Video lecture for this chapter
Plato gave his students a major problem to work on. Their task was to find a geometric explanation for the apparent motion of the planets, especially the strange retrograde motion. One key observation: as a planet undergoes retrograde motion (drifts westward with respect to the stars), it becomes brighter. Plato and his students were, of course, also guided by the Pythagorean Paradigm. This meant that regardless of the scheme they came up with, the Earth should be at the unmoving center of the planet motions. One student named Aristarchus violated that rule and developed a model with the Sun at the center. His model was not accepted because of the obvious observations against a moving Earth.
Some of the observations that convinced the Greeks that the Earth was not moving are
Plato taught that since an infinite number of theories can be constructed to account for the observations, we can never empirically answer what the universe is really like. He said that we should adopt an instrumentalist view: scientific theories are just tools or calculation devices and are not to be interpreted as real. Any generalizations we make may be shown to be false in the future and, also, some of our false generalizations can actually ``work''--an incorrect theory can explain the observations (see the scientific method page for background material on this).
Aristotle (lived 384--322 B.C.E.) was a student of Plato and had
probably the
most significant influence on many fields of studies (science, theology, philosophy,
etc.) of any single person in history. He thought that Plato had gone too far with
his instrumentalist view of theories. Aristotle taught a realist view:
scientific, mathematical tools are not merely tools---they characterize the way the
universe actually is. At most one model is correct. The model he chose was one
developed by another follower of Plato, Eudoxus. The planets and stars were on concentric
crystalline spheres centered on the Earth. Each planet, the Sun, and the Moon were on
their own sphere. The stars were placed on the largest sphere surrounding all of the rest.
Aristotle chose this model because most popular and observational evidence supported it
and his physics and theory of motion necessitated a geocentric
(Earth-centered) universe. In his theory of motion, things naturally move to the
center of the Earth and
the only way to deviate from that is to have a force applied to the object.
So a ball
thrown parallel to the ground must have a force continually pushing it along.
This idea was unchallenged for almost two thousand years until Galileo showed
experimentally that things will not move or change their motion unless a force
is applied. Also, the crystalline spheres model agreed with the Pythagorean paradigm of
uniform, circular motion (see the previous
section).
A slight digression: Another conclusion drawn from Aristotle's teachings was that the Earth was unique with its own set of physical laws that were different from how things worked in the heavens. The Earth was a world and filled with change and decay while the planets, Moon, and Sun were perfect, unchanging and essentially ornaments on the sky, not worlds that could be explored. (Imagine the transformation of our viewpoint when we discovered using telescopes that those wandering points of light are worlds like the Earth and then later discovered other planets orbiting other stars!)
Now, to return to the motions of the planets...
Astronomers continued working on models of
how the planets moved. In order to explain the retrograde motion some models used
epicycles---small circles attached to larger circles centered on the Earth. The
planet was on the epicycle so it executed a smaller circular motion as it moved around the
Earth. This meant that the planet's distance from us changed and if the epicyclic motion
was in the same direction (e.g., counter-clockwise) as the overall motion around the Earth,
the planet would be closer to the Earth as the epicycle carried the planet backward with
respect to the usual eastward motion. This explained why planets are brighter as they
retrogress.
Ptolemy's view of the world. Select the image to go to Jim Siebold's ancient
maps database from which this picture came (will display in another window).Ptolemy's geocentric universe
Ptolemy
(lived 85--165 C.E.) set out to
finally solve the problem of the planets motion.
He combined the best features of the geocentric models that used epicycles with the most
accurate observations of the planet positions to create a model that would last for
nearly 1500 years. He added some refinements to explain the
details of the observations: an ``eccentric'' for each planet that was the true center
of its motion (not the Earth!) and an ``equant'' about which each planet moved uniformly in
relation to (not the Earth!). See the figure below for a diagram of this setup.
These refinements were incompatible with Aristotle's model and the Pythagorean paradigm---a planet on an epicycle would crash into its crystalline sphere and the motion is not truly centered on the Earth. So Ptolemy adopted an instrumentalist view---this strange model is only an accurate calculator to predict the planet motions but the reality is Aristotle's model. This apparent contradiction between reality and a calculation device was perfectly fine in his time. Our modern belief that models must characterize the way the universe actually is is a tribute to the even longer-lasting influence of Aristotle's realism. Ptolemy was successful in having people adopt his model because he gathered the best model pieces together, used the most accurate observations and he published his work in a large 13-volume series called the ``Almagest'', ensuring that his ideas would last long after he died.
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last updated: January 21, 2022