Astronomy Test Flashcards

(32 cards)

1
Q

Astronomer #1

A

Aristotle
Greek
Geocentric
Syllogism
Epicycles to explain retrograde motion

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2
Q

Astronomer #2

A

Ptolemy
Egyptian of Greek descent
Geocentric
Epicycles + eccentric Earth + equant to explain retrograde motion

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3
Q

Astronomer #3

A

Copernicus
Polish
Heliocentric
Epicycles w sun in the middle

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4
Q

Astronomer #4

A

Tycho Brahe
Danish
Geocentric
Sextant to measure light from planet or star

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5
Q

Astronomer #5

A

Galileo
Italian
Heliocentric
Jupiter’s 4 moons

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6
Q

Astronomer #6

A

Kepler
German
Heliocentric
3 laws based on Tycho’s data

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7
Q

Astronomer #7

A

Newton
British
Heliocentric
Newton’s Law of Universal Gravitation

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8
Q

Astronomer #8

A

Hubble
American
Heliocentric
Further galaxies recede faster than closer ones

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9
Q

Sun

A

99.8% of the mass of the solar system
solar wind is charged particles flying off the sun

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10
Q

Sun’s 1st Layer

A

Core
nuclear fusion - fuse hydrogen to make helium

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11
Q

Sun’s 2nd Layer

A

Radiative Zone

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12
Q

Sun’s 3rd Layer

A

Convective Zone

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13
Q

Sun’s 4th Layer

A

Photosphere

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14
Q

Sun’s 5th Layer

A

Chromosphere
transition zone

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15
Q

Sun’s 6th Layer

A

Corona

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16
Q

Mercury

17
Q

Venus

A

Venus Express Mission

18
Q

Earth

A

Landsat Satellites
1 moon

19
Q

Mars

A

Viking 1
2 moons

20
Q

Jupiter

21
Q

Saturn

22
Q

Uranus

23
Q

Neptune

24
Q

Binary System

A

2 stars orbit center of mass

25
Dying Star
shrinks into white dwarf - electron degeneracy under goes supernova - neutron star - neutron degeneracy - black hole - denser core bigger star to live longer
26
Chandrasekher Limit
- 1.4x the mass of the sun - determines the transformation a dying star will go through
27
Standard Candles
Measure brightness of objects to tell how far they are
28
Cephid Variable Stars
Brighten and dim periodically - can tell how far away they are
29
Type 1a Supernova
White dwarf is in binary system and takes mass from the other star - mass exceeds Chandrasekhar limit and can undergo a supernova Better standard candle than Cephid Variables
30
Kepler's First Law
Planets move in elliptical orbits around the sun
31
Kepler’s Second Law
Planets move equal areas in equal time
32
Kepler’s Third Law
Major axis in an elliptical orbit Semimajor axis in an elliptical orbit Minor axis in an elliptical orbit Semimajor axis ^3 = period of an orbit ^2