Copernicus (1473-1543)
1. Not an observational but a theoretical astronomer. He accepts Ptolemy’s
data.
2. Copernicus wants to:
- systematize astronomy by using only (linear) uniform
circular motion, thus rejecting equants
- simplify astronomy by reducing retrograde motions and
brightness variations to the motion of the earth.
Note that one of the reasons for doing this is his belief in the
mathematical wisdom of the Author of things.
3. Main features of the system, which had more than one version, however:
- The system uses deferents and epicycles. It is
quite complex for inferior planets (especially mercury), but simpler for
superior planets (basically, one deferent eccentric and one epicycle).
- there is no common center to the deferent circles. For
example, the center of the deferent of the Earth and those of other
planets do not coincide; moreover, the deferent of the Moon has its center
on the Earth.
- the Earth is not at the center of the universe; the Sun
is.
- The centers of the planets' deferents is not the Sun. They are off by about
1/25 of the radius of the Earth’s revolution about the sun. So, since the
Sun is at the center of the universe, the center of the deferents carrying
the planets’ epicycles is not. Hence, although the universe is
heliocentric, C.’s planetary model is only heliostatic, as the orbits of
the planets do not have the Sun at their centers. To have our solar system, one has to wait for Kepler. All in all, C. was not a Copernican.
- the Earth-Sun distance is insignificant with respect to
that between the Sun and the fixed stars.
- the motions of stars, Sun, and planets arise, at least
in part, from the motion of the Earth. In particular, retardations,
stations, regressions are optical illusions due to the relative motions of
the planets and the Earth.
4. Evidence for the theory:
- there’s theoretical simplification because:
- the motions of the orbs
is circular uniform (no equants). However, Ptolemaic theory can be done without
equants.
- the distance of a
planet from the Sun is proportional to the planet’s period of revolution,
and this explains retrograde motion uniformly.
- there are some computational simplifications in lunar
theory.
Problem: However, while in Ptolemy the
apparent geocentric position of the planets is built into the theory, in
Copernicus it has to be inferred by considering the position of both planets
and Earth with respect to the Sun. Hence, at times the system is at least
computationally as complex as Ptolemy's. Famously, Galileo himself noted the
difficulty of understanding Copernicus.
- the idea of the sphere of the stars spinning once a day
seems preposterous if the same data can be more easily explained by the
rotation of the earth.
Problem: the Earth is heavy; so,
what makes it rotate? By contrast, the sphere of the stars is made of ether, a
weightless substance
- the phases of Venus (observable, however, only by
telescope, which comes about only 60 years later). Note that they can be
accounted for by Brahe's system as well.
- The paths of the planets are smooth, without nodes or
cusps (good for mathematics)
5. Problems for the theory:
- absence of stellar parallax.
Answer: the universe is immense,
although finite.
- since the earth is heavy, what prevents it from
returning to its natural place, the center of the universe?
Answer: heaviness is just the
tendency of every celestial body to form a whole with things of the same
nature, e.g., Earth objects with other Earth objects. There is no cosmic
gravity.
- why aren’t clouds, birds, arrows, etc. left behind by
the earth’s rotation?
Answer: all terrestrial bodies
share a natural rotational and orbital motion because, being terrestrial, they
have the same nature as the Earth. Note that this is not a physical
account. Copernicus lacks a proper
mechanics.
·
Inconsistent
use of eccentricity, sometimes measured from the Sun, sometimes from the earth
- what makes the Earth rotate?
Answer: round objects placed in space
rotate just because they are round.
6. The Sun is at the center of the universe because it is the giver of
light, the visible symbol of God. Around it (more or less) are the deferents of
the planets. The periods of revolution
increase with the distance from the Sun,
7. The instrumentalism of Osiander's preface.