Chapter 3 Flashcards

(41 cards)

1
Q

In Ptolemy’s model, it is possible to have a planetary orbit without retrograde motion

A

true

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2
Q

Copernicus’ heliocentric model was able to predict the location of the planets more accurately than Ptolemy’s geocentric model

A

false

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3
Q

Copernicus was the first to be able to prove that the Earth orbited around the Sun

A

false

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4
Q

According to the small angle equation, if an object at a fixed distance is suddenly shrunk to a smaller size, then the angular size will

A

decrease

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5
Q

Copernicus was the first person to suggest that the Sun is at the center of our solar system.

A

false

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6
Q

Copernicus figure out which planets were closer to the Sun and which were further

A

sidereal and synodic periods

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7
Q

Eratosthenes

A

ancient astronomer measured the radius of the Earth

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8
Q

size of the Earth could be measured accurately in ancient times by using

A

shadows on Earth

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9
Q

Ptolemy improved the geocentric model by

A

adding epicycles and deferents

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10
Q

One of the main objections to the heliocentric model

A

we do not feel the Earth moving

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11
Q

Aristotle believed that the planets

A

orbited the Earth in circular orbits

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12
Q

superiod conjunction

A

When a planet orbits to the opposite side of the Sun as Earth (and it appears near the Sun in our sky), the planet is at

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13
Q

sidereal period

A

The time it takes a planet to orbit the Sun once and return to the same location in space

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14
Q

Ptolemy’s improvements were important because they explained

A

retrograde motion

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15
Q

scientific ideas was never discussed in the ancient world

A

faint lights in the sky are galaxies

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16
Q

Aristotle

A

believed the universe could be understood by the power of reason alone

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17
Q

Geocentric cosmology

A

all other celestial bodies travel around the earth in circular orbits

18
Q

Small angle equation

A

θ = 206,265 * D / d

19
Q

D

20
Q

d

21
Q

θ

A

angular diameter

22
Q

distance equation

A

d=206,265*D/θ

23
Q

diameter equation

A

D=θ*d/206,265

24
Q

Retrograde motion

A

some planets can reverse their steady eastward motions among the stars

25
Ptolemaic model
requires the planets not only to move in circles around the Earth but also to move along smaller circles around imaginary points along the main circular orbits
26
Epicycles
circle that is carried and rides around on another circle
27
Epicycles
circle that is carried and rides around on another circle
28
Heliocentric model
relative spacing of planets is fixed uniquely by their apparent motions
29
Parallax
shift in angle that occurs when a nearby object is seen against a distance backdrop from two different perspectives
30
Elongation
angle between the sun and a planet as seen by an observer on earth
31
inferior planets
planets closer to the sun than the earth
32
superior planets
planets further from the sun than the earth
33
greatest elongation
inferior planets limit
34
inferior conjunction
planet is between the sun and the earth
35
superior conjunction
planet is on the other side of the sun as seen from earth
36
opposition
elongation is 180 degrees
37
synodic period
time it takes for a planet to make a complete cycle of elongation configuration
38
sidereal period
time it takes for a planet to complete an orbit
39
superior planets equation
1/S=1/E-1/P
40
inferior planets equation
1/S=1/P-1/E
41
E
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