Even Uranus Might Be Hiding An Ocean World
Dr. Alfredo Carpineti
Senior Staff Writer & Space Correspondent
Edited
by
Laura Simmons
Uranus’ icy moon Miranda, as seen by NASA’s Voyager 2 spacecraft on January 24, 1986.
Image credit: NASA/Jet Propulsion Laboratory-Caltech
Ocean worlds, such as Europa around Jupiter and Enceladus around Saturn, are recent and fascinating discoveries. These moons hide, far beneath their icy crusts, a deep liquid ocean. Other moons and dwarf planets also hide liquid oceans underneath, and the latest candidate is Miranda – the smallest of Uranus's five round moons.
Miranda might be the smallest round object in the Solar System. It has a diameter of just 470 kilometers (290 miles). Its surface area is just about the area of Texas. Still, it is a complex world. Its surface is among the most extreme we have observed anywhere and features the tallest cliff in the Solar System: Verona Rupes, which has a drop of about 20 kilometers (12 miles). An equivalent cliff on Earth would have to be over 270 kilometers tall.
It was these and many other interesting features that suggested the presence of an ocean. Once the surface structures are plugged into computer models, the enigmatic geology is best matched by the presence of a vast ocean that formed between 100 and 500 million years ago.
"To find evidence of an ocean inside a small object like Miranda is incredibly surprising," co-author Tom Nordheim, from Johns Hopkins Applied Physics Laboratory (APL), said in a statement. "It helps build on the story that some of these moons at Uranus may be really interesting – that there may be several ocean worlds around one of the most distant planets in our Solar System, which is both exciting and bizarre."
More:
https://www.iflscience.com/even-uranus-might-be-hiding-an-ocean-world-76607
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