Yes, the square of the orbital period of a planet is proportional to the cube of the average distance of the planet from the Sun. This relationship is known as Kepler's Third Law of Planetary Motion. It describes the mathematical relationship between a planet's orbital period and its average distance 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.
The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
Not totally true.
The orbital period of a planet can be calculated using Kepler's third law: P^2 = a^3 where P is the orbital period in years and a is the semi-major axis in astronomical units. For a planet with an average distance of 10 au, its orbital period would be approximately 31.6 years.
The orbit time of planets increases as the distance from the sun increases. 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.
The distance of a planet from the sun affects its orbital period. Generally, the farther a planet is from the sun, the longer its orbital period will be. This relationship is described by Kepler's third law of planetary motion, which states that the square of a planet's orbital period is directly proportional to the cube of its average distance 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 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.
The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
Not totally true.
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.
To determine the orbital period of a planet at an average distance of 33 AU from the Sun, we can use Kepler's Third Law of Planetary Motion, which states that the square of the orbital period (P) in years is proportional to the cube of the semi-major axis (a) in astronomical units: ( P^2 = a^3 ). For a planet at 33 AU, we calculate ( P^2 = 33^3 ), which gives ( P^2 = 35,937 ). Taking the square root, ( P ) is approximately 189.7 years. Thus, the orbital period of the planet would be about 190 years.
There is a direct relationship between the time for one complete orbit (orbital period) and the distance from the sun (orbital radius). This relationship is described by Kepler's third law of planetary motion, which states that the square of the orbital period of a planet is proportional to the cube of its average distance from the sun. In simple terms, planets farther from the sun take longer to complete their orbits.
To calculate the orbital period of Mercury, you can use Kepler's Third Law of Planetary Motion, which states that the square of the orbital period (P) of a planet is directly proportional to the cube of the semi-major axis (a) of its orbit. The formula is ( P^2 = a^3 ), where P is the period in Earth years and a is the average distance from the sun in astronomical units (AU). For Mercury, you would substitute ( a = 0.39 ) AU into the equation, yielding ( P^2 = (0.39)^3 ), and then take the square root to find the orbital period. This results in an approximate orbital period of 0.24 Earth years, or about 88 Earth days.
No it is not true. The second variable is the cube of the semi-major axis.
Johannes Kepler stated the relationship in his third law of planetary motion. This law, formulated in the early 17th century, describes the relationship between a planet's orbital period and its average distance from the sun.
The orbital period of a planet can be calculated using Kepler's third law: P^2 = a^3 where P is the orbital period in years and a is the semi-major axis in astronomical units. For a planet with an average distance of 10 au, its orbital period would be approximately 31.6 years.