Liquid Sea on Saturns Titan
Explanation:
What is this vast dark region on Titan?
Quite possible a sea of liquid
hydrocarbons.
The region was imaged earlier this month when the robotic
Cassini spacecraft
swooped past Saturn's cloudy moon and illuminated part of it with radar.
The dark region in the
above image
reflected little radar, an effect expected were the
dark surface relatively flat, as expected for a liquid.
Other indications that the vast dark area is liquid include the
coastline-like topology of the brighter regions,
which appear to include
islands, inlets,
and tributary channels.
The uninterrupted smoothness of much of the dark sea may indicate that the sea runs
deep,
with
speculation
holding a depth estimate of tens of meters.
A
hydrocarbon sea
on
Titan
holds particular interest for
exobiologists
as it might be a place where life could develop.
In 2005 the Huygens probe landed on Titan and returned the
first surface images.
Cassini will continue to explore Titan, as 13
more flybys are
planned.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
