Planet Motion

All of the visible planets in our solar system stay within 7° of the ecliptic.


flat solar system!

Venus and Mercury always stay close to the Sun. Visible within a few hours before sunrise or after sunset. Never visible around midnight.

Their orbits are inside Earth's orbit. (Remember that for last question of Mapping Solar System project.)

Venus and Mercury go through a complete set of phases. This proved that they orbit the Sun and that they do not orbit the Earth.

Other planets seen in only gibbous or full phases.

New, crescent and quarter phases only possible if planet can get inside Earth orbit.

Angle boundary between crescent and gibbous phase (i.e., the angle for the quarter phase) for the inferior planet depends on the size of the inner planet's orbit. When the other angle, Earth-to planet-to Sun angle, is 90°, the inner planet is half lit up (visible as a quarter phase).

venus phases and orbit positions

Do the "Mapping the Solar System from Earth" in the Student Guide to make the connection between a planet's position in its orbit and where in the sky it will appear as seen from Earth.

Link to Mapping Solar System Project help

Retrograde motion---when a planet moves ``backward'' (westward) with respect to its normal eastward drift against the stars. Happens when Earth is close to the planet.


Click on image to animate


Lecture slides (select the links to view the slides)

Motions of the Moon Eclipses - Geometry More eclipse pictures
Motions of the planets    

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