Module 10 - Ancient Greeks Models of the Universe Flashcards

1
Q

Around 600 BCE, Thales of Miletus proposed that Earth is a

A

disk floating on wate

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2
Q

suggested that Earth is a cylinder and that its surface is curved.

A

Anaximander, also from Miletus

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3
Q

considers Earth as the center of the universe.

A

Geocentric model

Pythagorean model

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4
Q

assumes the sun to be the center of the universe.

A

Heliocentric model

Copernicus’s model

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5
Q

was acknowledged to be the first to assert that Earth is round, and that the heavenly bodies move in circles.

A

Pythagoras

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6
Q

was credited with having determined the relative positions of the sun, the moon, and Earth during solar and lunar eclipses.

A

anaxagoras

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7
Q

retrograde motion.

A

west to east as predicted. But occasionally, they backtrack for a while

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8
Q

first to “save the appearances”

A

Eudoxus model

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9
Q

outermost sphere that was the domain of what he called the

A

Prime Mover

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10
Q

the order of heavenly bodies in the universe was (from Earth out) : Earth, moon, Mercury, Venus, sun, Mars, Jupiter, Saturn, the fixed stars, and the firmament of the Prime Mover.

A

Aristotlemodel

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11
Q

Aristotle divided the universe into two realms

A

terrestrial and the celestial

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12
Q

Aristotle’s model was based on the three types of terrestrial motion :

A

natural, violent and alteration.

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13
Q

tendency of an object to seek its natural place in the universe

A

Natural motion

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14
Q

objects can be compelled to move in unnatural ways by the application of a force.

A

violentmotion

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15
Q

vertical motion as

A

natural

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16
Q

horizontal motion as

17
Q

type of change or alteration

A

Generation is “coming to be”
corruption is “passing away.”

18
Q

known in his time as “The Greek Geometer”

A

Appollonius

19
Q

The Greek mathematician Appollonius , known in his time as “The Greek Geometer”, introduced the idea of an epicycle explain planetary motion.

A

Ptolemy model

20
Q

is a circle on which a planet moves

21
Q

The center of this small circle in turn moved around Earth along a bigger circular path called the

22
Q

refined this model by considering that Earth was off-center or eccentric in the deferent where the sun moved.

A

hipparchus

23
Q

He defined a point on the other side of the deferent’s center and called it the

24
Q

asserted that Earth spins on its axis every day and revolves around the sun just like the other planets; only the moon orbits Earth.

A

Nicolas copernicus

25
Johannes Kepler Laws
Law of Ellipses Law of Equal Areas Law of Harmonies
26
which states that the planets move in ellipses having a common focus situated at the sun
Law of ellipses
27
Closest point to the sun
perihelion
28
Farthest point to the send
Aphelion
29
move around the sun in such a way that a line drawn from the sun to the planet sweeps out equal areas in equal intervals of time. the planet moves fastest at the perihelion and slowest at the aphelion.
Law of Equal areas
30
It states that the squares of the periods of the planets are proportional to the cubes of their mean distances from the sun.
Law of harmonies