Eudoxus
408 to 355 BC
- Outside the earth are concentric transparent spheres.
- They carry the moon, sun and planets.
- They rotate at different speeds about different axes.
- The picture illustrates the spheres for Mars.
- The outer sphere rotates once per Earth day: its motion makes Mars
rise and set each day.
- The next sphere rotates once each Mars year. It carries Mars around
the ecliptic once per Mars year.
- The next two spheres have almost opposite motions and (approximately)
give Mars its retrograde motion (see picture below).
- Mars is on the innermost sphere, approximately between the viewer
of this drawing and Earth.
ASTR 121 Home
Davison E. Soper, Institute of Theoretical Science,
University of Oregon, Eugene OR 97403 USA
soper@bovine.uoregon.edu