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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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
Transcribed Image Text: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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