Yes, the larger the mass, the stronger the orbit, because for that much mass the orbit has to be strong; otherwise, it would float out deep into Dark Matter.
The time it takes for planets to orbit the Sun, known as their orbital period, is influenced by their distance from the Sun and their speed. According to Kepler's Third Law of Planetary Motion, a planet's orbital period increases with the distance from the Sun; the farther a planet is, the longer it takes to complete one orbit. Additionally, gravitational forces between the planet and the Sun affect the planet's velocity, contributing to the time required for each orbit. Therefore, larger distances and slower speeds result in longer orbital periods.
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.
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.
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.
The time it takes for a planet to orbit the sun is known as its orbital period. The order of planets from shortest to longest orbital period is: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Mercury has the shortest orbital period of about 88 Earth days, while Neptune has the longest orbital period of about 165 Earth years.
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 time it takes for planets to orbit the Sun, known as their orbital period, is influenced by their distance from the Sun and their speed. According to Kepler's Third Law of Planetary Motion, a planet's orbital period increases with the distance from the Sun; the farther a planet is, the longer it takes to complete one orbit. Additionally, gravitational forces between the planet and the Sun affect the planet's velocity, contributing to the time required for each orbit. Therefore, larger distances and slower speeds result in longer orbital periods.
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.
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 also known as its year.
In a two-planet system, when one planet is closest to its star and moving fastest (maximized velocity), the other planet is farthest away and moving slowest. This can affect the period of the two planets in their orbits, potentially leading to variations in their orbital time intervals.
The time a planet takes to revolve around the sun is called its orbital period.
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.
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.
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.