Solar System Flashcards

1
Q

nebular hypothesis was proposed by who

A

Emmanuel Swedenborg

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2
Q

solar system emerged from a giant cloud of molecular gas and dust

A

collapse

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3
Q

an event upset the balance between the cloud’s internal heat and gravity

A

collapse

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4
Q

it caused the cloud to compress and collapse in on itself

A

collapse

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5
Q

rotated to conservation of momentum

A

spinning

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6
Q

size decreased due to conservation of momentum, thus spinning faster

A

spinning

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7
Q

began to assume a flat disk shape with a bulge at the center

A

flattening

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8
Q

matter aggregated towards the center of the disk, turning very dense and hot

A

flattening

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9
Q

in the cooler spaces far from the center, molecules began to condense into solid or liquid droplets

A

condensation and accretion

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10
Q

gave birth to the sun

A

condensation and accretion

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11
Q

that blew away the cloud’s leftover materials that didn’t form planets

A

condensation and accretion

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12
Q

the solar system was formed through five stages

A

nebular hypothesis

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13
Q

how the solar system originated from a close encounter or collision between the sun and another heavenly object

A

encounter hypothesis

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14
Q

materials formed a cloud of debris that was ____ in the middle portion and ___ at the end

A

thick - thin

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15
Q

began to orbit around the sun and eventually formed into planets

A

sun star encounter

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16
Q

succession of bolts was torn from the sun by the gravity of the passing star

A

planetesimal hypothesis

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17
Q

blots from the far side of the star went to where

A

nearer distances

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18
Q

bolts from the near side of the star went to where

A

farther distances

19
Q

these bolts grew larger by gathering the

A

planetesimals, smaller, scattered bodies

20
Q

incorporated components of nebular hypothesis

A

protoplanet hypothesis

21
Q

_____ in the rotation of the nebula raised the whirlpools of gas in the _____

A

non uniformity - rotating mass

22
Q

whirlpools of gas condensed into protoplanets

A

protoplanet hypothesis

23
Q

did not explain adequately the chemical and physical differences of the planets

A

protoplanet hypothesis

24
Q

he proved that the differences in chemical and physical composition because of temperature

A

harold urey

25
gases are in constant motion
terrestrial planets
26
lost a huge chunk of their atmosphere
terrestrial planets
27
the ___ from the sun contributed to flowing the gases away from the primordial planets
solar winds
28
composed of mostly non-volatile metals and silicate rocks
terrestrial planets
29
relatively small, rotate quite slowly on their axes
terrestrial planets
30
far from the sun
jovian planets
31
jovian planets are initially what
cool
32
retained most of their gases
jovian planets
33
captured gases that escaped from terrestrial planets
jovian planets
34
composed of gases mostly what
hydrogen and helium
35
they aren't very dense and rotate fairly rapidly on their axes
jovian planets
36
where is much of the mass of the solar system concentrated at
center
37
the orbit of the planets are on the
same plane
38
all planets _____ the sun
revolve
39
the periods of revolution ____ with _____ distance from the sun
increase - increasing
40
all planets are located at where
regular intervals from the sun
41
planets rotate in what motion
prograde
42
rotates in the same direction as the orbit
proograde
43
planets revolve around what clock motion
counterclockwise
44
inner terrestrial planets are composed of what materials
high melting points (nickel and silicates)