New computer model may explain moon Europa's chaotic terrain

Dec 02, 2013 by Bob Yirka report
This rendering shows the temperature field in a simulation of Europa’s global ocean dynamics, where hot plumes (red) rise from the seafloor and cool fluid (blue) sinks downward from the ice-ocean interface. More heat is delivered to the ice shell near the equator where convection is more vigorous. Credit: K. M. Soderlund

(Phys.org) —A team of researchers at the University of Texas with assistance from a computer modeler at the Max Planck Institute in Germany has put together a computer model that might just explain the peculiar surface of Jupiter's moon Europa. In their paper published in the journal Nature Geoscience, the team suggests the odd surface terrain patterns likely come about due to convection. Jason Goodman of Wheaton College offers a perspective on the researchers' findings in a News & Views piece printed in the same journal.

The NASA space probe Voyager flew past Jupiter and its moons in 1979, and in so doing, set off a debate about the nature of the surface of one such moon, Europa, that has continued to this day—why is the surface so smooth, and why are there odd rough patches covering nearly 40 percent of its surface? Scientists agree that the general smoothness is likely due to the existence of water beneath the icy surface—the lack of craters indicates a surface that is able to heal itself after impacts. Less of a consensus has been found regarding the rough patches, however, which scientists call "chaotic terrain." In this new study, the researchers used data from hydro-systems here on Earth as well as data from both Voyager and the Galileo spacecraft (which detected a magnetic field) to create what they believe is a reasonable model of a process working beneath the icy shell of Europa's surface.

Some have suggested Europa's surface gets its unique features due to the pull of gravity from Jupiter—others have suggested the sun plays a role. Such theories have not held much weight however, as there is little evidence to suggest that either could account for the chaotic terrain. Instead, the modelers suggest, it's due to convection driven by heat from the interior of the moon itself. Their model shows, they write that currents beneath the ice tend to deliver heat primarily to the equatorial regions of the surface which in turn causes constant heating, melting and refreezing—resulting they say, in the chaotic terrain that we are able to observe.

This rendering shows the temperature field in a simulation of Europa’s global ocean dynamics, where hot plumes (red) rise from the seafloor and cool fluid (blue) sinks downward from the ice-ocean interface. More heat is delivered to the ice shell near the equator where convection is more vigorous, consistent with the distribution of chaos terrains on Europa. Credit: Model image created by K. M. Soderlund with the image of Europa taken from NASA/JPL/University of Arizona

Of course, the model is based on theory, which suggests, Goodman notes, that it could be either right or wrong, and we aren't likely to know which it is until we send a probe to Europa to study its first-hand.

This rendering shows isosurfaces of warmer (red) and cooler (blue) temperatures in a simulation of Europa’s global ocean dynamics. More heat is delivered to the ice shell near the equator where convection is more vigorous, consistent with the distribution of chaos terrains on Europa. Credit: Model image created by J. Wicht with the image of Europa taken from NASA/JPL/University of Arizona

Figure shows simulated zonal flows and temperature fields in planetary convection models in a Jovian (Jupiter-like) system (above) and a Europa-like setting (below). The Jovian simulation shows latitudinal bands of convection, visible as distinct stripes, reflecting the controlling influence of the planet's rotation. The Europa-like simulation shows a more three-dimensional convection pattern associated with dynamic ocean heat circulation, with greater activity near the equator and less circulation near the poles. Credit: University of Texas Institute for Geophysics.


Explore further: Image: A cosmic hurricane

More information: Ocean-driven heating of Europa's icy shell at low latitudes, Nature Geoscience (2013) DOI: 10.1038/ngeo2021

Abstract
The ice shell of Jupiter's moon Europa is marked by regions of disrupted ice known as chaos terrains that cover up to 40% of the satellite's surface, most commonly occurring within 40° of the equator1. Concurrence with salt deposits2 implies a coupling between the geologically active ice shell and the underlying liquid water ocean at lower latitudes. Europa's ocean dynamics have been assumed to adopt a two-dimensional pattern3, 4, 5, 6, 7, 8, which channels the moon's internal heat to higher latitudes. Here we present a numerical model of thermal convection in a thin, rotating spherical shell where small-scale convection instead adopts a three-dimensional structure and is more vigorous at lower latitudes. Global-scale currents are organized into three zonal jets and two equatorial Hadley-like circulation cells. We find that these convective motions transmit Europa's internal heat towards the surface most effectively in equatorial regions, where they can directly influence the thermo-compositional state and structure of the ice shell. We suggest that such heterogeneous heating promotes the formation of chaos features through increased melting of the ice shell and subsequent deposition of marine ice at low latitudes. We conclude that Europa's ocean dynamics can modulate the exchange of heat and materials between the surface and interior and explain the observed distribution of chaos terrains.

Press release

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Osiris1
1 / 5 (4) Dec 02, 2013
Nice technical subjects of a niche variety tend to scare away foolish self centered dilettantes. We might want to know more of this unique moon type which may be fairly common residents of gas giant moon systems.
Jonseer
1 / 5 (3) Dec 03, 2013
What I'd like to know is whether or not there has ever been an effort made to distinguish the age of various parts of the Moon's surface beyond the visual queues always used, by that I mean some sort of data that can detect extremely fresh ice only a few years old.

All I've ever read is gross measurements like relatively young, or only a million years old Etc.

Surely there must be some way to detect new ice formed on the surface from say the Europan equivalent of a mud volcano or spring on Earth.

Also has anyone ever heard of any effort by NASA to find cryovolcanic features on Europa?

I never read a word mentioning any such effort, and I've read volumes a lot of it several times LOL

No doubt the reason is due to the desire to NOT encourage any exploration of the surface of Europa in order to protect it from Earthly contamination just like Mars.

I just googled it again. I found a single mention of cryovolcano or volcano + Europa. Considering Io, that's suspicious