Solar System Flashcards

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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
Q

gases are in constant motion

A

terrestrial planets

26
Q

lost a huge chunk of their atmosphere

A

terrestrial planets

27
Q

the ___ from the sun contributed to flowing the gases away from the primordial planets

A

solar winds

28
Q

composed of mostly non-volatile metals and silicate rocks

A

terrestrial planets

29
Q

relatively small, rotate quite slowly on their axes

A

terrestrial planets

30
Q

far from the sun

A

jovian planets

31
Q

jovian planets are initially what

A

cool

32
Q

retained most of their gases

A

jovian planets

33
Q

captured gases that escaped from terrestrial planets

A

jovian planets

34
Q

composed of gases mostly what

A

hydrogen and helium

35
Q

they aren’t very dense and rotate fairly rapidly on their axes

A

jovian planets

36
Q

where is much of the mass of the solar system concentrated at

A

center

37
Q

the orbit of the planets are on the

A

same plane

38
Q

all planets _____ the sun

A

revolve

39
Q

the periods of revolution ____ with _____ distance from the sun

A

increase - increasing

40
Q

all planets are located at where

A

regular intervals from the sun

41
Q

planets rotate in what motion

A

prograde

42
Q

rotates in the same direction as the orbit

A

proograde

43
Q

planets revolve around what clock motion

A

counterclockwise

44
Q

inner terrestrial planets are composed of what materials

A

high melting points (nickel and silicates)