QUOTE (ngunn @ Jul 13 2007, 03:09 PM)
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Centsworth - since nobody else has come back on that point, yes, the relative timescales of the various processes that have to happen to emplace the berries in the Burt scenario is one aspect that is giving me problems when I try to 'run the simulation' in my head. Emotionally I like his ideas. .... As a physicist I'm happier with bangs and things flying through the air than I am with subterranean chemical wizardry. Nevertheless this one is getting harder to believe the more I think about the details - and that's not good for any hypothesis.
ngunn and centsworth - Thanks for your comments. Unfortunately, I am not a physicist, nor an aerodynamic modeler, so if you find problems in the details of my made-up explanation, improve on them please. My starting point all along has been two facts:
1) Those berries, other than being round, just don't look like any actual concretions I've ever seen, not even the Utah-Arizona "Moqui marbles" that so much as been made of. Their near-perfect sphericity and size limitation makes them look much more like, say, hailstones.
2) My co-author Paul Knauth, when I was studying volcanic surge deposits in the 1970s, was himself studying some of the oldest rocks preserved on Earth (Archean Era), in South Africa. A puzzling feature of these rocks, in some sections, is 100's of square km of several-meters-thick spherule beds, preserved in marine sediments (meaning they have been water reworked, chemically altered, and flattened somewhat by the weight of overlying rock). These were initially thought to be volcanic accretionary lapilli, but their huge aerial extent and details of geochemistry (including Ni-enrichment) eventually convinced him and most other people who study them that they were related to meteorite impacts. Here is the link to the abstract of a 2003 summary article by Don Lowe in Astrobiology (full article accessible via a link), as cited in our 2005 Nature article (which has a photo of the spherules):
http://www.liebertonline.com/doi/abs/10.10...110703321632408The full article reviews the historical controversies involved.
We're both Mars nuts from our earlier subsurface brine studies, and when the first web images came back from Opportunity in Eagle Crater showing the intricate pattern of cross-beds in sandy layers, I thought "surge" as a possiblity. At the same time, looking at the images on his own computer, Knauth thought "impact spherules" upon seeing the berries. We met for lunch that day and thus the hypothesis of "impact surge" was born - athough we initially called it "brine splat" to account for the salts. Shortly afterwards we invited Ken Wohletz of Los Alamos to join us, inasmuch as he knows far more about the nuts and bolts than we do. Naturally, we were both astounded by the complex "son of a beach" story, described as a scientific discovery, not merely a working hypothesis, that the MER team came up with a few weeks later - their story seemed so unlike the cold, dry Mars we knew, especially for the highlands, and ignored the impact craters all over the place.
Anyway, make up your own details, but the fact is that large terrestrial impacts (including the one that is presumed to have killed the dinosaurs, Chicxulub) produce, via vapor condensation processes, billions of spherules, comparable in sphericity and diameter to the berries at Meridiani, and scatter them at least as widely. Although terrestrial target rocks are much poorer in Fe than any on Mars, meaning the spherules are not particularly Fe-rich, the Fe in the spherules is invariably fully oxidized, and they are characteristically enriched in Ni (plus a whole suite of other elements that cannot be analyzed by the rovers). The Ni is usually concentrated in high temperature ferrite spinels, an end-member of which is the mineral trevorite, NiFe2O4 (Ni is 2+, Fe is 3+). No one yet knows how Ni occurs in the Ni-enriched Meridiani berries (Oppy's instrumentation is too primitive).
The MER team has argued that Oppy's berries can't be impact spherules, because terrestrial examples tend to be concentrated in distinct beds, but this argument ignores the obvious fact of concentration by faster settling velocities through seawater plus later current reworking (analogous the the obvious fact of wind-reworking for the lag concentration of berries on the surface of Meridiani).
So there you go - I really don't know exactly where in the vapor cloud they formed, or how long it took, or the details of how they were distributed, but the inescapable fact is that impact spherules characteristically happen, at least for ancient impacts on Earth (like Mars, a planet with atmosphere and subsurface volatiles).
Hope this admission of ignorance helps.
HDP Don
P.S. Please note that for purposes of simplification I am using "impact spherules" in a very general and inclusive way that not all scientists would agree with (especially those who like to sub-classify everything). I am using it for all varieties of spherules resulting from vapor condensation after an impact (and excluding the splash droplets called tektites). Such condensates include direct condensates such as metals, glasses, minerals presumably including hematite, salts, brines, and liquid water or ice and snow. Some direct condensates, particularly brines, form sticky coatings on surfaces of other particles and tend to stick them together into spherical aggregates called accretionary lapilli. Accretionary lapilli and rare glassy microspherules can be produced by volcanism; the other varieties seem to require impacts (much more vaporization at a larger scale). Most impact spherules (direct condensates) are tiny and on Mars probably would be lost among the sand grains. Accretionary lapilli tend to be the largest impact spherules (or impact-related spherules, for the purist) and, as indicated in previous posts, that is what we hypothesize the hematitic spherules at Meridiani to be. Evidence, in addition to their relatively large size, includes the concentric structure seen in some broken ones, their sticky nature as indicated by occasional doublets and far rarer triplets, and doubts about their hematite content (somewhere in the range of 50-100%). The terrestrial impact spherules referred to above are mainly relatively large accretionary lapilli and other spherules believed to represent altered glass. Accretionary lapilli formed solely by terrestrial particulate matter plus condensing steam would not be expected to display an extraterrestrial trace element signature and, indeed, many don't (which is one reason why their impact origin has been controversial). Sorry for the technical lecture - I tend to oversimplify for this audience, and my co-author Knauth objected when he read the above post.