The First Europa Lander, What can be done first, cheapest & best? |
The First Europa Lander, What can be done first, cheapest & best? |
Dec 31 2005, 12:08 AM
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Merciless Robot Group: Admin Posts: 8790 Joined: 8-December 05 From: Los Angeles Member No.: 602 |
I think that many people in this forum would agree that somebody's going to have to land on Europa someday before the rather elaborate schemes to penetrate the outer ice layer will ever fly, if for no other reason than to get some relevant ground truth before committing to such an elaborate, expensive, and risky mission.
EO seems to have ruled out any surface science package for that mission (though it would be nice to change their minds! ), but I think that there is a valid requirement at some point to directly assess the surface properties of Europa in an inexpensive yet creative way. Some candidate instrument payloads might be: 1. A sonar transducer/receiver set embedded within a penetrometer to determine crust density and examine the uniformity of the ice layer within the operational radius of the instrument (looking for cracks and holes, in other words). 2. A conductivity sensor again embedded inside a penetrometer to measure the native salinity of the surrounding material and possibly derive some constraints on the composition of metallic salts in the European crust (saltiness has a major effect on ice properties, in addition to the obvious need to derive the salt content of any underlying ocean). 3. A seismometer for all sorts of reasons. How does this sound? Any critiques, additions, or subtractions? I omitted a surface imager not only because of bandwidth/extra complexity considerations but also because it seems desirable to penetrate the crust in order to minimize as much as possible reading any contaminants from Io during surface measurements. The orbiter data could be used to sense and subtract this from the penetrometer readings. -------------------- A few will take this knowledge and use this power of a dream realized as a force for change, an impetus for further discovery to make less ancient dreams real.
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Jul 1 2006, 08:50 AM
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Senior Member Group: Members Posts: 1870 Joined: 20-February 05 Member No.: 174 |
In the outer solar system, we have tended to find that higher albedo objects have more active, self-cleaning (due to activity) surfaces. These surfaces tend to be the roughest on a meter scale, while the cratered-to-hell-and-gone iceballs like Rhea or Callisto have relatively block and rubble free undulating but smooth meter-scale surfaces. They've been hit so much you just make the rubble bounce and pound it finer.
I'm overstating this, but it's a clear trend. |
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