OpenBCM V1.08-5-g2f4a (Linux)

Packet Radio Mailbox

IZ3LSV

[San Dona' di P. JN]

 Login: GUEST





  
EI2GYB > ASTRO    26.08.21 13:02l 123 Lines 6055 Bytes #999 (0) @ WW
BID : 13615_EI2GYB
Read: GUEST
Subj: Tiger Stripes on Enceladus
Path: IZ3LSV<I3XTY<I0OJJ<GB7CIP<EI2GYB
Sent: 210826/1158Z 13615@EI2GYB.DGL.IRL.EURO BPQ6.0.22

     _        _               _   _                   
    / \   ___| |_ _ __ ___   | \ | | _____      _____ 
   / _ \ / __| __| '__/ _ \  |  \| |/ _ \ \ /\ / / __|
  / ___ \\__ \ |_| | | (_) | | |\  |  __/\ V  V /\__ \
 /_/   \_\___/\__|_|  \___/  |_| \_|\___| \_/\_/ |___/
                                                      
 "Tiger Stripes" on Enceladus could be even more unique than previously thought

Enceladus's unusual features could help scientists search for 
evidence of life outside Earth.


Enceladus, Saturn's sixth largest moon, is awash with liquid water beneath 
its icy shell. At the moon's south pole, the subsurface ocean erupts from 
one hundred geysers located along four parallel fractures known as 'tiger 
stripes.' The towering jets of ice particles form a plume that snows back 
down to the surface. Some of the ice even escapes the moon's gravity 
and forms Saturn's E-ring.

Icy moons that have (or are thought to have) subsurface oceans are 
common in the outer solar system. For example, Jupiter has several of them. 
These form when gravity from the planet they orbit stretches and squeezes 
their interior.

Scientists think that these tidal stresses generate enough heat to sustain 
the liquid water. Tidal stresses can crack the ice shell, but it may be 
difficult for these fractures to travel all the way through. Enceladus' 
tiger stripes are unusual because they extend down to the ocean - and they 
present an enticing opportunity to search for evidence of life outside Earth.

The tiger stripes
=================
These famous features are surrounded by 300-meter-high margins that form 
a valley-like trough up to several kilometers wide at the moon's surface.

To understand exactly how the tiger stripes formed, researchers model 
ice shell fractures based on various thicknesses. 
"Our models show that tidal stresses can fracture the ice shell all 
the way through, but indirectly limit how thick the ice can be," says
 Catherine Walker, a glaciologist from the Woods Hole Oceanographic 
Institution and lead author of a recent study published in The Planetary 
Science Journal.

This new research shows that fractures originating at the surface are 
unlikely to reach the subsurface ocean, even for thinner ice depths. 
But fractures that begin at the base of the ice shell have a better 
chance of piercing the surface, especially if they connect with cracks 
that originate from the top of the ice shell.

"The ocean is under pressure, so water is forced into tiny cracks at 
the base of the ice shell, which widens and propagates the cracks 
all the way up to the surface," says Carolyn Porco, a planetary
scientist and visiting scholar at the University of California, Berkeley, 
and former leader of the Cassini Imaging Team, who suggested this
 possibility with colleagues in 2014.

The recent study also found that it's more difficult to form fractures 
through the entire ice shell than previously thought. 
Existing fractures reduce the overall amount of stress, and when this 
is accounted for, new ones don't propagate as deep or as high, says Walker. 
"The exact ice shell thicknesses are not known - but it could just be 
that Enceladus' ice shell is thinner than we think at the south pole."

A habitable ocean
=================
Over a decade ago, the Cassini spacecraft flew through the plume and 
detected a composition of mostly water, but also salts and organic 
molecules that hinted at the subsurface ocean.

The spacecraft detected tiny grains of silica, too, which suggests the 
presence of hydrothermal vents. 
Temperatures may reach close to 212 degrees Fahrenheit within these 
vents, which would allow organisms to survive without sunlight, says 
Morgan Cable, a chemist who heads NASA's Astrobiology and Oceans Worlds Group.

Like hydrothermal vents on Earth, those on Enceladus sit on the seafloor. 
There, heat from the moon's rocky interior may erupt hot mineral-rich 
water in chimney-like ocean currents - and organisms could take 
advantage of the different concentrations of dissolved minerals 
in these streams. 
"We are conservative in our estimate of life due to the limited energy 
budget, but you could certainly have multicellular organisms such as 

crabs," Cable says.

A future mission
================
All in all, Enceladus' tiger stripes offer a unique opportunity to 
collect and analyze fresh material from a subsurface ocean without 
the need to dig or drill. A future mission would include repeat 
fly-throughs of the plume, and a possible landing on the south 
polar terrain to sample freshly falling material that erupts from the geysers.

Touching down on Enceladus would enable the most comprehensive search 
for evidence of life and allow for easier collection of materials, 
including repeat and varied measurements to increase scientists' 
confidence levels in any discoveries, Porco explains.

A landing could also offer detailed insights into Enceladus' 
geophysical workings and help resolve open questions; for example, 
the ice shell thickness and the width of the fractures.

But of all the burning questions, discovering whether life exists 
outside of Earth is the most alluring.

"It's only in the outer reaches of our solar system that we could be 
assured any life found there would represent a genesis of life that 
is independent of life on Earth," Porco says.ÿ"And whether or not 
life has arisen independently elsewhere is the most beguiling question 
that we could hope to answer in exploring the solar system."


             ____  __  ____   ___  _  _  ____    ____  ____  ____ 
            (  __)(  )(___ \ / __)( \/ )(  _ \  (  _ \(  _ \/ ___)
             ) _)  )(  / __/( (_ \ )  /  ) _ (   ) _ ( ) _ (\___ \
            (____)(__)(____) \___/(__/  (____/  (____/(____/(____/
                   PART OF THE DONEGAL PACKET RADIO NETWORK 
                     Packet: EI2GYB@EI2GYB.DGL.IRL.EURO
                           Email: EI2GYB@GMAIL.COM
+------------------------------------------------------------------------------+




Read previous mail | Read next mail


 22.12.2024 14:56:48lGo back Go up