Encyclopedia of the Solar System 2nd ed

(Marvins-Underground-K-12) #1
Atmospheres of the Giant Planets 389

FIGURE 4 Vertical profiles of photochemical species in the
Neptunian stratosphere. (From P. Romani et al., 1993,Icarus
106 , 442–462. Copyright by Academic Press.)


Tropical Zones, are persistently bright, whereas others,
like the South Equatorial Belt, are sometimes bright and
sometimes dark. On Jupiter, there is a correlation between
visible albedo and temperature, such that bright zones are


usually cool regions and dark belts are usually warm near
the tropopause. Cool temperatures are associated with adi-
abatic cooling of upwelling gas, and the correlation of cool
temperatures with bright clouds points to enhanced con-
densation of ice particles as condensable gases flow up-
ward and cool. This correlation does not hold completely
on Jupiter and almost not at all on the other giant plan-
ets. The mechanisms responsible for producing reflectivity
contrasts and color remain largely mysterious, although a
number of proposals have been advanced. These will be
discussed in more detail.
Our understanding of aerosols and clouds is rooted in
thermochemical equilibrium models that predict the tem-
perature (and hence pressure and altitude) of the bases of
condensate clouds. The cloud base occurs where the vapor
pressure of a condensable gas equals its partial pressure.
Model predictions for the four giant planets are shown in
Fig. 6. The deepest cloud to form is a solution of water and
ammonia on Jupiter and Saturn, with dissolved H 2 S as well
on Uranus and Neptune. At higher altitudes, an ammonium
hydrosulfide cloud forms, and its mass depends on both the
amounts of H 2 S and NH 3 available and the ratio of S to N.
At still higher altitudes, an ammonia or hydrogen sulfide
cloud can form if the S/N ratio is less than or greater than
1, respectively. If the ratio is greater than 1, all the N will
be taken up as NH 4 SH, with the remaining sulfur avail-
able to condense at higher altitudes. This seems to be the
situation on Uranus and Neptune, but the reverse is true
for Jupiter and Saturn. Only the atmospheres of Uranus

FIGURE 5 Voyagerimages of
Jupiter, Saturn, Uranus, and
Neptune, scaled to their relative
sizes. Earth and Venus are also
sown scaled to their relative sizes.
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