancies that occur when numbers are approximated during calculations.