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Atmospheres of Uranus and Neptune

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Equator receives slightly less solar energy than poles. Planet radiates slightly more energy than it ... Zonal Winds. Far fewer bands than on Jupiter and Saturn ... – PowerPoint PPT presentation

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Title: Atmospheres of Uranus and Neptune


1
Atmospheres of Uranus and Neptune
  • Sam Williams
  • http//www.cs.berkeley.edu/samw/249/

2
Energy
  • Uranus
  • Equator receives slightly less solar energy than
    poles
  • Planet radiates slightly more energy than it
    receives (13)
  • Significantly more energy emitted than absorbed
    at equator
  • Neptune
  • Equator receives about twice as much solar energy
    as the poles
  • Planet radiates more than twice the energy it
    receives (internal heat source), and about the
    same as Uranus radiates.

3
Appearance (Uranus)
  • To the unaided eye, it appears uniform, but there
    are slight color variations
  • Photochemical meteor/ring dust haze in
    stratosphere?

4
Appearance (Uranus)
  • In IR, features are more pronounced

5
Appearance Neptune
  • High altitude clouds

6
Appearance (Neptune)
  • Neptune shows color variation in bands
  • Also, As season progresses, southern bands
    brighten (near IR)

7
Composition
  • Uranus
  • 83 H2 15 He 2 CH4
  • Neptune
  • 79 H2 18 He 3 CH4
  • Traces of N2, HCN, H2S, NH3, CO
  • 30-40x solar ratio of CH

8
Zonal Winds
  • Far fewer bands than on Jupiter and Saturn
  • Uranus -100m/s(10o), 0(-15o,30o), 175(-50o)
  • Neptune -300m/s(0o), 0(50o), 225(75o)
  • Less sunlight less turbulence flow less
    disturbed

9
Temperature
  • Tropopause 55K
  • Stratosphere on Uranus is less than 75K until
    1mbar (cooler than Neptune), but more recent IR
    observations have shown a warming in the
    stratosphere.
  • Methane, ethane, acetylene act as coolants in
    stratosphere, similar mesospheric temperature
    (150K)

10
Processes
  • Ethane (C2H6), ethylene (C2H4), acetylene (C2H2)
    from methane photodissociation.

11
Processes
  • Uranus micrometeorites bring CO and H2O to the
    stratosphere. (French group using VLTESO)
  • Neptune N2 in stratosphere (accretion from
    Triton/rapid upward convection)

12
Clouds
  • methane ice (CH4) lt1bar
  • (limit of probing)
  • Probably have
  • Methane droplets?
  • hydrogen Sulfide (H2S) 2-5bar
  • more H2S, so no NH3 clouds?
  • NH4 hydrosulfide (NH4SH) 15-30bar
  • water 15-50bar
  • Solution Cloud to a few 100bar

13
Great Dark Spot
  • Comparable in size to GRS
  • Storm? (1200mph, counterclockwise rotation,
    anticyclone)
  • Below the tropopause
  • Moved towards equator, dissipated, new one formed
    in the northern hemisphere

14
Great Dark Spot
  • Hole in the methane droplet cloud deck?
  • Like the ozone hole over Antarctica?
  • What would destroy methane in that spot?
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