Not exact matches
The seemingly bleak
icy surfaces of these
moons are in fact among the most
active landscapes in the solar system.
A team of researchers led by Cornell's Radwan Tajeddine examined Cassini data and found evidence that the
active south polar region of Enceladus — the fractured terrain seen here at bottom — may have originally been closer to the
icy moon's equator.
A global ocean lies beneath the
icy crust of Saturn's geologically
active moon Enceladus, according to new research using data from NASA's Cassini mission.
Cassini is scheduled to make a close flyby of Enceladus on Oct. 28, in the mission's deepest - ever dive through the
moon's
active plume of
icy material.
For example, Cassini discovered that the Saturn satellite Enceladus is a mini-world of
active jets — geyser - like phenomena that blast out water vapor and ice particles from the huge, salty ocean that lies beneath the
moon's
icy crust.
Cassini first revealed
active geological processes on Enceladus in 2005 with evidence of an
icy spray issuing from the
moon's south polar region and higher - than - expected temperatures in the
icy surface there.
The water - rich
moon is «one of the few places beyond Earth where we can watch geology happen in real time, giving us a primer for understanding other, less
active,
icy worlds,» John Spencer, a scientist at the Southwest Research Institute in Boulder, Colo., who was not involved in the study, wrote in a commentary.
According to two science papers, the results are the first clear indications an
icy moon may have similar ongoing
active processes.
Neptune's
moon Triton has
active volcanoes that do not spew out hot magma like familiar Earth - bound volcanoes do, but giant jets of
icy liquid nitrogen instead.