32 AUSTRALIAN SKY & TELESCOPE January 2018
8: NASA / JPL / SPACE SCIENCE INST. / JASON MAJOR; 9 & 11: NASA / JPL / SPACE SCIENCE INST.; 10: NASA / JPL / UNIV. OF ARIZONA
/ UNIV. OF IDAHO
10.GEOMETRIC ODDITYDiscovered by Voyager
2in1981,thehuge,hexagon-shapedcloudpattern
surroundingSaturn’snorthpoleremainsanenigma.
Here’showitlookedtoCassinionNovember27,2012.
Computersimulationshaveshownthatashallow
eastward-movingjetnearthepole,likeoneofthejet
streamsinEarth’satmosphere,candevelopintoa
hexagonal pattern.
11.RHEA IN TRANSITSaturn’s two largest moons,
Titan(5,150kmacross)andRhea(1,528km),appear
tobestackedontopofeachotherinthistrue-colour
scene recorded June 16, 2011. Titan’s dense, nitrogen-
dominatedatmospheresportsadetachedhazelayer
(seenatupperright)knownastheNorthPolarHood.
12.TITAN REVEALEDCassini visited Saturn’s biggest
moon often, making 127 flybys in all. Ordinarily cloaked by
opaquehaze,thesurfaceofTitanemergesintoviewwhen
seen at infrared wavelengths. This view shows terrain
that is mostly on the moon’s Saturn-facing hemisphere.
Several places show more details than elsewhere because
the spacecraft took those images when closer to Titan
during its November 13, 2015, flyby. The scene features
the dark, dune-filled regions named Fensal (toward north)
and Aztlan (closer to equator), which together form a
crude, sideways H.
- BACKLIT BEAUTY Saturn’s backlit rings, gauzy
Titan, and Enceladus created this dramatic scene
on June 10, 2006. Hazes in Titan’s thick atmosphere
scatter sunlight to encircle the disk. The crescent of
Enceladus encroaches slightly along its lower-right limb,
with eruptive plumes faintly visible at its bottom. In this
viewing geometry, the brightest parts of the rings are
otherwise tenuous features that are rich in tiny, forward-
scattering particles.
appearance results from a feedback loop driven
by ice’s faster evaporation from dark regions
than from bright ones. This ‘thermal runaway’
began billions of years ago, when Iapetus’s
leading hemisphere was coated with dust blasted
from the surfaces of Saturn’s even-more-distant
irregular moons, the biggest of which is Phoebe.
Cassini flew close to Phoebe during its initial
approach to Saturn and measured the moon’s
density, which is higher than is typical of
Saturn’s ice-dominated satellites. By implication,
Phoebe must have a rock-and-ice composition
more like that of Pluto, suggesting that this
moon originally orbited the Sun before being
captured by the planet’s powerful gravity.
Like Earth, Saturn has aurorae near its poles
produced by the interaction between its magnetic
field and the solar wind. The aurorae cause Saturn
to emit radio waves whose strength varies as the
10.
13.
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CASSINI’S SATURN