Network for Ocean Worlds (NOW)

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Network for Ocean Worlds (NOW)

Network for Ocean Worlds (NOW)

@Ocean_Worlds

NOW is a @NASAAstrobio-funded RCN investigating science and tech of #OceanWorlds exploration in our solar system and beyond. Not an official NASA account.

Beneath the Ice Katılım Ekim 2020
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Network for Ocean Worlds (NOW)
Network for Ocean Worlds (NOW)@Ocean_Worlds·
NOW’s Future Leaders of Ocean Worlds #FLOW have created their own Twitter account! Follow @NowFlow for exciting updates from our amazing early career researchers.
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Network for Ocean Worlds (NOW)
Network for Ocean Worlds (NOW)@Ocean_Worlds·
The newly-formed Ocean Worlds Working Group (OWWG) is pleased to announce its inaugural virtual town hall meeting, on June 29th from 9 – 10:30 AM PT. You can also find out more about the OWWG and join the mailing list at: lpi.usra.edu/owwg/
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ARCHIVED – NASA Astrobiology
ARCHIVED – NASA Astrobiology@NASAAstrobio·
The volcanic vent system at Gakkel ridge – the newly identified analog – appears similar in many ways to those predicted for Enceladus, and could be spontaneously synthesizing materials important for the origin of life on this and other ice-covered ocean worlds.
ARCHIVED – NASA Astrobiology tweet media
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OriginsHabitabilityLab
OriginsHabitabilityLab@OHLlab·
If you are interested in hydrothermal vent systems and their role in habitability & CO2 sequestration through lab simulated chimneys! Then, my friends you're in luck! You can make your way to Julia Chavez's poster (Board 029)!!! #AbSciCon22 #astrobiology #hydrothermalsystems
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Sanjoy Som
Sanjoy Som@sanjoymarcel·
Hey #AbSciCon22, you want to hear about how I quantify habitability? Stop by poster 19! @Ocean_Worlds
Sanjoy Som tweet media
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Michael Wong
Michael Wong@miquai·
Tori Hoehler: The residual CO2–H2 disequilibrium on Enceladus cannot be used to say that life isn’t present, because unused free energy occurs in Earthly methanogenic ecosystems too. #AbSciCon22
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Michael Wong
Michael Wong@miquai·
.@PlanetarySpiers: Europa’s thermal history, driven by changes in its orbit, affects the H2 flux from serpentinization and the oxidant flux from its ice shell into its subsurface ocean, changing the satellite’s geochemistry over deep time. #AbSciCon22
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