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Does the sun move with the earth and moon?

No, the moon orbits the Earth and the Earth Orbits the Sun. The Earth does not orbit in circular patterns. This is proved by Johannes Kepler. Kepler states that the planets orbit in elliptical.


How was Copernicus' model of the universe different from ptomely's model?

Copernicus proposed a heliocentric model of the universe with the sun at the center, while Ptolemy's model was geocentric, with the Earth at the center. Copernicus' model revolutionized astronomy by correctly positioning the planets in relation to the sun and providing a simpler explanation for the motion of celestial bodies.


What year did Johannes Kepler prove that planets orbit in an oval or elliptical motion?

Johannes Kepler proved that planets orbit in an elliptical motion in 1609 with the publication of his work "Astronomia Nova." This marked the formulation of his first law of planetary motion, which states that planets move in ellipses with the Sun at one focus. Kepler's discoveries significantly advanced the understanding of celestial mechanics and laid the groundwork for future astronomical research.


How did Kepler figure out that planets orbit is elliptical?

Kepler, the person who first wrote about elliptical orbits, had a Trinitarian view of the solar system in which it made perfect sense theologically to have the Sun at the centre of the universe. Copernicus also believed in a Sun-centred system.


How do you evaluate this sentence '' The revolution accomplished from Copernicus to Newton was the great spiritual adjustment that modern civilization had to make?

It was certainly a scientific revolution if not a spiritual one. It started in1543, the year Copernicus published his theory of the planets' orbits in a book called 'De revolutionibus'. Copernicus's model differed from the ancient Ptolemaic model by having the Sun at the centre instead of the Earth, but in all other respects it was similar, with the planets still moving around epicycles which in turn moved in circles round the common centre. Johannes Kepler in 1609 produced an entirely novel theory explaining the planets' orbits, with the Sun at (or near) the centre and the planets travelling in fixed elliptical paths or orbits. Finally in 1687 Newton explained the planets' orbits using the new scentific discoveries of the law of gavity and the laws of motion, and confirmed the validity of Kepler's model. In that period of around 150 years the Earth's place at the centre of the Universe was evaluated and rejected, and some of the mathematical methods of modern physics were discovered and applied to the planets. Also in that period Galileo had a long quarrel with the catholic church and was tried for heresy after being accused of re-interpreting the scriptures by saying that the Copernican system was the absolute truth. However Galileo was eventually proved wrong because Kepler's model was adopted and Copernicus's model was rejected. His insistence that the Sun is at the centre was however accepted, and it still is.

Related Questions

Does the sun move with the earth and moon?

No, the moon orbits the Earth and the Earth Orbits the Sun. The Earth does not orbit in circular patterns. This is proved by Johannes Kepler. Kepler states that the planets orbit in elliptical.


Who used mathematics to prove the theories of Copernicus?

In physics, theories are not mathematically proved but instead they are compared with physical observations to see if they are correct. Copernicus's theory was not just an idea that the Sun is at the centre, but also a detailed mathematical system of circle and epicycles that provided a model of the planets' orbits. At the time of Copernicus and for a time afterwards, his theory was used to predict the planets' positions, and when the predictions were found to be 'correct', the theory was considered 'proved' . But later Tycho Brahe developed more accurate measurement techniques, and using those he discovered small errors in the predicted positions of the planets. That led to Kepler's work and the discovery of elliptical orbits.


When were elliptical orbits discovered?

That has never been proven, and it's impossible to prove. It's "only a theory".However, in the 16th Century, Johannes Kepler showed that IF that's what's happening, then itwould accurately explain all the motions of the sun, moon, and planets that we actually do see inthe sky.Since that model so successfully explained what we see ... and a century later, Newton showedthat if his ideas about gravity were correct, then planets have to travel elliptical paths aroundthe sun ... Kepler's model was accepted as the best theory. But it can't be proven.And not only that! If you find something seen in the sky that Kepler's model doesn't explain, orif you come up with an explanation that fits the observations with better accuracy, then Kepler'stheory will be thrown out, and yours will become the accepted one.That's how Science works.


How was Copernicus' model of the universe different from ptomely's model?

Copernicus proposed a heliocentric model of the universe with the sun at the center, while Ptolemy's model was geocentric, with the Earth at the center. Copernicus' model revolutionized astronomy by correctly positioning the planets in relation to the sun and providing a simpler explanation for the motion of celestial bodies.


Why do you think other religious men condemned the ideas of Copernicus if he was providing that god created a more perfect system?

Copernicus produced an alternative model of the planets that had the Sun at the centre, which contradicted the religious view at the time. The church was unwilling to change its theology without adequte proof. The wisdom of the church's attitude was eventually proved when Copernicus's model was rejected in favour of one discovered by Kepler with elliptical orbits. It also had the Sun at the centre, and when the elliptical orbits were confirmed by Newton's theoretical discoveries the model was generally adopted.


Who proved you had eliptical orbits and not sircular ones?

Johannes Kepler.


Why do planets take different times to orbit the sun?

Kepler's Third Law of Planetary Motion gives the mathematical formula for this. Isaac Newton proved the Law follows from his theory of gravitation. I will not go into the mathematics, but basically it's just how gravity works with planets.


What did Johannes Kepler do?

He simply discovered many things that makes technology where we are! -m In astronomy he used measurements made by Tycho Brahe to do many complicated calculations to discover the shape of the planets' orbits. The results were published as the three laws of planetary motion in 1618. They were found to give good results when used to predict the future positions of the planets. For this work Kepler is recognised as one of the founders of modern astronomy. ________________________________ Kepler worked with Tycho Brahe for several years. Brahe had no great skill in science or mathematics, but was a METICULOUS and precise observer. Based largely on Brahe's observations, Kepler was able to determine that the planet Mars - and by extension, all the other planets - traveled in elliptical paths under the influence of a force that was inversely proportional to the square of the distance between the Sun and the planet. This paved the way for Newton's development of calculus and the math that describes gravity.


How did Kepler figure out that planets orbit is elliptical?

Kepler, the person who first wrote about elliptical orbits, had a Trinitarian view of the solar system in which it made perfect sense theologically to have the Sun at the centre of the universe. Copernicus also believed in a Sun-centred system.


How do you evaluate this sentence '' The revolution accomplished from Copernicus to Newton was the great spiritual adjustment that modern civilization had to make?

It was certainly a scientific revolution if not a spiritual one. It started in1543, the year Copernicus published his theory of the planets' orbits in a book called 'De revolutionibus'. Copernicus's model differed from the ancient Ptolemaic model by having the Sun at the centre instead of the Earth, but in all other respects it was similar, with the planets still moving around epicycles which in turn moved in circles round the common centre. Johannes Kepler in 1609 produced an entirely novel theory explaining the planets' orbits, with the Sun at (or near) the centre and the planets travelling in fixed elliptical paths or orbits. Finally in 1687 Newton explained the planets' orbits using the new scentific discoveries of the law of gavity and the laws of motion, and confirmed the validity of Kepler's model. In that period of around 150 years the Earth's place at the centre of the Universe was evaluated and rejected, and some of the mathematical methods of modern physics were discovered and applied to the planets. Also in that period Galileo had a long quarrel with the catholic church and was tried for heresy after being accused of re-interpreting the scriptures by saying that the Copernican system was the absolute truth. However Galileo was eventually proved wrong because Kepler's model was adopted and Copernicus's model was rejected. His insistence that the Sun is at the centre was however accepted, and it still is.


Who was the German astronomer who proved that the planets move in oval paths called ellipses?

Johannes Kepler was the German astronomer who proved that the planets move in oval paths called ellipses. His work laid the foundation for the laws of planetary motion.


Why did the earth centered model prove to be difficult?

If we assume that the Earth is in the center of the solar system, then the math of predicting the path and the positions of the planets is extraordinarily difficult. It was even HARDER when the early astronomers, shackled as they were to the presumption that Aristotle knew something, that every celestial object traveled in circles.They don't, and the assumptions that astronomers had to make to justify circular motion in the skies was what eventually brought everything down. Then Copernicus demonstrated that the math was easier if he presumed that the Sun was in the center, and Kepler proved that everything traveled in ELLIPTICAL rather than circular orbits. This further simplified the math.Then Newton proposed the inverse-squares law for the relationship between gravity and distance, and everything fell into place.