Sort the characteristics according to whether they are part of the a cocentric model, the heliocentric madel, or both solar system models This model is Sun-centered. Retrograde motion is explained by the orbital speeds of planets. Epicycles and deferents help explain planetary motion. This model is Earth-centered. The brightness of a planet increases when the planet is closest to Earth. Planets move in circular orbits and with uniform motion. Retrograde motion is explained by epicycles. Geocentric Heliocentric Both geocentric and heliocentric
Sort the characteristics according to whether they are part of the a cocentric model, the heliocentric madel, or both solar system models This model is Sun-centered. Retrograde motion is explained by the orbital speeds of planets. Epicycles and deferents help explain planetary motion. This model is Earth-centered. The brightness of a planet increases when the planet is closest to Earth. Planets move in circular orbits and with uniform motion. Retrograde motion is explained by epicycles. Geocentric Heliocentric Both geocentric and heliocentric
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