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The orbital period of a planet can be calculated using Kepler's Third Law, which states that the square of the orbital period is directly proportional to the cube of the semi-major axis of the orbit. For a planet with twice the mass of Earth orbiting a star with the same mass as the Sun at a distance of 1AU (Earth-Sun distance), the orbital period would be the same as Earth's, which is about 365 days.
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.
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.
The planet must be farther from the star than Earth is from the Sun. According to Kepler's third law, a longer orbital period means that the planet must be farther from its star. In fact you could work out its average distance from the star, using Kepler's law.
Because Venus has less distance to travel than the Earth and is travelling faster. With an orbital speed of 35.02 km/s and an orbital period of 224.70069 days gives an orbital distance of 679,883,169.35km The Earth has an orbital speed of 29.78 km/s (Slower than Venus) and an orbital period of 365.256 days gives an orbital distance of 939,800,765.95km
The orbital velocity of an object depends on its distance from the center of mass it is orbiting. For example, the orbital velocity of the Moon around Earth is about 1 km/s, while the orbital velocity of the International Space Station (ISS) around Earth is about 8 km/s.
870 km is its altitude according to NASA (answred bt divyansh tiwari)
it is the distance between what an object is orbiting around and the object itself in any given point
The orbital high point, or apogee, is the farthest point in an object's orbit around another body, such as a planet or star. It is the point in the orbit where the object is at its maximum distance from the body it is orbiting.
The orbital period of a planet can be calculated using Kepler's Third Law, which states that the square of the orbital period is directly proportional to the cube of the semi-major axis of the orbit. For a planet with twice the mass of Earth orbiting a star with the same mass as the Sun at a distance of 1AU (Earth-Sun distance), the orbital period would be the same as Earth's, which is about 365 days.
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.
In space, orbiting the sun. Its orbital position is fourth, between the Earth and Jupiter or, more specifically, between the Earth and the asteroid belt.
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.
You can calculate this with Kepler's Third Law. "The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit." This is valid for other orbiting objects; in this case you can replace "planet" with "satellite". Just assume, for simplicity, that the satellite orbits Earth in a circular orbit - in this case, the "semi-major axis" is equal to the distance from Earth's center. For your calculations, remember also that if the radius is doubled, the total distance the satellite travels is also doubled.
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 word orbiting is a verb. It is the present participle of orbit.
What you are referring to is known as orbiting around an object. This involves moving in a circular or elliptical path around another object, maintaining a certain distance from it. Orbital motion is commonly observed in celestial bodies like planets orbiting around the sun.