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If a planet had an average distance of 10 au what would it's orbital period be?
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.
An object has been located orbiting the sun at a distance from the sun of 65 AU what is the approximate orbital period of this object?
The approximate orbital period of an object at a distance of 65 AU from the sun would be around 177 years. This corresponds to Kepler's third law of planetary motion, which relates the orbital period of a planet to its distance from the sun.
Is the square of the orbital period of a planet proportional to the cube of the average distance of the planet from the Sun?
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.
The relationship between the average distance of a planet from the sun and the planets orbital period is described by what?
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.
Which properties can be inferred from the stars orbital period?
From a star's orbital period, we can infer its distance from the object it is orbiting (based on Kepler's third law), the system's total mass (by combining other observable parameters), and potentially the star's luminosity and size if additional information is available. The orbital period can also give insights into the stability of the system and the potential presence of other planets or companions.
What effect has distance of a planet to the sun to its orbital period?
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.
If a planet had an average distance of 10 au what would it's orbital period be?
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.
An object has been located orbiting the sun at a distance from the sun of 65 AU what is the approximate orbital period of this object?
The approximate orbital period of an object at a distance of 65 AU from the sun would be around 177 years. This corresponds to Kepler's third law of planetary motion, which relates the orbital period of a planet to its distance from the sun.
At what distance from the Sun would a planets orbital period be 3 million years?
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.
Is the square of the orbital period of a planet proportional to the cube of the average distance of the planet from the Sun?
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.
The relationship between the average distance of a planet from the sun and the planets orbital period is described by what?
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.
Which properties can be inferred from the stars orbital period?
From a star's orbital period, we can infer its distance from the object it is orbiting (based on Kepler's third law), the system's total mass (by combining other observable parameters), and potentially the star's luminosity and size if additional information is available. The orbital period can also give insights into the stability of the system and the potential presence of other planets or companions.
A planet is detected via the Doppler technique The repeating pattern of the stellar motion tells us?
The repeating pattern of the stellar motion reveals the presence of a planet orbiting the star. By analyzing the variations in the star's radial velocity, astronomers can determine the planet's mass, orbital period, and distance from the star. This information helps to characterize the planet and understand its orbit within the stellar system.
Which two of the planet are closely related to their distance from the sun?
Temperature and orbital period.
I used Newton's version of Kepler's third law to calculate Saturn's mass from orbital characteristics of its moon Titan?
Yes, the equation p2 = a3, where p is a planet's orbital period in years and a is the planet's average distance from the Sun in AU. This equation allows us to calculate the mass of a distance object if we can observe another object orbiting it and measure the orbiting object's orbital period and distance.
How to calculate the orbital period of a planet?
To calculate the orbital period of a planet, you can use Kepler's third law of planetary motion. The formula is T2 (42 r3) / (G M), where T is the orbital period, r is the average distance from the planet to the sun, G is the gravitational constant, and M is the mass of the sun. Simply plug in the values for r and M to find the orbital period of the planet.
Which two characteristics of the planet are closely related to their distance from sun?
Temperature and orbital period.
