Chapter 6 : Formation of Solar System Flashcards

1
Q

Formation Theory Property 1

A

Patterns of motion of the large bodies
- orbit in the same direction and plane

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2
Q

Formation Theory Property 2

A

Existence of two types of planets
- Terrestrial and jovian

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3
Q

Formation Theory Property 3

A

Existence of smaller bodies
- asteroids and comets

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4
Q

Formation Theory Property 4

A

Notable exceptions to usual patterns
- rotation of uranus, earth’s moon

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5
Q

nebular theory

A

states our solar system formed from the gravitational collapse of a giant interstellar gas cloud (solar nebula)

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6
Q

why did the solar nebula heat up as it collapsed?

A

as the cloud shrank, its gravitational potential energy was converted to thermal energy

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7
Q

what kind of material in the solar nebula could condense at temperatures as high as 1500 K in the inner region of the nebula?

A

metals

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8
Q

Relevance of nebular theory

A

-Kant and Laplace proposed nebular hypothesis over two centuries ago
-large amount of evidence now supports this idea

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9
Q

Close Encounter Hypothesis

A

rival idea proposed that the planets formed from debris torn off the sun by a close encounter with another star

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10
Q

accuracy of close encounter hypothesis

A

does not explain observed motions and types of planets

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11
Q

Galactic Recycling

A

Elements that formed planets were made in stars and then recycled through interstellar space

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12
Q

nebular theory evidence from other gas clouds

A

we can see stars forming in other interstellar gas clouds

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13
Q

what caused the orderly patterns of motion in our solar system?

A

conservation of angular momentum and flattening

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14
Q

Conservation of Angular Momentum

A

rotation speed of cloud from which our solar system formed must have increased as the cloud contracted

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15
Q

flattening

A

collisions between particles in the cloud caused it to flatten into a disk
-spinning cloud flattens as it shrinks

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16
Q

how do collisions between gas particles effect motions?

A

-gradually reduce random motions
-reduce up and down motions

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17
Q

Why are there two major types of planets?

A

conservation of energy

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18
Q

as gravity causes cloud to contract…

A

it heats up

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19
Q

temp of inner parts of disk

A

hotter than other parts

20
Q

rock remains solid at…

A

greater temps then ice

21
Q

inside the frost line

A

too hot for hydrogen compounds to form ices

22
Q

outside the frost line

A

cold enough for ices to form

23
Q

how did terrestrial planets form?

A
  • small particles of rock and metal were present inside frost line
  • planetesimals of rock and metal built up as these particles collided
24
Q

how did gravity change the planetesimals?

A

-assembled planetesimals into terrestrial planets

25
Q

accretion, process of assembly

A

-draws planetesimals together to form planets

26
Q

how did jovian planets form?

A

-ice could form small particles outside frost line
-larger planetesimals and planets were able to form

27
Q

how did gravity affect jovian planets?

A

-gravity of larger planets and rock and ice was able to draw in surrounding H and He gases

28
Q

Where are the leftover gases?

A

a combination of photons and solar wind, outflowing matter from sun, blew away the leftover gases

29
Q

Solar rotation over time

A

in nebular theory, young sun rotated much faster than now
- friction between solar magnetic field and solar nebular thought to have slowed rotation over time

30
Q

where did asteroids and comets come from?

A

Leftovers from accretion process
- heavy bombardment

31
Q

where are rocky asteroids?

A

inside frost line

32
Q

where are icy comets?

A

outside frost line

33
Q

origin of earth’s water

A

water may have come to earth by icy planetesimals

34
Q

captured moons

A

unusual moons of some planets may be captured planetesimals

35
Q

why does our moon exist?

A

giant impact

36
Q

odd rotations explanation

A

giant impact

37
Q

how would the solar system be different if the solar nebula had cooled with a temperature half its actual value?

A

jovian planets would have formed closer to the sun

38
Q

which of these facts is not explained by the nebular theory?
a. 2 main types of planets
b. planets orbit in same direction and plane
c. existence of asteroids and comets
d. number of planets of each type

A

d. number of planets of each type

39
Q

considering only the tilt of their axis, which planet would have the most extreme seasons?

A

uranus

40
Q

how do we explain “exceptions to the rules”?

A

bombardment of newly formed planets by planetesimals may explain the exceptions

41
Q

how do you measure the age of a rock?

A

-some isotopes decay with a well-known half life
-comparing proportions of those isotopes with decay products tells us the age

42
Q

how do we know the age of the solar system?

A

-radiometric dating of meteorites indicates planets formed 4.5 billion years ago

43
Q

plasma

A

consists of gas in which many or most of atoms are ionized (missing electrons)

44
Q

what happens to energy in the sun’s convection zone?

A

energy is transported outward by the rising of hot plasma

45
Q
A