Rings, comets, asteroids, belts, and creation Flashcards

1
Q

Planetary rings are on what planets

A

-all 4 jovian planets

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2
Q

Roche limit and rings

A

-rings lie within the Roche limit
-the distance from planet within, which tides break apart a satellite

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3
Q

Planetary rings

A

-all made up of small particles
-all ringed planet’s rings are made up of dark dust except Saturn’s which is made up of “rocks” of water ice

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4
Q

rings of Jupiter

A

-made of dust from moons

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5
Q

rings of saturn

A

-complex rings
-has rings we cant see (called diffuse rings)
-thousands of narrow rings and gaps
-embedded moons in gaps

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6
Q

Saturn’s rings (ABC system)

A

-A and C are translucent
-B is solid
-C has a division due to the moon mimas in it
-F ring is guarded by Shepard satellites

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7
Q

Uranus and Neptune’s rings

A

-narrow
-not uniform

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8
Q

2 asteroid belts

A

-Kuiper belt and Oort cloud

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9
Q

asteroids

A

-most lie in “main belt” which is 2.1-3.3 AU away between Mars and Jupiter
-orbits are jumbled and crossed
-few big, many small
-biggest is Cercus (still smaller than moon)

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10
Q

asteroid families

A

-groups of asteroids with similar orbits
-could be collision fragments

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11
Q

asteroid shapes and reason

A

-largest are round due to gravity
-smaller are irregular due to less gravity to pull together

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12
Q

reflection spectrum

A

-used to detect what asteroids are made of

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13
Q

3 main spectral classes

A

-C: outer belt, 3% dark flat carbon rich
-S: inner belt 15% dark flat silicates and iron
-M: outer belt 10% dark reddish iron

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14
Q

cercus

A

-large asteroid
-heavily cratered, spherical
-photos taken by Dawn spacecraft
-metallic core and rocky mantle

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15
Q

Vesta

A

-3rd largest asteroid
-almost spherical, heavily cratered
-metallic core and rocky mantle

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16
Q

Mars’s asteroids/moons

A

-captured satellites
-phoebes and Deimos

17
Q

Apollos

A

-earth crossers
-may collide with earth
-from main belts and comets

18
Q

Hilda’s resonance group

A

-dark, red
-unlike main belt asteroids
-define outer edge of main asteroid belt

19
Q

Trojan asteroids

A

-shares Jupiter’s orbit
-leads and trails Jupiter by 60 digress
-dark, very red, unlike main asteroid belts
-more like comets?

20
Q

asteroids are…

A

-leftover rocky pieces of planet building material from inner solar system

21
Q

comets are…

A

-icy pieces of planet building material from outer solar system
-mostly in Kuiper belt

22
Q

Kuiper belt

A

-30-50 AU away
-around 1000 icy objects (most likely more than 7000)
-orbits are jumbled
-includes Pluto and its moons

23
Q

Pluto and Charon

A

-Charon is pluto’s moon

24
Q

Pluto

A

-discovered in 1930
-N ice surface and water beneath
-heart shaped smooth ice

25
Q

charon

A

-water surface
-organic tars on planet

26
Q

Eris (Kuiper belt)

A

-bigger than Pluto
-water and methane ice

27
Q

Quaoar

A

-half the size of Pluto
-spectrum shows crystalized water ice

28
Q

Oort Cloud

A

-50,000 AU
-edge of suns gravity control

29
Q

What makes a comet

A

-The nucleus is a dirty ice ball a few miles across (just remember water ice with carbon)

30
Q

A comets travel

A

-starts far from the sun frozen and invisible
-moves in towards sun and heats up and begins to evaporate

31
Q

Making the coma of the comet

A

-some ice evaporates and some dirt is carried off forming a cloud/ coma around the nucleus
-a huge invisible hydrogen cloud surrounds the coma

32
Q

2 tails of the comet

A

-the dust tail is made from dust being pushed off by light
-the gas tail is made from being pushed by solar wind
-both point away from the sun

33
Q

the key to the creation of the solar system is…

A

temperature