Evidence for Water on Europa

europaraft2_gal.jpg (67214 bytes)

A small region of Europa's Conamara region. The white and blue colors highlight regions covered by ice dust from the collision that created the Pwyll Crater. Disconnected islands of ice are visible that have apparently rafted to new positions.

(Source:  http://antwrp.gsfc.nasa.gov/apod/ap980102.html}


europaplains.jpg (44117 bytes)

The picture above is a mosaic of images from Europa's southern hemisphere. The brown, linear ridges extending across the scene are thought to be frozen remnants of cryo-volcanic activity.  "Cryo-volcanoes" (cold volcanoes) occur when liquid or partially frozen water erupts onto the Europan surface, freezing instantly in the extremely low temperatures so far from our sun.   The ridges are similar in appearance to those involved in seafloor spreading on Earth.

seafloor.gif (15567 bytes)

 

europazoom.jpg (20830 bytes)

A geologically older, smoother surface, bluish in tone, underlies the ridge system. The blue surface is composed of almost pure water ice, whereas the composition of the dark, brownish spots and ridges is not certain. One possibility is that they contain mineral salts in a matrix of
high water content.

bonneville.jpg (19543 bytes)

(Sources:  http://www.science.nasa.gov/newhome/headlines/ast03dec98_1.htm and
                http://pubs.usgs.gov/publications/text/developing.html)


therathrace.jpg (35078 bytes)

Thera (left) and Thrace (right) are two dark, reddish regions of enigmatic terrain that disrupt
the older icy ridged plains on Jupiter's moon Europa. One model for the formation of these and other chaos regions on Europa is a complete melt-through of Europa's icy shell from an ocean below.  

The surface may be salty in places. The best spectral match is to magnesium sulfate, better known as Epsom salts. When warm convecting ice rises up and hits a salty area it melts at a lower temperature than the surrounding plains. This sort of process might explain regions like Thrace where we see what appears to be melting and liquid-like flows across the surface.   The best candidates for the brown material are iron compounds or some sort of sulfur compound.

(Source:  http://www.science.nasa.gov/newhome/headlines/ast09sep99_1.htm)


hex.jpg (7968 bytes)

At temperatures above 170K, ice formed from liquid water or from 'warm' water vapor has a hexagonal crystal, just like ice on Earth.  If we could find evidence for hexagonal ice crystals on Europa, it would mean that the ice formed fairly recently from liquid water or warm vapor.

If hexagonal ice crystals are present on Europa, their signature may be seen using Galileo's Near Infrared Mapping Spectrometer.  When sunlight hits the surface of Europa at near grazing incidence it penetrates the surface and refracts through the ice crystals.   Hexagonal crystals will produce a ring-like glow in the infrared much like the familiar "ring around the Moon."

moonbow.jpg (3326 bytes)

(Source:  http://www.its.caltech.edu/~atomic/snowcrystals/gallery99/snow99.htm
               http://www.science.nasa.gov/newhome/headlines/ast09sep99_1.htm
               http://www.dxd.com/gallery.htm )

back | next