[HN Gopher] Uranus' moon Miranda may have an ocean beneath its s...
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       Uranus' moon Miranda may have an ocean beneath its surface
        
       Author : geox
       Score  : 21 points
       Date   : 2024-11-03 19:17 UTC (3 hours ago)
        
 (HTM) web link (phys.org)
 (TXT) w3m dump (phys.org)
        
       | munchler wrote:
       | > The team set out to explain Miranda's enigmatic geology by
       | reverse engineering the surface features, working backward to
       | uncover what the moon's interior structure must have been to
       | shape the moon's geology in response to tidal forcing.
       | 
       | "Must have been" is doing a bit too much work in that sentence.
       | This project is a cool idea and it would certainly be huge news
       | if there is liquid water inside Miranda, but this is a long way
       | from actual evidence.
        
       | echelon wrote:
       | Is there a comprehensive list of all the planets, dwarf planets,
       | moons, etc. that we suspect may have liquid water?
       | 
       | How many of them have liquid water without being super saturated
       | with salts? What is the level of confidence we have?
       | 
       | Which are most likely to bear life given our current hypotheses
       | around the origins of life?
        
         | kevinkeller wrote:
         | I have been doing some late-night wikipedia binges on this
         | matter, so I consider myself qualified to answer.
         | 
         | > Is there a comprehensive list of all the planets, dwarf
         | planets, moons, etc. that we suspect may have liquid water?
         | 
         | Most large moons orbiting the gas giants are suspected to have
         | subsurface water oceans, most prominent among them Europa.
         | Ganymede, Enceladus, and Triton are other honorable mentions:
         | https://en.wikipedia.org/wiki/Planetary_oceanography#Natural...
         | 
         | > How many of them have liquid water without being super
         | saturated with salts? What is the level of confidence we have?
         | 
         | We don't know the composition yet, just that a salty ocean
         | supports the evidence we've seen. For example, Europa interacts
         | with Jupiter's magnetic field in such a way that makes sense
         | only if there is a large amount of electrically conducive
         | material inside Europa. Given what we know about its formation,
         | metallic stuff is unlikely. A salty subsurface ocean is a more
         | suitable explanation. We'll know once Europa Clipper gets there
         | (one of its missions is to 'taste' the ocean by flying past
         | really close).
         | 
         | There are other reasons to suspect a subsurface ocean, such as
         | signs of a geologically active body (like Enceladus), which in
         | turn implies there is enough heat inside to have an ocean.
         | 
         | > Which are most likely to bear life given our current
         | hypotheses around the origins of life?
         | 
         | Europa, maybe Enceladus. Note that our search for life is
         | heavily guided (biased?) by our understanding of how we think
         | life started here on Earth.
         | 
         | Specifically, we needed these ingredients (non-exhaustive):
         | 
         | * a liquid medium to act as shelter and transport medium
         | (liquid water ocean) * a source of energy, something that life
         | can 'eat' (hydrothermal vents in the beginning, sunlight later)
         | * protection from space-borne threats (atmosphere, magnetic
         | field) * a home that isn't geologically dead (like the Moon, or
         | Mercury), but also isn't _too_ active (like Io)
         | 
         | Europa checks most of the requirements:
         | 
         | * suspected subsurface ocean * geologically active. This is
         | important because Europa and other moons are too far away for
         | sunlight to be a big source of energy. There has to be another
         | source. Radiogenic heating (released by radioactive isotopes)
         | and primordial heating (left over from its formation) aren't
         | enough for moons to sustain liquid water (especially 4.5 B
         | years after formation). This means tidal flexing is what we
         | should be looking for -- something we know Europa has. *
         | Europa's thick icy crust blocks pretty much all radiation.
         | Barring a thick atmosphere (which only Titan has), a subsurface
         | ocean underneath an icy crust is the best life can hope for out
         | there, for protection against radiation. * We don't know much
         | about what goes on underneath the surface. If the bottom of the
         | ocean contains geothermal vents, then that could harbor earth-
         | like life.
         | 
         | Saturn's moon Enceladus checks many of these same boxes (tidal
         | heating, abundant water, signs of a young surface indicative of
         | geological activity).
         | 
         | JUICE and Europa Clipper missions should fill in many of these
         | gaps, and help confirm our understanding.
        
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       (page generated 2024-11-03 23:01 UTC)