Episode 483 - Constantly changing moons of Jupiter episode artwork

EPISODE · May 16, 2022 · 15 MIN

Episode 483 - Constantly changing moons of Jupiter

from Lagrange Point · host Lagrange Point

Jupiter's moons may be way more dynamic than we previously thought. Europa has the most potential to harbor life outside of Earth, but it's ice sheets may be more Earth like than we imagined. Europa's spectacular double ridges are similar to those found in Greenland. The ice sheets on Europa may not be static and still, but churning. Melting and refreezing could drive exchange between the surface of Europa and it's icey depths. How do you form sand dunes without any wind? Is it possible to form a Dune on Io using just volcanic flows and sulfur snows? Culberg, R., Schroeder, D.M. & Steinbrügge, G. Double ridge formation over shallow water sills on Jupiter’s moon Europa. Nat Commun, 2022 DOI: 10.1038/s41467-022-29458-3 George D. McDonald, Joshua Méndez Harper, Lujendra Ojha, Paul Corlies, Josef Dufek, Ryan C. Ewing, Laura Kerber. Aeolian sediment transport on Io from lava–frost interactions. Nature Communications, 2022; 13 (1) DOI: 10.1038/s41467-022-29682-x

Episode metadata supplied by the publisher feed · Published May 16, 2022

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Episode 483 - Constantly changing moons of Jupiter

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