Uranus Flashcards

1
Q

uranus physical characteristics

  • diameter
  • avg. dist. from sun
  • mass
  • orbital pd
  • rotational pd
  • # of moons
  • magnitude
A
  • diameter = 4 x earth
  • avg. dist. from sun = 19 AU
  • mass = 14.5 x earth
  • orbital pd = 84 yrs
  • rotational pd = 17.25 days; differential; retrograde
  • # of moons = 27
  • magnitude = 5.3
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2
Q

uranus atmosphere (4)

A
  • bland, blue-green world bc methane absorbs red light
  • mostly hydrogen w/ some methane & high-altitude haze
  • under haze = clear air w/ methane clouds
  • presence of lightening
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3
Q

axial tilt (3)

A
  • rotation axis = tilted 98 degrees from orbit perpendicular
  • north pole = titled below orbital plane
  • extreme tilt = cause for seasonal variations in its weather
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4
Q

retrograde rotation (2)

A
  • as it orbits the sun, n. & s. poles alt. point directly toward or away from the sun
    • gives uranus very long seasons (about 20 years each)
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5
Q

interior (3)

A
  • 3 layers
  • atmosphere lies atop 1st layer
  • little ammonia in atmosphere bc it is dissolved in 2nd water layer
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6
Q

3 interior layers

A

1- outer 30& = liquid hydrogen & helium
2- next 40% inward = highly compressed liquid water w/ some methane & ammonia
3. inner 30% = rocky core

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7
Q

alternate interior description (2)

A
  • new evidence says 2nd layer is nonexistent

- composed of rock & ices w/ only 15% hydrogen & little helium

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8
Q

magnetic field (3)

A
  • @ cloud tops = 3/4 strength of earth’s field
  • magnetotail is twisted by uranus’ rotation into corkscrew shape
  • field’s source is unknown
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9
Q

magnetic field’s axis tilt (4)

A
  • field tilted 59 degrees from rotation axis
  • field’s axis doesnt pass thru center of planet (unusual)
    • means field wobbles as uranus rotates
    • wobble allows rotation rate of interior to be measured
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10
Q

magnetic field’s rotation rate (2)

A
  • uranus’s field rotates in 17 hr & 14 min

- cloud layers rotate in 16 hrs & 30 min

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11
Q

ring system (6)

A
  • orbited by 13 thin, dark rings
  • each ring composed of ringlets
  • orbit in plane of equator
  • held in orbit by shepherd moons
  • has a pair of giant rings
  • dim & dark bc they’re mostly dust rather than ice
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12
Q

moons

A

-most orbit in plane of uranus’ equator

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13
Q

miranda description & orbital pd (2)

A
  • innermost & smallest of major moons

- orbits in 1.5 days

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14
Q

miranda composition (2)

A
  • 1/2 water ice

- remainder divided b/t rock & methane-related organic compounds

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15
Q

miranda surface (3)

A
  • surface = unusually wrinkled & banded features
  • varied terrain = broken into many pieces by impact, then pieces re-coalesced
    • or tidal heating moved lg. pieces of the crust
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16
Q

titania (3)

A
  • largest of uranus’ moons
  • orbits in 8.75 days
  • huge canyon (same class as mariner valley on mars)
17
Q

titania composition (3)

A
  • 50% water ice
  • 30% rock
  • 20% methane-related organic compounds
18
Q

ariel (4)

A
  • orbits in 2.5 days
  • regions of fresh frost
  • devoid of impact craters
  • intense geological activity has produced huge network of fault canyons & liquid water outflows over its surface
19
Q

ariel composition (3)

A
  • 50% water ice
  • 30% rock
  • 20% methane ice
20
Q

umbriel (3)

A
  • orbits in 4 days
  • darkest surface of uranus’ moons
  • least geologically active
21
Q

umbriel composition (3)

A
  • mostly composed of water ice
  • balance made up of rock & methane ice
    • most of methane ice is on its surface
22
Q

oberon (4)

A
  • outermost of major moons
  • 2nd largest & 2nd most massive of major moons
  • orbits in 13.5 days
  • old, heavily cratered icy surface
23
Q

oberon composition (3)

A
  • 50% water ice
  • 30% rock
  • 20% methane-related carbon/nitrogen compounds
24
Q

spacecraft visitor

A

voyager 2 = only one to visit uranus