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Galileo Galilee

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Q: Which famous astronomer observed Venus and Jupiter and supported Copernicus' theory of a heliocentric solar system?
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The heliocentric system gained support when galieo observed that?

the phases of Venus could only be explained by it orbiting the Sun, not Earth as in the geocentric model. This observation provided evidence that supported the heliocentric system proposed by Copernicus.


Do The observed phases of Venus supported the heliocentric system?

The phases of Venus are well supported by the heliocentric system, but they are also supported very well by the previous geocentric system. All you need for Venus to have phases is that Venus should pass between Earth and Sun. That happens in both the heliocentric system and the geocentric system.


What did Galileo observe to Mae him conclude that your solar system was heliocentric?

Galileo observed the phases of Venus, which could only be explained if Venus orbited the Sun and not Earth. This observation supported the heliocentric model proposed by Copernicus.


What did Galileo see when he observed Venus through his telescope?

Galileo observed phases of Venus, which were only possible if Venus orbited the Sun and not Earth, supporting the heliocentric model of the solar system proposed by Copernicus. This observation was a key piece of evidence in favor of the heliocentric theory.


Do the observed phases of Venus support the heliocentric system?

The phases of Venus are well supported by the heliocentric system, but they are also supported very well by the previous geocentric system. All you need for Venus to have phases is that Venus should pass between Earth and Sun. That happens in both the heliocentric system and the geocentric system.


How did Galileo and observation of Venus support the heliocentric?

Galileo's observations with his telescope supported the concept of heliocentricism. He noted that the satellites of Jupiter and Venus, based on their range of phases, did not match geocentricism supported by Ptolemy. He noted that based on these findings, that the Heliocentric theory was correct.


When did Galileo discover the craters in the moon?

Galileo Galilei discovered the craters on the Moon in 1609, when he observed them through a telescope he had developed. This observation played a crucial role in supporting the heliocentric model of the solar system proposed by Copernicus.


When comparing the cosmology of Copernicus with Ptolemy Copernicus had provided a far explanation for all the celestial motions?

Copernicus proposed a heliocentric model of the solar system where planets revolve around the Sun, providing a simpler and more accurate explanation for celestial motions compared to Ptolemy's geocentric model where planets were believed to orbit the Earth. Copernicus' model was more consistent with observed planetary movements and laid the foundation for modern astronomy.


Who was the famous astronomer who observed Venus and Jupiter?

Seventeenth-century astronomer Galileo Galilei.


What caused Copernicus to challenge aristotles theories of planetary motion?

Copernicus challenged Aristotle's theories of planetary motion due to observations that didn't align with the geocentric model, particularly the retrograde motion of planets. Through his own observations and mathematical calculations, Copernicus proposed a heliocentric model where the Earth and other planets revolve around the Sun, providing a simpler explanation for the observed phenomena in the sky.


Who does said that the sun is in the middle of solar system?

Nicolaus Copernicus proposed the theory that the Sun is at the center of the solar system in his work "De revolutionibus orbium coelestium" (On the Revolutions of the Celestial Spheres) in the 16th century. This heliocentric model replaced the geocentric model, which had Earth at the center of the universe.


Why is Copernicus' model much simpler than Ptolemy's?

Copernicus' model is simpler than Ptolemy's because it places the sun at the center of the solar system, with planets orbiting around it in nearly circular paths. This heliocentric model eliminates the need for complex epicycles, which Ptolemy used in his geocentric model to explain the retrograde motion of planets. Copernicus's model also provides a more elegant explanation for the observed movements of celestial bodies.