Geocentric model: how long was it taught in universities?

In summary: Copernicus' heliocentric model was not accepted by the majority of scientists until the 19th century.
  • #1
Aidyan
180
13
I have a historical question which I'm not finding any reference for. I recall how my former professor of history of science told us that the geocentric model was still taught for about a century in the accademia, long after Galileo's discovery of the phases of Venus and long after the heliocentric model became an established fact. I'm curious to know more about this. Can someone point me to some historical research or some reference that describes this?
 
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  • #2
Just look up the history of heliocentricism - you can easily establish the timeline from that.
 
  • #3
I did. Never found something about how long geocentrism was taught in academia.
 
  • #4
So when was the first University?
What were the main events in heliocentricism?
You only need to confirm or refute your profs general timeframe not get exact dates.
 
  • #6
Can you summarize it? It's behind a pay wall. I'd like to hear the answer to your question also, it is a good question because we often imagine that "scientific inertia" is near zero, but they may not always be true.
 
  • #7
Ken G said:
Can you summarize it? It's behind a pay wall. I'd like to hear the answer to your question also, it is a good question because we often imagine that "scientific inertia" is near zero, but they may not always be true.
Ken G, here is a version outside paywall (scroll to page 72) for educational purposes, somebody at FSU has it.
http://www.hep.fsu.edu/~wahl/artic/SA/mag/2014/201401.pdf
Example---if annual parallax cannot be detected, the stars must be very far away. We can gauge their angular size. If they are very far away they must be inconceivably large--huge. Copernicans were forced to argue that this is possible due to God's omnipotence. Being God, H e could make such huge objects and place them at such vast distance. But this was greeted with skepticism.
Here is a brief excerpt at the end:
==quote SciAm article by Dennis Danielson and Christopher M. Graney==
...in the middle of the 1600s, well after the deaths of pioneers such as Copernicus, Brahe and Galileo, Italian astronomer Giovanni Battista Riccioli published an encyclopedic assessment of cosmological options that he called (after Ptolemy’s great work) the Almagestum Novum. Riccioli weighed many arguments for and against the Copernican system, arguments dealing with matters of astronomy, physics and religion. But Riccioli judged that two main arguments tipped the balance decisively against Copernicus. Both were based on scientific objections. Both were rooted in Brahe’s ideas. Neither would be answered decisively until some hundreds of years later.
One argument was based on the inability to detect certain effects that Riccioli said a rotating planet should produce in projectiles and falling bodies. Brahe had felt that a rotating Earth should deflect a projectile away from a straight path. Yet these detections would not be observed until the 19th century, when French scientist Gaspard- Gustave de Coriolis worked out a full mathematical description of such effects.

The other argument was the one Brahe had made about star size, which Riccioli updated with telescopic observations. (Brahe had worked without a telescope.) Having designed a repeatable procedure for measuring the diameters of stars, he found that stars looked smaller than Brahe thought. Yet the telescope also increased the sensitivity to annual parallax, which still had not been detected, implying that the stars had to be even farther away than Brahe had assumed. The net effect was that stars still had to be every bit as titanic as Brahe had said.

[[Rather than give up their theory in the face of seemingly incontrovertible evidence, Copernicans were forced to appeal to divine omnipotence.]]

Riccioli complained about the Copernicans appealing to divine omnipotence to get around this scientific problem. A Jesuit priest, Riccioli could hardly deny the power of God. But still he rejected this approach, saying, “Even if this falsehood cannot be refuted, nevertheless it cannot satisfy the more prudent men.”

The acceptance of Copernicanism was thus held back by a lack of hard scientific evidence to confirm its almost incredible claims about cosmic and stellar magnitudes. In 1674 Robert Hooke, curator of experiments for the British Royal Society, admitted, “Whether the Earth move or stand still hath been a problem, that since Copernicus revived it, hath much exercised the wits of our best modern astronomers and philosophers, amongst which notwithstanding there hath not been anyone who hath found out a certain manifestation either of the one or the other.”

By Hooke’s time a growing majority of scientists accepted Copernicanism, al- though, to a degree, they still did so in the face of scientific difficulties. Nobody convincingly recorded the annual stellar parallax until Friedrich Bessel did it in 1838. Around that same time, George Airy produced the first full theoretical explanation for why stars appear to be wider than they are, and Ferdinand Reich first successfully detected the deflection of falling bodies induced by Earth’s rotation. Also, of course, Isaac Newton’s physics—which did not work with Brahe’s system—had long since provided an explanation of how Brahe’s “hulking, lazy” Earth could move.

Back in Galileo’s and Riccioli’s day, however, those opposed to Copernicanism had some quite respectable, coherent, observationally based science on their side. ...
==endquote==
 
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  • #8
It's interesting that Brahe's views, now no more than a footnote in the Ptolemy vs. Copernicus domination of that debate, had a significant period of being taken quite seriously. As for the colossal sizes of stars, I always wondered why the "stars are suns" unifying view did not hold more sway!
 

1. How long was the geocentric model taught in universities?

The geocentric model, which proposed that the Earth was the center of the universe and all celestial bodies revolved around it, was taught in universities for over 1,500 years. It was first introduced by the ancient Greek philosopher Aristotle in the 4th century BCE and was widely accepted until the 16th century CE.

2. Why was the geocentric model taught for so long in universities?

The geocentric model was taught for so long in universities because it was supported by influential figures such as Aristotle and Ptolemy, who were highly respected in the scientific community. It also aligned with religious beliefs at the time, which held that the Earth was the center of God's creation.

3. When did the geocentric model start to lose its credibility?

The geocentric model began to lose its credibility in the 16th century with the introduction of the heliocentric model by Nicolaus Copernicus. This model proposed that the Sun, not the Earth, was at the center of the universe, and was supported by evidence from observations and calculations made by astronomers such as Tycho Brahe and Johannes Kepler.

4. Did universities immediately stop teaching the geocentric model when the heliocentric model was introduced?

No, universities did not immediately stop teaching the geocentric model when the heliocentric model was introduced. In fact, it took several decades for the heliocentric model to gain widespread acceptance and for the geocentric model to be completely abandoned. This was due to the resistance from the Catholic Church and other institutions that supported the geocentric model.

5. Is the geocentric model still taught in universities today?

No, the geocentric model is not taught in universities today. It has been replaced by the heliocentric model, which is widely accepted by the scientific community and is supported by evidence from modern technology and advancements in astronomy. However, the geocentric model is still studied and discussed in history of science courses to understand the evolution of scientific thought and the impact of cultural and religious beliefs on scientific theories.

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