JUPITER: King of the Planets - PowerPoint PPT Presentation

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JUPITER: King of the Planets

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JOVIAN (GAS GIANT) PLANETS SATURN Nearly as big as Jupiter, and it rings very nicely. Cassini image of Saturn, edge-on rings, their shadows, & moons Dione & Enceladus ... – PowerPoint PPT presentation

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Title: JUPITER: King of the Planets


1
JOVIAN (GAS GIANT) PLANETS
2
SATURN
  • Nearly as big as Jupiter, and it rings very
    nicely.
  • Cassini image of Saturn, edge-on rings, their
    shadows,
  • moons Dione Enceladus

3
SATURN Ringed and Very Gassy
  • Mass is 95.2 times that of Earth.
  • Radius is 60,268 km or 9.45 times Earth's.
    Density is only 0.687 g/cm3 or 0.125 of Earth's.
  • The most distant naked eye planet.
  • Period of 29.42 years.
    Semi-major axis, a 9.54 AU,
    e 0.054. Inclination to ecliptic 2.49 deg
  • 9 moons discovered from the ground.
  • No solid surface differential rotation
    Magnetic (interior) spin period 10h 40m
    Spins so fast is so gassy that its
    ellipticity gt 10 axial tilt 26.7 deg

4
Rings and Orbit
Rings are prominent tilted at 27 degrees so seen
from different angles from Earth nearly
invisible when edge-on
5
Saturn's Atmosphere and Interior are Very Similar
to Jupiter's
  • BUT the main interior differences include
  • Lower density less mass so less compression and
    relatively more gaseous
  • Molecular H2 layer ? 30,000 km thick Metallic
    H layer ? 15,000 km thick Rocky/metallic core, R
    ? 15,000 km
  • Central T 15,000 K P 5 x 106 atm
  • Strong magnetic field, but still only 5 of
    Jupiter's.

6
Saturns Interior
7
Saturns Atmospheric Differences from Jupiter
  • Fewer belts and zones (due to lower T) but faster
    winds (to 1500 km/h) Thicker cloud
    layers (lower gravity) Less
    coloration (probably due to lower T)
  • In atm H2 over 92, He almost 8 Why?
  • He has settled or rained downwards.
    At the lower T and P of Saturn's atm,
    He doesn't dissolve in H2 Separation of He
    and compression of whole planet yields much more
    heat, so Saturn's surface T is 97 K, not 74 K.

8
Saturns Atmosphere
  • Real color from HST showing storm near equator
    and pole at earlier time.
  • False color image from IR blue, haze free
    green, more haze orange, high clouds

9
Atmospheric Structure and Fast Winds
10
URANUS and NEPTUNE
  • Most Distant Official Planets are NEARLY TWINS
  • MU 14.54 M? MN 17.15 M? .
  • RU 25,559 km or 4.01 times Earth's.
  • RN 24,766 km or 3.88 times Earth's.
  • ?U 1.27 g cm-3 ?N 1.64 g cm-3 .

11
As seen from Earth, URANUS
  • Discovered by Wm. Herschel in 1781 (barely
    visible to naked eye, greenish, nearly
    featureless)
  • Period of 83.75 years
  • Semi-major axis 19.19 AU, e 0.047
  • 5 moons discovered from the ground pre-space 10
    by Voyager, 2 more by 200-inch.
  • Tilted by 98 deg ? LONG seasons
  • Magnetic (interior) spin period 17.2 h
    (retrograde)

12
Seasons on Uranus
  • Axis almost in orbital plane so equatorial zones
    have two summers near equinoxes and two winters
    near solstices poles have 42 yr of light and 42
    years of dark

13
Rotation on Uranus
  • HST shows cloud motions over 8 hours
  • IR HST picture shows clouds and rings

14
As seen from Earth, NEPTUNE
  • Predicted by John Adams (1845) and Urbain
    Leverrier (1846) producing growing error in
    Uranus's position noticed over the years
  • Found in the right place by Johann Galle in Sept.
    1846 -- bluish, tiny disk Voyager showed some
    bands
  • P163.7 yr a 30.07 AU e0.009
  • 2 moons discovered from the ground 11 from space
  • Magnetic (interior) spin period 16.1 h surface
    17.3 h

15
ATMOSPHERES
  • Temperatures Uranus, 58 K Neptune 59 K
  • Both Uranus and Neptune are about 84 H2 and 14
    He.
  • Methane (CH4 ) is most of the remainder
    Methane absorbs red light, so planet looks
    blueish/green More CH4 in Neptune, so it's bluer
    Ammonia is frozen out in
    these very cold atmospheres
  • No internal heat source for Uranus, so washed out
    bands and zones covered by a haze. Fairly
    strong winds distribute Sun's heat so sunny side
    isn't much hotter than shady side.
  • Neptune has an internal heat source probably
    extra methane has helped to trap internal heat of
    formation ?more noticeable bands and some storms

16
Neptunes Dark Spot (from Voyager) and
Cloudsfrom IR HSTviews showing brightening as
more sunlight hits South side
17
Interiors of Uranus and Neptune
  • Below atmospheres, each about 1/3 of R
  • MOLECULAR HYDROGEN (unlikely to convert to metal)
  • below that, SLUSH, including water ice and
    dissolved ammonia an electrically conducting
    fluid
  • ROCKY CORE (maybe 10 M? )

18
Magnetic Fields
  • Despite not having (much) metallic hydrogen both
    have substantial internal fields (100 times
    earth's, 1/10th Saturn)
  • Off-center and misaligned with spin axis (60O for
    Uranus, 46O for Neptune, vs. 10O for Jupiter and
    well-aligned for Saturn).
  • Why? currently reversing reflecting a blow
    ionic NH3 ?
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