Final Flashcards

1
Q

Meteorites

A

Rocks that fall from the sky (mostly astroid fragments)

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2
Q

Astroids

A

Rocky bodies that orbit in the inner solar system, most are located in the asteroid belt

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3
Q

How big are largest astroids

A

few hundered kilometers

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4
Q

Kirkwood gaps

A

empty areas with no astroids due to jupiter’s ressonances

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5
Q

Meteor

A

phenomenon of a flash in the sky

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6
Q

Comets parts

A

Nucleus, coma, ion-tail, plasma tail, hydrogen cloud (be able to draw this

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7
Q

Oort cloud

A

10^12 comets sent by jupiter (10^4 AU away)

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8
Q

Comet composition

A

dirty ice or maybe icy dirt

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9
Q

Biggest Kuiper Belt Object?

A

Pluto – discovered by lowells calculations of the perturbations to neptune’s orbit (but those calculations were in error)

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10
Q

Planetary Rings composed of?

A

Billions of small particles in orbit around a body.

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11
Q

Why are rings flat?

A

Collisions dissipate energy and cause the rings to be flat

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12
Q

Optical Depth equation

A
I = Io exp(-T) where T=n*Pi*a^2*H
n = number per vol
a = radius (cross section)
H = thickness
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13
Q

What is Roche Limit

A

inside this, planets ties are stronger than gravity holding objects together

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14
Q

Roche limit eq

A

r

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15
Q

What is found in the roche zone

A

rings

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16
Q

Ring natural frequencies

A

mean motion, epicyclic motion, and vertical oscillation

17
Q

Empty Cylinder Argument

A

If we have uniformly randomly distributed particles, the probability of volume, V, being empty is a poisson eq

18
Q

Empty Cylinder Eq

A

P(o) = exp(-T) where T = nopia^2*H

19
Q

How do rings and moons interact

A

Waves sheppard edges, there is possibly recycling between moons and rings

20
Q

Ring Origins

A

Moon break-up or frustrated accretion, or comet came to close and broke up

21
Q

Are rings young or old?

A

Could be either, maybe young, or maybe recycled

22
Q

Jupiter Rings

A

tenuous, dusty

23
Q

Saturn Rings

A

broad, thick, made of ice

24
Q

Uranus Rings

A

narrow, dark

25
Q

Neptune Rings

A

dusty, hyphenated, ring arcs

26
Q

Planet formation steps (9 steps)

A
  1. Giant molecular cloud collapses, fragments
  2. solar nebula surrounds proto-sun
  3. solids condense, ices outside of frost line
  4. grains accrete to form planetesimals
  5. great collisions reduce planet number
  6. giand planet cores trap gas
  7. moons and rings form in mini nebula around planets
  8. continued accretion and impacts clean up solar system
  9. solar wind blows away leftover gas
27
Q

Parallels to planetary rings

A
  1. Flat, low temperature
  2. accretion in both
  3. Embedded bodies interact with disk: propellers, gaps, density waves
  4. Angular momentum transfers and cause planet migration (explains ‘hot jupiters’)
  5. Gian planets may kill smaller ones before star turns on
28
Q

Temperature Equilibrium Eq

A

Teq = [ Fo/rau^2 (1-Ab)/(4eps*sig)]^1/4

29
Q

multiple plate tectonic resurfacing time eq

A

T = circumference / (number of plates * rate)

30
Q

Volcanic resurfacing rate equation

A

R = num of volc * rate / surfarea

31
Q

Comparitive Planetology

A
  • suffered late heavy bombardment,
  • early stage of basaltic volcanism,
  • smaller planets have cooled and are now geologically dead.
  • Maria indistinguishable (moon, mercury, mars)
  • venus, earth were similar when life arose
32
Q

mafic rocks

A

more magnesium and iron, denser, more viscous, darker

33
Q

sialic rocks

A

lighter, more viscous, brighter

34
Q

keplers 3 laws

A
  1. all planets move in elliptical orbits around the sun
  2. orbit sweeps out area at a constant rate
  3. harmonic law p^2 = a^3
35
Q

Def of planet

A

orbits the sun, spherical, has cleared the neighborhood around it, orbit

36
Q

Why is pluto not a planet

A
  1. orbit is eccentric an inclined
  2. small size (2/3 or the moon)
  3. composition of rock and ice