Chapter 8 Flashcards

1
Q

jupiter and saturn are mostly what gases?

A

H and He gas

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2
Q

Uranus and Neptune mostly what?

A

mostly hydrogen compounds; water H2O, CH4, NH3

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3
Q

Uranus has most extreme what?

A

seasonal change (rotation/tilt)

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4
Q

Jovian planet formation

A

beyond the frost line planetesimals could form ice

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5
Q

Hydrogen compounds are ________ than rock/metal so jovian planets got ______ and acquired H/He atmospheres

A

more abundant
got bigger
(more massive but less dense than terrestrial planets)

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6
Q

Jovian cores are very similar

A

mass of 10 earths

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7
Q

Jovian planets differ in the amount of?

A

H/He accumulated

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8
Q

timing : the planet that forms earliest captures what?

A

he most Hydrogen and helium gas

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9
Q

capture ceases after what?

A

the first solar wind blows the left over gas away

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10
Q

Location : the planet who forms in the denser part of the nebula what?

A

forms its core first

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11
Q

density differences: why are uranus and neptune denser than saturn?

A

they have less h/he gas and more hydrogen compounds and rocks, proportionately

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12
Q

jupiter is denser than saturn :

adding mass to a jovian planet ______ the underlying gas layers

A

compresses

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13
Q

greater compressions is why jupiter is not much larger than saturn

A

although it is 3 times more massive

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14
Q

jovian planets with even more _____ can be ______ than jupiter

A

mass

smaller

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15
Q

what are jovian planets like on the inside?

A

internal heat: from gravitational potential energy into thermal energy by contracting

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16
Q

describe the interiors of jovian planets

A
  • no solid surface
  • high pressure and high temperatures
  • cores made up of hydrogen and compounds, metals and rocks
  • layers are differnt for planets
17
Q

inside jupiter

A
  • the core is thought to be made of rock, metals, and hydrogen compounds
  • core is the same size as earth but 10x more massive
18
Q

jupiters atmosphere

A
  • hydrogen compounds in Jupiter form clouds

- different cloud layers corresponds to freezing points of different hydrogen compounds

19
Q

methane gas on neptune and uranus absorbs

A

red light but transmits blue light

20
Q

blue lights reflects off ______ making those planets look blue

A

methane clouds

21
Q

jupiters great red spot

A
  • a storm twice as wide as earth

- has existed for at least 3 centuries

22
Q

Ios Volcanoes

A

volcanic eruptions continue to change ios surface, impact craters have all been buried in lava flows

23
Q

tidal heaing

A

Io is squished and stretched as its orbits jupiter causing volcanoes

24
Q

io orbits around jupier in how many days?

A

1 1/2, highly elliptical

25
Q

Europas interior also warmed by ______

A

tidal heating

26
Q

titans is the only moon in the solar system that….

A

has a thick atmosphere

27
Q

titans atmosphere consists mainly of ?

A

nitrogen, with some argon, methane and ethane

28
Q

what provided the first look at titans surface?

A

Huygens probe in 2005

29
Q

what did titans surface have?

A

liquid ethane/methane, “rocks” made of ice

30
Q

neptunes moon triton is similar to what?

A

pluto but bigger

31
Q

what does triton have?

A
  • evidence for past geological activity
  • thin atmosphere
  • coldest large moon
32
Q

jovian planets all have what?

A

ring systems, others have ring particles that are smaller and darker than saturn

33
Q

what are planetary rings like?

A

nearer to the planet than any of the planets large moons

-orbiting equatorial plane of their planet

34
Q

what are saturns rings like?

A

they are made of numerous, icy individual particles
they orbit over the equator
they are very thin (flattening via collisions)

35
Q

rocky planets vs icy moons

A

-rocks melt at higher temp.
- only large planets have enough heat for activity
-

  • ice melts at lower temperatures
  • tidal heating can melt internal ice, driving activity