Why were Aristotle’s and Ptolemy’s models accepted for more than a thousand years in spite of being incorrect? (2 correct answers)(2 points) Responses Followed the current church's ideas about Earth. Followed the current church's ideas about Earth. There models made the sun the center of the solar system. There models made the sun the center of the solar system. No one had the technology to disprove the models. No one had the technology to disprove the models. The models were actually correct.
The two correct answers are:
1. No one had the technology to disprove the models.
2. The models were actually correct.
The correct answers are:
1. The models followed the current church's ideas about Earth.
2. No one had the technology to disprove the models.
The correct answers are:
1. The models followed the current church's ideas about the Earth. During Aristotle's and Ptolemy's time, the prevailing belief was that Earth was at the center of the universe, and these models aligned with this geocentric view. The Catholic Church heavily influenced scientific thought during this period, and any theories that contradicted religiously accepted beliefs were met with skepticism and opposition.
2. No one had the technology to disprove the models. In Aristotle's and Ptolemy's time, scientific instruments and technology were limited compared to what we have today. They did not have access to telescopes or sophisticated mathematical tools that could provide the necessary evidence to disprove their models. Therefore, without the means to gather strong empirical evidence against them, their models remained largely unquestioned for centuries.
It is worth noting that the models themselves were not actually correct. Both Aristotle's and Ptolemy's geocentric models proposed Earth as the center of the universe, with celestial bodies moving in perfectly circular orbits around it. However, later developments in astronomy, such as Copernicus' heliocentric model and Kepler's laws of planetary motion, provided more accurate explanations of the motion of celestial bodies.