Wow, it was feast or famine, and now's the feast - I'll try to reply briefly (and shall of course fail, being a professor), in order. First to Doug: Thank you. I love devil's advocates - a favorite teaching role. That spherule size would vary with position in the section, and that many beds would be free of spherules, strikes me as just as consistent with the impact/vapor condensation hypothesis as with the concretion hypothesis. That deep spherules would be dug up and homogeneously redistributed around a small impact crater (Victoria) speaks for itself regarding the importance of impacts.
What we want is observations and predictions that might help differentiate one hypothesis from the other. What the impact hypothesis predicts is that impact spherules of various types (e.g., glassy, possibly metallic if from a metallic impactor, possibly sulfidic if the target was sulfidic, various accretionary lapilli) should be extremely widespread on Mars (given how heavily cratered it is), and that their specific composition and size might depend on the composition and energetics (size, velocity) of the impactor, and, more importantly, on the composition (including ice or brine content) and mechanical nature (e.g., hard rock, very soft rock) of the target area. (The surge cloud can also pick up dust and sand and possibly larger rock fragments - ordinary lapilli - by scouring along its path; scouring forms cross-bedding.) So far only two landers with microscopic imagers have landed on Mars - and both have found tiny, nearly perfect spherules in cross-bedded, salty, sandy rock (more homogeneously distributed at Meridiani than at Gusev's Home Plate). The impact hypothesis would predict that any future rovers with MI's landing in similar layered terrains should be able to find similar spherules, and perhaps that spherules should litter the surface everywhere. Most spherules would be at least as small as ordinary sand grains, in which case they could be mixed (diluted) with normal basaltic sand and moved along by the wind. Comparatively large, dense (hematitic) spherules, like those at Meridiani and probably other areas, would be left behind as a wind-resistant lag (spherule pavement or armor) after wind removal of fines. So far predictions of the impact hypothesis seem okay - tiny spherules at both Gusev and Meridiani, and probably all over the place. Current instrumentation is not able to detect the impact-formed high pressure minerals, melts, and microtextures that should likewise be widespread. Craters, the best evidence of impacts, are everywhere of course.
That brings us to predictions concerning spherule size, shape, clumping, and distribution in the rock. I note that I am partly rehashing my 2007 LPSC abstract so far, so I'll just refer you to that for the detailed arguments:
http://www.lpi.usra.edu/meetings/lpsc2007/pdf/1922.pdfThe impact hypothesis passes with an "A" and the concretion hypothesis fails, as far as I can tell, even considering the Navajo Sandstone and similar rocks of uniform porosity and permeability. Ditto regarding the distinctive Ni enrichment detected in spherules at the "berry bowl" and elsewhere (nickel enrichment, along with enrichment in iridium and other platinum group elements, characterizes fully oxidized impact spherules related to the impact assumed to have killed the dinosaurs 65 million years ago). How alleged sedimentary concretions got to contain relatively coarse, shiny "gray hematite" (so-called specular hematite, the high temperature hydrothermal kind) has never been properly addressed by the concretion crowd, as far as I know. High temperature formation of specular hematite is obviously no problem during a steamy impact. And so on. If the MER team wants to convince me that Oppy has found concretions, in terms of size they'd have to show me some that are far too big or too massively clumped together for a turbulent cloud to support (not simple doublets and triplets, which are easily explained by surface stickiness). In terms of shape, they'd have to show me some that are irregular shapes, flattened by vertical permeability variations in the rock, or elongated by fluid flow (look in any freshman textbook for typical concretion shapes and sizes). In terms of distribution, they'd have to show me variations that obviously depend on fluid flow, and on mixing of different brines that were oxidized and reduced, or concentrated and dilute (e.g., spherules should concentrate just below the paleo water table, or along fractures or veins, or beside brine mixing surfaces that cut bedding). So far, nothing like that has been imaged, whereas you see such features everywhere in the Navajo Sandstone (an alleged analog).
With regard to your comment on possibly biased interpretations, I'll let "follow the water" speak for itself. Recall that prior to the rover landing Meridiani was first supposed to be the largest hot spring in the solar system, and then the largest lake-deposited metamorphosed sedimentary iron formation. Expectations of finding evidence for a lake was why they landed there (and at Gusev). Subconsciously, they weren't going to give up that lake idea too easily, I would guess (just dry it up, blow it around, soak it, erode it down to the water table, blow it around some more, uniformly mix different-density brines in it without dissolving or recrystallizing soluble salts, erode it down to the water table again, and make fairly deep water flow across it locally without carving channels, although I admit I do get confused over the exact order of events, and I may have left something out). We started out with no prior expectations, but to us the images as they came down each day simply did not show what was claimed at the initial news conference and afterwards in meeting presentations and refereed publications. Examples: Why were the alleged concretions all so perfectly spherical, and all so uniformly tiny? Why were the alleged water-soaked evaporites a uniform mixture of highly soluble and nearly insoluble sulfate salts? Where were the large salt crystals and bulk impermeability that one would expect from water soaking? Where were the shales that could indentify a playa lake or smaller interdune puddle? Where did most of the chlorides go? Do hematitic concretions even occur in evaporites? Why do almost all terrestrial analogs for alleged atmospheric acids ultimately depend on weathering of pyrite - fool's gold - or other sulfides in mineral deposits or districts like Rio Tinto, Spain? If there was flowing surficial water, why weren't there also visible channels or braided stream patterns or mud cracks? And similar questions by the hundreds, only some of which were answered by the elegant and highly complex genetic models that the MER team evolved (these interpretational models and hypotheses were erroneously referred to as "discoveries"). These interpretations, BTW, seem only to apply to a rare set of circumstances that occurred only at Meridiani, and so their predictive power is limited. The team chose to apply a completely different interpretation to almost identical-appearing rocks at Home Plate and vicinity, despite the cross-bedded sands, acid salts, and spherules. In place of the hypothetical enormous "vanished playa" of Meridiani, they hypothesized a little "vanished volcano". Why not notice the impact craters that are so highly visible all over the place, and that all the rocks are fragmental (bashed near to death)? Why not notice that MOC and then HiRise imaging make it appear that similar-looking cross-bedded, salty rocks occur all over the place, not just at the two landing sites? (Pardon my little rant.)
With regard to impacts, please don't confuse our impact hypothesis with the "white Mars" hypothesis of Nick Hoffman. They're not the same. That said, Nick's a very intelligent, well-read guy, and I'd hate to take him on in a technical discussion of outflow channels. A lot of what he thinks about Mars in general I now agree with, and he said it first. Unlike him, however, my co-authors and I see no reason to exclude geologically fleeting occurrences of liquid water (brine) in ancient outflow channels and seas at lower elevations, or in temporary streams and crater lakes (like Gusev) at higher elevations, or in young gullies. Such waters, unless they were a concentrated Ca-enriched chloride brine (or concentrated sulfuric acid, unlikely for other reasons), were probably freezing over and then sublimating furiously (as so beautifully described in the original "Red Mars" novel by Kim Stanley Robinson). Our own "white Mars" model (with apologies to both Hoffman and Robinson), might then consist of lots of buried water ice above chloride-enriched brines and/or white crystalline salts, and Knauth and I published a couple of papers to that effect in 2002 and 2003 (inspired by the young gully phenomenon). You didn't specifically ask about salts I realize, although you did mention hydrous sulfates and empty crystal cavities. We covered those in our original Nature paper in 2005. No more moisture is required than would be present in the original surge cloud (mainly condensing steam) or could later be removed from the atmosphere by water-attracting (hygroscopic or deliquescent) salts. For us the rovers have imaged absolutely no unambiguous surface evidence for large quantities of standing or flowing liquid water (brine) at either landing site (including ground water or spring water). We don't a priori exclude evidence for liquids anywhere else, especially in rocks older than those now exposed at the surface of the two landing sites (i.e., you could drill a deep hole at either landing site and possibly find the desired evidence beneath the impact beds, if that's what they are).
Well, that's way too long, as predicted, but then Doug is the boss here and presumably merits a detailed discourse. I'll have to address other people's questions and concerns later (sorry). Let me close with a naive question: A week ago, in this forum's probably greatest triumph to date, many of you questioned the ability of liquid water in the form of a puddle to exist on the 20 degree slope of Burns Cliff. What do you think about the ability of bottom-fed surficial water to flow vigorously across a perfectly horizontal surface (allegedly made horizontal by wind erosion of sand down to the water table) while trapped in localized interdune depressions not connected to each other by any visible flow channels? That's what seems to be required by the highly localized "festoon" hypothesis of one member of the MER team, unless I have his argument for the rarity of "festoons" completely wrong (which is certainly possible - he loves to cloak what he is saying in obscure geojargon like "festoon"). Is flowing water any more likely in an isolated horizontal basin (where I'd expect a puddle) than puddles are on a slope? Or am I overlooking something important that's obvious to everyone else? Note that I didn't say such flow was flat-out impossible - there could be a slight slope and the sands could be extraordinarily permeable - it just seems unlikely and unsatisfying (like so much of the rest of the complex Meridiani scenario).
Finally, I am writing this rant at home on Father's Day, and am certainly not speaking for my employer, my co-authors (who have not seen this), or my more plantetological colleagues. And I'm not a lawyer, so please forgive me if I have unintentionally offended anyone. And evolution, plate tectonics, and gravity are all still "theories" (in science, that's as good as it gets - there is no infallible source of wisdom, we all make mistakes, and any theory is always subject to modification by new observations. For example, I wish we understood gravity better, so I could go study Mars instead of just Antarctica and the Peruvian/Bolivian altiplano.)
--Don