NASA/JPL-CALTECH/ASI/USGS
T
HINKING out-
side the box is
normal for most
space scientists, but
when the box includes
Saturn’s biggest moon,
Titan, ideas have to be
even more audacious
than usual. What sets Titan apart is
not mere size: it is the only world,
other than Earth, known to have large
stable bodies of liquid on its surface.
And Titan’s lakes and seas drive a
weather cycle of evaporation and rain-
fall, exactly as the oceans on Earth do.
That, however, is where the similarity
ends. With Titan’s average ambient
temperature of –180°C, the moisture in
its atmosphere is not water vapour, but a
melange of hydrocarbons that are best
thought of as liquid natural gas – ethane,
methane and other compounds. These
liquids pool in basins in Titan’s bedrock,
which is actually frozen water.
Titan’s seas and lakes dominate its
northern polar region, but there are a few
in the south too. And they are large –
comparable with North America’s Great
Lakes in the case of the three biggest,
which are designated as ‘maria’, or seas.
Some 30 smaller lakes, ranging from a
few kilometres in length to a couple of
hundred have also been identified.
The discovery and exploration of
these lakes by remote sensing from the
orbiting Cassini spacecraft has raised
questions. Are they fed by methane and
ethane springs from a ‘water table’?
Could cyclones form over the larger seas?
And do they have hydrocarbon ‘icebergs’
- as radar observations suggest?
The best way to answer these ques-
tions, says Ralph D. Lorenz, a scientist
at Johns Hopkins University in the
USA, is to send a submarine to Titan.
It would be a robotic submarine similar
to the unmanned underwater vehicles
already in use for military, scientific and
commercial purposes. And it could be
carried there by a mini space shuttle
able to glide through Titan’s thick
atmosphere – perhaps similar to the
US military’s secret X-37B space shuttle.
Exploring the sea floors of Titan to
reveal its chemical and climatic history
could be the next big step in our
understanding of the Solar System.
Are galaxies rotating? Astron-
omy has only been around for
a few hundred years; surely the
rotation measured would be so
small as to be negligible in such
a short time period?
David Frankland, Perth
You’re quite right that the visible
rotation of galaxies is infinitesi-
mally small on human timescales.
Instead, we measure their rotation
with the Doppler effect, which
shifts the wavelength of light
emitted by moving sources.
Measuring the rainbow spectra of
galaxies lets us determine their
rotational velocities very accurately.
If you have a space question for Fred,
email it to [email protected]
Fred answers
your questions
x1
NAKED EYE Venus and
Jupiter are visible, low
in the western evening sky. The
‘Goddess of Love’ is the brighter
of the planets. Their meeting with
the thin crescent on 19 July will
be impressive. In August they are
seen only early in the month.
BINOCULARS Look high
in the evening sky to
Scorpius the Scorpion. Where the
tail makes a right-angle turn is an
impressive triple star formed by
Zeta (1 and 2), Sco and HR 6266.
Its star field is rich, including the
open star cluster NGC 6231.
SMALL TELESCOPE
NGC 6397, in the
southern constellation of Ara,
is considered to be the fourth-
brightest globular star cluster in
the sky. It has a brilliant, compact
core with the stars more loosely
scattered towards the edge.
Glenn Dawes is a co-author
of Astronomy Australia 2015
(Quasar Publishing).
Glenn Dawes
looking up
x10
x10 0
Exploring the seas of Titan
Getting to the bottom of Titan’s unique geography might
require an underwater mission, says Fred Watson.
SPACE
FRED WATSON is astronomer-in-charge
of the Australian Astronomical Observatory.
Surface detail.
Cassini has captured
images of the lakes
and seas around
Titan’s north pole.
22 Australian Geographic 圀漀爀氀搀䴀愀最猀⸀渀攀琀圀漀爀氀搀䴀愀最猀⸀渀攀琀
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