← if you were there

BENEATH EUROPA'S ICE

Through a shell of ice, toward water we have never seen.

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stage 01

THE SURFACE

You arrive above water ice cut by fractures, ridges and disrupted terrain. Radiation from Jupiter alters materials at the surface; this is not an untouched window into the ocean below.

stage 02

THROUGH THE ICE

The shell is not known to have one uniform thickness. Earlier estimates commonly span about 15 to 25 kilometres, while Juno measured an average near 29 kilometres only across the region it observed.

stage 03

DARK WATER

Multiple lines of evidence point to a salty ocean beneath the shell. NASA commonly estimates it may be 60 to 150 kilometres deep and hold about twice the water in Earth's global ocean, but no probe has entered it.

stage 04

THE UNSEEN BOUNDARY

Whether ocean water interacts directly with a rocky seafloor, and what chemistry occurs there, remain uncertain. Europa Clipper will constrain the moon's structure and habitability; it is not designed to find life directly.

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