Europa's Chaos Terrains
Hard layers of ice make up the surface of Jupiter's frozen moon Europa. Glacial cracks and ridges scar its frigid white plains, carving paths across an icy shell that conceals a deep ocean of liquid water. Closer inspection of the moon's fractured topography reveals highly disrupted areas, called chaos terrains, where blocks of ice appear to have broken off, drifted and refrozen to the surface. Searching for an explanation of how these features formed, researchers studying images of Europa taken by NASA's Galileo spacecraft have come up with an answer. As plumes of warm ocean water rise to the subsurface, massive lakes develop inside the moon's crust—some larger than North America's Great Lakes combined. Over time, the ice directly above these lakes collapses, splintering into floating geometric fragments that rotate, raft and resettle into all kinds of chaotic configurations. Watch the video to learn more about Europa's chaos terrains.
Giant lakes trapped in Europa's crust bust up this distant moon's icy surface.
Find out what Europa's chaos terrains could mean for the possibility of finding life deep within its chilly ocean.
An artist's interpretation of a subsurface lake formed inside Europa's crust due to a rising plume of warm ocean water.
The Conamara Chaos, indicated with an arrow, is a well-known chaotic region on Europa.
A close-up view of the Conamara Chaos reveals jumbled blocks of ice that have refrozen to the surface.
For More Information
See Science@NASA
Credits
Please give credit for this item to:
Science@NASA and NASA's Goddard Space Flight Center
Cover image courtesy of NASA/JPL/Ted Stryk
Video courtesy of Science@NASA
Illustration courtesy of Britney Schmidt/Dead Pixel VFX/Univ. of Texas at Austin
Conamara Chaos image courtesy of NASA/JPL/University of Arizona and NASA/ NSSDC Photo Gallery
Conamara Chaos close-up courtesy of NASA/JPL/University of Arizona
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Producer
- Tony Phillips (Wyle Information Systems)
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Writer
- Alex Kasprak (USRA)
Release date
This page was originally published on Thursday, January 31, 2013.
This page was last updated on Tuesday, October 10, 2023 at 11:53 PM EDT.