Planetary Orbits #1: Prevailing Models
Tycho Brahe and
Johann Kepler are one of the great pairs of science. The former collected
immaculate data from his observations of the skies; which the latter then
analyzed to come up with his famous laws of planetary motion. Very fairy tale
like, right? Except that reality was far more complicated, as Kitty Ferguson
describes in Tycho
and Kepler, her awesome biography of the two men, their personal lives
and their science.
This blog, the
first in a four-part series, explains the prevailing astronomical views before Brahe and Kepler changed our
understanding forever.
There was
Ptolemy’s model, with the Earth at the center, and everything else orbiting the
Earth. In this model, planets seemed to slow down and accelerate at times and
even reverse direction: this is because we on Earth are moving in a circle
while observing the other planets. Hence the concept of epicycles (circles
within circles) was added to the model:
How did the
epicycles help describe the observed motion?
“By adjusting the size, direction, and
speed of the epicycles, astronomers could explain many of the irregularities
observed in the way the planets, Sun and Moon move.”
Does this sound
very convoluted? Why didn’t astronomers wonder what might cause such weird changes in both the direction and speed of motion?
1)
Because
it was complicated enough to describe the motion of planets, so few wanted to
venture into the “why” question.
2)
Blame
Aristotle!
“(Aristotle had drawn) a line between
physics and the mathematical sciences, including astronomy, in a way that could
be interpreted to mean that astronomers need not search for Aristotelian
“causes” for celestial motions.”
But why wasn’t
Aristotle’s view questioned? Ah, because the Church had incorporated
Aristotelian views; and the waters were now horribly muddied. Could one
contradict any aspect of Aristotle
without also (in effect) attacking the Church? But what about Aristotle’s view
was so attractive to the Church in the first place? The fact that he had also
declared that:
“Everything below the orbit of the Moon was
subject to change, degradation, and decay, while the heavenly spheres beyond
the Moon were a realm of unvarying, eternal perfection”.
This aligned with
Christianity’s picture of “fallen, lost humanity on Earth and eternal, holy
realms above”. Which is why his views were adopted by the Church.
The alternate
model was by Copernicus that held the Sun at the center around which all the
planets revolved. While the orbits weren’t as twisted as those in Ptolemy’s
model, they weren’t perfectly circular either.
With neither model
simple in its orbits, in the absence of any attempt to identify causes, it just seemed like a matter of preference (or geometric convenience)
which model one believed: Ptolemy or Copernicus. But since Copernicus’ model
didn’t align with Church doctrine whereas Ptolemy’s did, no points for guessing
which view prevailed at that time…
Interesting. I don't know how much this will interest who are not somewhat alive to astronomy.
ReplyDeleteYour reference to "The former collected immaculate data from his observations of the skies; which the latter then analyzed to come up with his famous laws of planetary motion" invoked a memory of a somewhat similar situation. After the first quarter of the last century, the telescopes became very powerful and a lot of observations were made. It led to the discovery of countless galaxies. Application grew and scientific interpretations revolutionized the subject. Not only they found that all galaxies were receding from one another but also leaned heavily on Einstein's special theory of relativity to explain the astronomic domain.
The combination of observation nature and fitting scientific understanding probably get refined steadily over a few centuries prior to our 21st.