Saturn orbits the Sun in an elliptical (oval) orbit, close to the solar ecliptic plane, with a minimum distance of about 1.35 billion kilometers and a maximum of 1.51 billion kilometers. It takes Saturn about 30 Earth years to make a complete orbit of the Sun. Saturn is the fifth major planet from the Sun and one of the four outer "gas giants". Saturn's atmosphere reflects most of the solar radiation that reaches it, which is considerably less than Earth receives.
They are all in orbits round the Sun, kept there by the force of gravity because the Sun is very massive and its gravity is strong.
The relationship is orbital in nature.
They're both planets.
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the planets
There is no real relationship between their diameter and distance from the sun, except that you could say that the four outer gas planets are much bigger than the four inner rocky (or terrestrial) planets.
If two planets are in orbits with radii of R1 and R2, the distance between them varies from R2-R1 to R2+R1.
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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.
the planets
the planets
there is no true relationship between distance from the sun and orbit time as some planets go revolves at a different velocity.
The difference is that the sun is a star, the other planets are just planets
There is no real relationship between their diameter and distance from the sun, except that you could say that the four outer gas planets are much bigger than the four inner rocky (or terrestrial) planets.
You have to orbit around
If two planets are in orbits with radii of R1 and R2, the distance between them varies from R2-R1 to R2+R1.
Extra solar (or Exo) planets are planets that do not orbit the Sun. Planets in our solar system orbit the Sun.
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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.
The sizes of the Sun and planets determine the strength of gravitational pull of the planets on each other and the Sun. The Sun's mass is so great that the planets can't escape from the Sun's pull and so as the planets are moving by the Sun pulls them back into orbit.