Chapter 6 Flashcards

1
Q

what does the solar system look like?

A
  • some planets have unusual tilts, large moons, or moons with unusual orbits
  • some planets are rocky and some are large hydrogen rich jovian planets
  • swarms of asteroids and comets populate the solar system (steroids between mars and Jupiter, oort cloud (even more comets))
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2
Q

planets are are very tiny compared to what?

A

distances between them

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3
Q

Describe the Sun..

A
  • over 99.8% of solar system’s mass
  • 100 times bigger than the sun
  • made mostly of Hydrogen and Helium gas (plasma)
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4
Q

Describe Mercury…

A
  • made of metal and rock: large iron core
  • desolate, cratered; long, tall, steep cliffs, no moon
  • very hot and very cold: 425C during day and 170C at night
  • closest to the sun
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5
Q

Describe Venus…

A
  • is it the hottest bc of thick atmosphere
  • nearly identical size to earth
  • no moon
  • extreme green house effect
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6
Q

Describe Jupiter

A
  • father from sun than inner planets
  • No solid surface (mostly H/He) like sun
  • 300 times more massive than earth
  • many moons and rings
  • jupiter has 4 galilean moons
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7
Q

Four Galilean moons

A
  • Io ; active volcanoes all over
  • Europa; possible subsurface ocean
  • Ganymede; Largest moon in solar system
  • Callisto- a large cratered “ice ball’
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8
Q

Jovian ring systems

A
  • all four jovian planets
  • others have ring particles that are smaller and darker than saturn’s
  • jovian ring system just means they have moons
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9
Q

Icy bodies are

A

many icy bodies like pluto, beyond neptune (kuiper belt objects)
-largest ones are compared to the earths moons (eris is bigger than pluto)

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10
Q

pluto and other dwarf planets

A
  • icy comet like composition

- much smaller than other planets

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11
Q

major planet types

A
  • terrestrial planets are rocky, relatively small and close to the sun
  • jovian planets are gaseous, larger, and farther from the sun
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12
Q

why are there two major types of planets?

A

-most mass is h/he 98%

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13
Q

inside of the frost line

A

too hot for hydrogen compounds to form ice

  • hydrogen compounds stay gaseous
  • metals and rocks condense
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14
Q

outside of the frost line

A

cold enough for ice to condensate

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15
Q

Formation of terrestrial planets

A
  • small particles of rocks and metal were present inside the frost line
  • planetesimals of rocks and metal built up as these particles are collided
  • they collide and they make planets
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16
Q

gravity draws planetesimals together to form

A

planets

17
Q

this process of assembly is called

A

accretion

18
Q

formation of jovian planets

A
  • ice could also form small particles outside the frost line
  • larger planetisimals and planets were able to form
  • the gravity of these larger planets was able to draw in surrounding H and He gases.
19
Q

where did steroids and comets come from?

A
  • left over from the accretion process
  • rocky steroids inside frost line
  • icy comets outside frost line
20
Q

solar system is how old?

A

4.5 billion years (age dating meteorites that are unchanged)

21
Q

when did planetesimals bombarded other objects?

A

late stages of solar system formation

22
Q

the origin of earths water

A

icy planetesimals from the outer solar system

23
Q

how do we explain the existence of our moon and other exceptions to the rules?

A
  • captured them (planetesimals)

- giant impact

24
Q

Gravitational Tugs

A
  • suns motion depends on the planets tugs
  • astronomers who measured this motion around the stars could determine masses and orbits of all planets
  • (gravitational change bc planets are changing position)
25
Q

Astronomic Technique

A
  • detecting planets by measuring the change in a star’s position in the sky
  • however these tiny motions are difficult to measure
26
Q

Doppler Technique

A
  • measuring a star’s doppler shift can tell us its motion towards and away from us
  • current techniques could measure motions as small as 1 m/s
27
Q

first extrasolar planet detected

A
  • short period means small orbital distance
  • first planet was discovered in 1995
  • monitors 1 star
  • moving away from us every 4 days
28
Q

the bigger the planet

A

the easier it is to see its light

29
Q

a transit is when

A

a planet crosses in front of a star (edge on)

30
Q

the resulting eclipse

A

reduces the stars apparent brightness and tells us the planets radius

31
Q

what can be obtained when there is no orbital tilt?

A

accurate measurement of planet mass can me obtained

32
Q

Hot Jupiters

A
  • close to star

- 5 AU from sun