Yes, spot on, good guess . .
Kepler's third law of planetary motion, which states that the square of the orbital period of a planet is directly proportional to the cube of its semi-major axis or orbital radius. This relationship allows astronomers to predict the orbital periods of planets based on their distances from the sun.
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.
Kepler's 3rd law of planetary motion. It states that the square of a planets orbital period is proportional to the cube of a planets distance from a star.In mathematical notationTO2 = k*R03WhereTO = It's orbital periodRO = It's distance from the stark = A constant.
There are no planets in orbit around the Earth !. Orbiting the Sun - Pluto has the longest orbital period at 248 years - although it has now been declassified as a planet. This leaves Neptune - with an orbital period of just under 165 years.
To determine which planet is closest to the Sun based on their orbital periods, we can use 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. Generally, planets with shorter orbital periods are closer to the Sun. Without the specific values from the table, we cannot identify which planet (A, B, C, or D) is closest, but the one with the shortest orbital period would be the closest to the Sun.
Kepler's third law of planetary motion, which states that the square of the orbital period of a planet is directly proportional to the cube of its semi-major axis or orbital radius. This relationship allows astronomers to predict the orbital periods of planets based on their distances from the sun.
Planets farther from the sun have larger orbits, which means they have to travel a greater distance to complete one revolution around the sun. This larger distance results in a longer orbital period compared to planets closer to the sun. It follows Kepler's third law of planetary motion, which states that the square of a planet's orbital period is proportional to the cube of its average distance from the sun.
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.
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.
A planet's orbital radius directly affects its orbital period through Kepler's third law of planetary motion. The farther a planet is from the star it orbits, the longer its orbital period will be, assuming all other factors remain constant. This relationship is expressed mathematically as T^2 ∝ r^3, where T is the orbital period and r is the orbital radius.
As a planet moves farther from the Sun, its orbital period increases, meaning it takes longer to complete one orbit. This relationship is described by Kepler's Third Law of Planetary Motion, which states that the square of a planet's orbital period is proportional to the cube of its average distance from the Sun. Consequently, planets that are more distant from the Sun, like Neptune, have significantly longer orbital periods compared to those closer, like Mercury.
Kepler's 3rd law of planetary motion. It states that the square of a planets orbital period is proportional to the cube of a planets distance from a star.In mathematical notationTO2 = k*R03WhereTO = It's orbital periodRO = It's distance from the stark = A constant.
Jupiter's orbital period is only 1.53% less than1/7 the orbital period of Uranus.
This is known as the planets orbital period. For the Earth, this is one year.
This is known as the planets orbital period. For the Earth, this is one year.
The time a planet takes to revolve around the sun is called its orbital period.
There are no planets in orbit around the Earth !. Orbiting the Sun - Pluto has the longest orbital period at 248 years - although it has now been declassified as a planet. This leaves Neptune - with an orbital period of just under 165 years.