If two planets are in orbits with radii of R1 and R2, the distance between them varies from R2-R1 to R2+R1.
Keplar showed that there is a relationship between the planets distance from the sun and the time taken for one orbit (planets year). This is described in Keplars third law; the square root of the time taken to orbit the sun is proportional to the cube of the average distance between the sun.
He referred to it as an eclipse where the planets orbit the sun in a path.
The period of revolution of a planet (time taken to complete one orbit around the sun) is directly proportional to its average distance from the sun. This relationship is described by Kepler's third law of planetary motion. Planets that are farther from the sun take longer to complete an orbit compared to planets that are closer to the sun.
The distance between the inner planets (Mercury, Venus, Earth, Mars) is comparatively smaller than the distance between the outer planets (Jupiter, Saturn, Uranus, Neptune) in our solar system. The inner planets are closer to the Sun and each other, while the outer planets are much farther apart due to the gap between the terrestrial and gas giant planets.
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.
the planets
there is no true relationship between distance from the sun and orbit time as some planets go revolves at a different velocity.
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Keplar showed that there is a relationship between the planets distance from the sun and the time taken for one orbit (planets year). This is described in Keplars third law; the square root of the time taken to orbit the sun is proportional to the cube of the average distance between the sun.
There is no direct relationship between the rotation of a planet (which governs day length) and a planets distance from the sun. The nature of the planets spin is more to do with the formation of the system early on, by large impacts of the more numerous bodies that would have been around.
He referred to it as an eclipse where the planets orbit the sun in a path.
The period of revolution of a planet (time taken to complete one orbit around the sun) is directly proportional to its average distance from the sun. This relationship is described by Kepler's third law of planetary motion. Planets that are farther from the sun take longer to complete an orbit compared to planets that are closer to the sun.
There is a relationship between the planets distance from the sun and the time taken for one orbit (planets year), described in Keplers third law. The square root of the time taken to orbit the sun is proportional to the cube of the average distance between the sun.
There is no real relationship, a planets spin depends on collisions it may have had in the past, rather than on its distance from the sun (which governs its orbital rotation time around the sun).
The distance a planet is from the sun influences its year length. Planets closer to the sun have shorter years because they travel a shorter distance to complete one orbit around the sun. Conversely, planets farther from the sun have longer years because they have a greater distance to travel in their orbit.
The relationship between the planet's SPEED and its distance from the Sun is given by Kepler's Third Law.From there, it is fairly easy to derive a relationship between the period of revolution, and the distance.
The distance between the inner planets (Mercury, Venus, Earth, Mars) is comparatively smaller than the distance between the outer planets (Jupiter, Saturn, Uranus, Neptune) in our solar system. The inner planets are closer to the Sun and each other, while the outer planets are much farther apart due to the gap between the terrestrial and gas giant planets.