, 17.05.2020batopusong81

# Illustration of saving the appearances

Pythagoras was acknowledged to be the first to assert is round and that the heavenly bodies move in circles. Earth is at rest at the center of the universe and everything rotates around Earth. He also considered the motions of the planets were mathematically related to musical sounds and numbers. These ideas are called “The Music of the Spheres.” Anaxagoras, a follower of Pythagoras, was credited for determining the relative positions of the sun, the moon, and Earth, during solar and lunar eclipse. The Greek Philosopher and teacher Plato adopted Pythagorean view of the motion of heavenly bodies as combinations of circular motion about Earth. He assumed that all motions in the universe are perfectly circular and all that heavenly bodies are ethereal or perfect. Most of the time, planets moved from west to east as predicted. But occasionally, they backtrack for a while, that is, they move westward before resuming their eastward motion. This is called the retrograde motion. The followers and students of Plato were tasked to explain the retrograde motion of the planets.

In particular, Plato challenged them with this problem: “What circular motions, uniform and perfectly regular, are to be admitted as hypothe This challenge is known as “Plato’s Saving the Appearances” in the history of astronomy.
Pythagoras was acknowledged to be the first to assert is round and that the heavenly bodies move in circles. Earth is at rest at the center of the universe and everything rotates around Earth. He also considered the motions of the planets were mathematically related to musical sounds and numbers. These ideas are called “The Music of the Spheres.” Anaxagoras, a follower of Pythagoras, was credited for determining the relative positions of the sun, the moon, and Earth, during solar and lunar eclipse. The Greek Philosopher and teacher Plato adopted Pythagorean view of the motion of heavenly bodies as combinations of circular motion about Earth. He assumed that all motions in the universe are perfectly circular and all that heavenly bodies are ethereal or perfect. Most of the time, planets moved from west to east as predicted. But occasionally, they backtrack for a while, that is, they move westward before resuming their eastward motion. This is called the retrograde motion. The followers and students of Plato were tasked to explain the retrograde motion of the planets. In particular, Plato challenged them with this problem: “What circular motions, uniform and perfectly regular, are to be admitted as hypothesis so that it might be possible to save the appearances presented by the planets?” This challenge is known as “Plato’s Saving the Appearances” in the history of astronomy.
Explain how Plato's problem of ''saving the appearances ''constrained greek models of the universe.

The Greeks believe in the theory of planetary motion, an assumption that planets must move in a perfectly circular motion.

Meanwhile, in ''saving the appearances'', Plato explained that although planets move towards a perfect path or circular motion, it is still apparent that there are still planets that move in an irregular motion or wander across the sky.

The Greek Philosopher and teacher Plato adopted Pythagorean view of the motion of heavenly bodies as combinations of circular motion about Earth. He assumed that all motions in the universe are perfectly circular and all that heavenly bodies are ethereal or perfect. Most of the time, planets moved from west to east as predicted. But occasionally, they backtrack for a while, that is, they move westward before resuming their eastward motion. This is called the retrograde motion. The followers and students of Plato were tasked to explain the retrograde motion of the planets. In particular, Plato challenged them with this problem: “What circular motions, uniform and perfectly regular, are to be admitted as hypothesis so that it might be possible to save the appearances presented by the planets?” This challenge is known as “Plato’s Saving the Appearances” in the history of astronomy.

it means that the student of Plato must made a model of the universe

Kapag pinataas ng klerk ng supermarket ang aking mga groseri, \$ 12 ako kaysa sa mayroon ako. Sinimulan kong alisin ang mga item mula sa mga bag, nang ang isa pang mamimili ay nag-abot sa akin ng isang \$ 20 bill. "Mangyaring huwag ilagay ang iyong sarili," sabi ko sa kanya. "Hayaan mo akong magkwento sa iyo," sinabi niya. “Ang aking ina ay nasa ospital na may cancer. Binisita ko siya araw-araw at dinadala sa kanya ang mga bulaklak. Nagpunta ako kaninang umaga, at nagalit siya sa akin sa paggastos ng aking pera sa higit pang mga bulaklak. Hiniling niya na gumawa ako ng iba pa sa perang iyon. Kaya, dito, mangyaring tanggapin ito. Ito ang mga bulaklak ng aking ina. " - Leslie Wagner, Peel, Arkansas.

1-4 UITS

click create

click new

click file

B. Opening a previously Saved document

click the Look in drop down arrow when the dialog box appears.

choose the filename where your document was saved, then click open.

click file tab

ciick open command

C. Saving a document

Type the name of the document

Then click save to save your document

Dialog box of Save as appears, open the location where you want to save

Press or click save command

A. Creating a new document

select blank document​

Explanation:

Plato's Problem of "Saving the Appearances" Constrained Greek Models of the Universe

Saving the appearances is plausible in the context of Plato's philosophy, which in turn can be understood as his reaction to the moral and political chaos of his age, which left him highly dissatisfied with the physical world. His concept of an ideal reality is simply illustrated. A circle drawn on paper is an imperfect representation in the visible world of experience of a perfect circle, which exists only in the world of thought. In his Republic, Plato wrote that the sky was part of the visible world, and the true revolutions of the planets, sun, and moon were to be discerned by reason and thought, not by sight. Pythagoras was acknowledged to be the first to assert is round and that the heavenly bodies move in circles. Earth is at rest at the center of the universe and everything rotates around Earth. He also considered the motions of the planets were mathematically related to musical sounds and numbers. These ideas are called “The Music of the Spheres.” Anaxagoras, a follower of Pythagoras, was credited for determining the relative positions of the sun, the moon, and Earth, during solar and lunar eclipse. Greek Philosopher and teacher Plato adopted Pythagorean view of the motion of heavenly bodies as combinations of circular motion about Earth. He assumed that all motions in the universe are perfectly circular and all that heavenly bodies are ethereal or perfect. Most of the time, planets moved from west to east as predicted. But occasionally, they backtrack for a while, that is, they move westward before resuming their eastward motion. This is called the retrograde motion. The followers and students of Plato were tasked to explain the retrograde motion of the planets. In particular, Plato challenged them with this problem: “What circular motions, uniform and perfectly regular, are to be admitted as hypothesis so that it might be possible to save the appearances presented by the planets?” This challenge is known as “Plato’s Saving the Appearances” in the history of astronomy.

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