kepler's third law Synonyms
No Synonyms and anytonyms found
kepler's third law Meaning
kepler's third law (n)
a law stating that the ratio of the square of the revolutionary period (in years) to the cube of the orbital axis (in astronomical units) is the same for all planets
kepler's third law Sentence Examples
- Kepler's Third Law states that the square of the orbital period of a planet is proportional to the cube of the semi-major axis of its orbit.
- The mathematical representation of Kepler's Third Law is T^2/r^3 = k, where T is the orbital period, r is the semi-major axis, and k is a constant.
- Kepler's Third Law holds for all orbits, regardless of the shape of the orbit.
- The law was first proposed by Johannes Kepler in the 16th century, based on his observations of the orbits of Mars and Jupiter.
- Kepler's Third Law was one of the key pieces of evidence that led Isaac Newton to develop his law of universal gravitation.
- Kepler's Third Law can be used to calculate the period of an object in orbit around a star, even if the mass of the star is unknown.
- The law can also be used to calculate the semi-major axis of an orbit, if the period of the orbit is known.
- Kepler's Third Law has been tested and confirmed by numerous observations of planets, moons, and artificial satellites.
- The law is also applicable to binary star systems, where two stars orbit around a common center of mass.
- Kepler's Third Law is a fundamental law of physics that governs orbital motion in our universe.
FAQs About the word kepler's third law
a law stating that the ratio of the square of the revolutionary period (in years) to the cube of the orbital axis (in astronomical units) is the same for all pl
No synonyms found.
No antonyms found.
Kepler's Third Law states that the square of the orbital period of a planet is proportional to the cube of the semi-major axis of its orbit.
The mathematical representation of Kepler's Third Law is T^2/r^3 = k, where T is the orbital period, r is the semi-major axis, and k is a constant.
Kepler's Third Law holds for all orbits, regardless of the shape of the orbit.
The law was first proposed by Johannes Kepler in the 16th century, based on his observations of the orbits of Mars and Jupiter.
