As I recall, the ambiguous results of the Viking landers' life detection experiments were explained at the time by postulating that the surface soils are highly enriched with extremely oxidized clays (I seem to recall descriptions of clays enriched with peroxides).
Nearly identical results were seen at both V1 and V2 sites, so, assuming that the results are explained by what was called "exotic soil chemistry," this chemistry would have to be widespread on Mars.
We now have some very good elemental analyses of the Martian soils, both from orbit and ground-truth from the MER rovers. In these analyses, clays seem not at all widespread, only appearing in very, very old outcrops that were presumably laid down during a very short geological timeframe during which non-acidic water was common on the Martian surface.
Soils in the Viking landing sites would appear, from the more advanced sensors we've flown since Viking, to be basaltic with admixtures of ferrous sulphates. Not exactly the exotic chemistry required to explain the Viking results.
So, the million-dollar question seems to be: if the Viking experiments can only be explained by *either* biotic processes that do not involve what we always considered the pre-requisite organic molecules, *or* by ubiquitous exotic chemistry in the soils that we're simply not seeing with more advanced instruments, which theory are we forced to accept as fact?
If neither, then what theory *does* account for the Viking results?
-the other Doug
Not really -- the main element involved is oxygen, in combination with either hydrogen or a wide variety of metals already known to exist in Martian minerals. (That's not counting Albert Yen's alternate theory, which simply calls for unusually shaped and electrically charged microscopic surfaces on ordinary Martian mineral crystals.) Nailing down the Oxidant Mystery is likely to be the major contribution of Phoenix's wet chemistry experiment.
I would note also that some in the anti-life camp still use the lack of organics found by Viking as an argument, despite the fact that it was later shown that the detector used on Viking was not able to verify the smaller traces of organics in testing done in the Antarctic (I think that's where it was done), which were in the soil and confirmed by better instruments. If similar trace amounts of organics had been in the Martian soil, Viking could or would have easily missed them completely.
I've also seen other later papers which now dispute the idea that the Martian soil is so highly oxidizing, yet that is also still used as a primary anti-life argument and has been widely accepted as fact, but again there is no real firm consensus or agreement on that.
There are certainly SOME major oxidants in the soil -- the fact that Mars' soil retained much of its oxidizing power even after being roasted at several hundred degrees proves that. Any germs capable of withstanding that must hail from the planet Krypton. This, in turn, makes it a suspicious coincidence that the results from the Labeled Release experiment could be due to actual germs living in the same highly oxidizing environment -- and more likely that the LR results are just from another type of nonliving oxidant which does break down under heating.
In this connection, the new LPSC had an abstract connected with the recent studies of the very powerful (and bacteria-destroying) oxidants which have been discovered in the Atacama Desert's soil, produced by regular Earth sunshine: http://www.lpi.usra.edu/meetings/lpsc2006/pdf/1778.pdf . It claims that "hydrogen peroxide together with hematite reproduces the kinetics of the LR experiment", and indeed the reaction does follow the time curve of the Viking results very closely -- but the study didn't test whether this reaction ceases when the soil is heated. (There are a number of LPSC abstracts dealing with Atacama soil, and I haven't yet read all of them -- I'll see whether any of them mentions temperature-dependent effects.)
Well, there are no LPSC abstracts this year dealing with the thermally "labile" (unstable) oxidant suggested by the Viking LR experiment, although there are four other interesting papers dealing with the overall question of the surface destruction of Martian organics: # 2098, 2162, 2262 and 2397.
Plausible post-Viking studies interpreted the weathered component of the soils as being dominated by "palagonite", which is a mineraloid -- not a mineral -- derived by hydration and weathering of volcanic glass, without well defined mineral content or well-crystalized phases. This goes with the lack of well defined oxide or oxy-hydroxide mineral spectral signatures for a lot of the reddish iron color in the global dust and reddish soils. Added to these dust coponents in the soils were assumed to be basaltic and related sand minerals, sulfates and other water soluble salts and oxidizing compounds, possibly metal peroxides.
One thing Gil Levin doesn't seem to want to talk about much is the glaring LACK of one finding from his experiment. While he found a sterlization-destroyable release of carbon-bearing gas from his radioactive "soup", the reactions were "one-shot" events that happened immediately upon addition of the soup, and there was no growth signature, no delay and increase in gas output whatever. This behaviour is consistent with a rapidly reacting chemical in the sample and not growing organisms. Abundant metabolizing organisms that progressively die off is consistant with the observations, but I don't know to what extent he modeled the plausible biomass required for the prompt gas evolution rates.
And to add to this - the APXS's on MER can't detect hydrogen, and if your trying to find peroxides........
To carry on JR's analogy - It's like knowing how many of every letter EXCEPT E there are in a paragraph, and wondering what it means.
Doug
Silly Question of the Day: When they designed Viking to look for
life on the Martian surface, why didn't they include instruments to
fully analyze the materials to separate and detect the inorganic
elements?
Didn't they want to know what the Martian surface was made of
outside of the life issue? I am still amazed at how much of the
results were left to guesswork.
Actually, the one instrument for inorganic analysis of the surface -- the X-ray spectrometer -- was itself a last-minute addition to the payload, put on only in 1971 after a growing number of scientists raised a stink about the lack of any such instrument whatsoever. Viking was explicitly designed as a biological mission, becuase that was by far the highest-priority scientific question about it -- and it was assumed at the time that more Mars missions would soon follow to do other research. (Which, of course, they would have done had the Shuttle not eaten up all the space-science funding in the 1980s.)
This brings us back yet again to that interminable debate: if the manned program (in this case the Shuttle) was removed, would the total funding for the unmanned program increase or decrease? I still see absolutely no logical argument that it would have decreased. The Space Pork Congressmen, without a manned program to supply their districts with that pork, would have supported a compensatory bigger unmanned program; and the public seems quite interested in some spects of unmanned space exploration -- what they want to see is something new and interesting, and they don't much care whether it's Buzz Lightyear or Robbie the Robot holding the camera. TOTAL space spending would certainly have decreased (explaining by itself NASA's frantic support for Shuttle and Station by any means necessary, up to and including regularly committing perjury before Congress), but that's an entirely different matter.
As for the Reagan Administration having a "slash and burn" mentality: if they really had had one, they wouldn't have inflated the budget deficit to the size of the Crab Nebula. David Stockman -- the one member of the Administration who seriously favored zapping the hell out of the unmanned space program -- later wrote a bitter book on how Reagan had deceived him by falsely saying that he DID favor big spending cuts.
Well, yeah -- but virtually all the theories floating around regarding what the oxidants may be (and there are a lot) already rule out any elements which we know not to exist (or to be likely to exist) in Mars soil or atmosphere.
OK -- I think I understand what y'all are saying. I guess the absolute certainty with which the MER team, for example, comes out with statements like "these soils are ground-up basaltic dust with a small admixture of sulphate binding materials" made me think that they had identified the chemical composition of the soils pretty definitively -- and with absolutely no mention of the peroxides, etc., necessary for the old explanations of the Viking results.
So, the truth really is that the MER team states definitively what they know to be in the rocks and soils, but leaves out any references to what *else* might be in the rocks and soils? And they're making somewhat confident statements about the origins of the rocks and soils, when a whole suite of constituents -- those necessary to recreate the Viking results on chemical reactions alone -- aren't detected by their instruments and, so, aren't even discussed?
Is that what y'all are saying?
-the other Doug
David Des Marais' discussion in the Jan. 2005 "Geochemical News" that I mentioned on another thread ( http://gs.wustl.edu/archives/gn/gn122.pdf, pg. 9-16) contains quite a detailed discussion of the instruments which he regards as crucial to a remote analysis of Martian material by a rover. One is a good detector and analyzer of trace organics -- specifically, a GCMS -- and the other is a "definitive mineralogy analyzer", for which he regards an X-ray diffractometer as being best. MSL '09 will carry both -- but both require a quite sophisticated system for ingesting, grinding up and distributing hard samples like rocks, which the MERs were simply too small to carry. (The proposed follow-up "Viking 3", interestingly, probably would have carried all of these; but even if it was mobile, its range would have been far more limited than that of MSL, or for that matter of the MERs.)
And neither of these instruments would do a good job of analyzing Martian oxidants, which are very unstable and will require specially designed analysis techniques to nail them down precisely. Wet chemistry tests -- of the sort that Phoenix will do -- will probably be best for that purpose; I don't know how good MSL will be at analyzing them, although its GCMS may provide some data. In fact, oxidants probably cannot even be returned successfully in Mars sample-return missions -- they're too unstable and would break down en route, without constant reapplication of the Martian environmental processes that created them in the first place. Thus they will likely require in-situ analysis.
About a decade ago, NASA published a very authoritative guide to the sorts of analyses that different instruments on planetary landers can do -- if I can track the damn thing down. At the moment I can't find it on Google, but I know I have a copy of it somewhere.
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