At what distance from the Sun would a planet's orbital period be 3 million years?
Makemake's orbital period is 309.88 years or 113,183 days
The orbital characteristics of the planets in our solar system include their elliptical orbits, which vary in shape and size. Most planets orbit the Sun in a plane known as the ecliptic, with a slight tilt. The distance from the Sun affects their orbital period; for instance, Mercury has a short orbital period of about 88 Earth days, while Neptune takes about 165 Earth years to complete one orbit. Additionally, the planets generally move in the same direction around the Sun, with their orbits becoming more circular as the distance from the Sun increases.
The temperature of a planet generally decreases with increasing distance from the Sun due to the inverse square law of radiation, where the intensity of sunlight diminishes with distance. Additionally, a planet's period of revolution, or orbital period, increases with distance from the Sun as described by 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. Therefore, planets that are farther from the Sun tend to have longer orbital periods and, on average, cooler temperatures.
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.
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.
Makemake's orbital period is 309.88 years or 113,183 days
The orbital characteristics of the planets in our solar system include their elliptical orbits, which vary in shape and size. Most planets orbit the Sun in a plane known as the ecliptic, with a slight tilt. The distance from the Sun affects their orbital period; for instance, Mercury has a short orbital period of about 88 Earth days, while Neptune takes about 165 Earth years to complete one orbit. Additionally, the planets generally move in the same direction around the Sun, with their orbits becoming more circular as the distance from the Sun increases.
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.
The square of the time period of revolution is directly proportional to the cube of the mean distance between the planet and its Sun. T2 α R3T = Time Period R = Length of the semi-major axis
The temperature of a planet generally decreases with increasing distance from the Sun due to the inverse square law of radiation, where the intensity of sunlight diminishes with distance. Additionally, a planet's period of revolution, or orbital period, increases with distance from the Sun as described by 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. Therefore, planets that are farther from the Sun tend to have longer orbital periods and, on average, cooler temperatures.
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.
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.
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.
This depends on the mass of the planet (and sun or star that it orbits around) and the distance between the two. See Kepler's laws of planetary motion.
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.