
All planets....around the Sun at different speeds билимленд пж


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Ответ revolve
можно 5 звезд это для получения нового уровня



Certainly! All planets in our solar system orbit the Sun, but they do so at different speeds. This phenomenon is a result of Kepler's laws of planetary motion and is primarily determined by two factors:
Orbital Radius: The distance of a planet from the Sun is a significant factor in determining its orbital speed. According to Kepler's laws, planets closer to the Sun have shorter orbital periods and thus move faster in their orbits. Conversely, planets farther from the Sun have longer orbital periods and move more slowly.
Mass of the Sun: The gravitational force that the Sun exerts on each planet depends on its mass. A more massive Sun exerts a stronger gravitational pull, causing planets to move faster in their orbits.
Here's a basic overview of the orbital speeds of some of the planets in our solar system:
Mercury: The closest planet to the Sun, Mercury, has the shortest orbital period and the highest orbital speed. It completes one orbit roughly every 88 Earth days.
Venus: Venus is the second planet from the Sun and has an orbital period of about 225 Earth days.
Earth: Earth takes approximately 365.25 days to orbit the Sun, giving it an orbital speed of about 29.78 kilometers per second (km/s).
Mars: Mars is the fourth planet from the Sun and has an orbital period of roughly 687 Earth days.
Jupiter: Being much farther from the Sun, Jupiter has a longer orbital period of about 11.86 Earth years.
Saturn: Saturn, another distant planet, takes about 29.46 Earth years to complete one orbit around the Sun.
Uranus: Uranus, even farther from the Sun, has an orbital period of approximately 84 Earth years.
Neptune: Neptune, the farthest planet in our solar system, takes about 164.8 Earth years to complete its orbit.
These variations in orbital speed and period are due to the intricate gravitational interactions between the Sun and each planet, as described by Kepler's laws of planetary motion and Newton's law of universal gravitation.


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