QUOTE (climber @ Aug 2 2006, 02:37 PM)
May be you've noticed that my first reaction seeing Beagle interior was : it looks hand made! That's consistant to what You and Castor are saying.
Yeah -- my first reaction was "It's a masonry crater." It looks, for all the world, like a laid fieldstone structure, made in the shape of a crater, with the interior polished into a smooth bowl.
It may well be that the action of Martian winds as they swirl around the crater's interior is enough, all by itself, to have smoothed the interior to the degree we see. It's also evident that a portion of the interior rim has *not* been smoothed, or has been roughened since the crater interior was "polished." That portion lies to the right of center in our current view.
Another indication of varying rates of erosion is the "ray" that extends from between the one and two o'clock positions in our current view (with the nearest point of the near rim being the six o'clock position). This appears to be a classic impact ray from above (in the MOC image), but from this angle, it looks significantly *less* blocky than the surface we're on. What it *does* look like is a small ridge of evaporite, with its once-exposed evaporite blocks having been worn down smooth. The ridge is not really populated by the blocky evaporite (and other rock type) debris we see around the rest of the crater. I'd guess the ridge is a deformation of the shocked Victoria debris apron that the Beagle impactor struck -- perhaps a seismic reflection from a somewhat deeper structure created when Victoria's ejecta blanket was emplaced. Or maybe it was already there, a ridge of Victoria debris, and Beagle just happen to smack right down onto it...
So -- the "ray" looks more like a deformation feature than an ejecta feature, that has been preferentially eroded down flat, as has much (but not all) of Beagle's inner rim. I'd bet the less-eroded, blockier portions of Beagle and its ejecta blanket are more wind-shadowed than the polished portions.
-the other Doug