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Olduvai Gorge, Tanzania: XRF and Olduvai Gorge, Tanzania: XRF and XRD studies of the geologicalXRD studies of the geologicalXRD studies of the geological XRD studies of the geological
context Early Man and Early Marscontext Early Man and Early MarsLindsay J. McHenryLindsay J. McHenry
Department of GeosciencesDepartment of GeosciencesUniversity of WisconsinUniversity of Wisconsin-- MilwaukeeMilwaukee
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Acknowledgements:Dr. Richard HayD G d i M ll lDr. Godwin MollelDr. Carl SwisherDr. Alan DeinoDr. Christian SchröderDr. Vincent ChevrierDr Robert Blumenschine and everyone in the OLAPP project groupDr. Robert Blumenschine and everyone in the OLAPP project group
Funding: The Leakey Foundation, Geological Society of America, A i Ch i l S i t Si Xi U i it f Wi iAmerican Chemical Society, Sigma Xi, University of Wisconsin-Milwaukee RGI, and NSF.
Permits: Tanzania Department of Antiquities, The Ngorongoro Conservation Area Authority, COSTECH
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OutlinePart 1: Tephrostratigraphy and GeoarchaeologyUsing the unique chemical composition of volcanic ash layers toUsing the unique chemical composition of volcanic ash layers to improve the stratigraphic and age control of Olduvai Gorge archaeological sites.
Part 2: GeochemistryThe weathering of volcanic ash at Olduvai Gorge: can we still use altered ash in tephrostratigraphy?
Part 3: MarsThe weathering of volcanic ash at Olduvai Gorge: analogue for e we e g o vo c c s O duv Go ge: ogue oMars?
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How “tephrostratigraphy” works
Major explosive eruptionsMajor explosive eruptionsblanket the landscape withvolcanic ash.
Most volcanoes produce ash that is uniquelyash that is uniquelyidentifiable based on itschemical composition
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Feibel, 1999
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Volcanic ash = shards of glass + tiny mineral grains
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Sample prep for compositional analysis of ash. (Feibel, 1999)
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Feibel 1999
Some ashes (e.g. Tulu Bor) are well suited to a “bulk” compositional technique like XRF, others are not
Feibel, 1999
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Gulf of Aden
Awash
Gulf of Aden
Turkana
Olduvai Gorge
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Regional tephra correlations: Turkana (Kenya) to Awash (Ethiopia) and offshore (Gulf of Aden)( )
Feibel,1999
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Ash layers from Yellowstone and Long Valley calderas
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Olduvai Gorge, Tanzania: Pleistocene
Postcard: © David Keith Jones FRPS
Many hominid fossils: Homo habilis, Homo erectus, Australopithecus boisei, Homo sapiens.Stone artifacts: Oldowan, Developed Oldowan, Acheulean, etc.Extensive faunal remains
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Olduvai Gorge and nearby volcanic sources
Ngorongoro VolcanicVolcanic Highlands (NVH)
Olduvai GorgeActive 4.32 Ma to today
NVH
20 km
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Collecting samples: summit g pof Oldoinyo Lengai volcano, Tanzania, July 23, 2007
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Oldoinyo Lengai,S t 4 2007Sept. 4, 2007(satellite image)
(glad I wasn’t(glad I wasn t there at the time)
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Olduvai: Near source volcanoes, with a good ash record.record.
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To conduct landscape archaeological research, you need to be able to identify the same “time slice” across the landscape
At Olduvai this is accomplished using volcanic ash layers, or “Tuffs”
Tuff IF
Ng’eju TuffTuff IE
Tuff ID
Upper Bed I tuffs at the “Zinjanthropus” site McHenry, 1999
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Principal Method:Principal Method:
Elemental analysis of volcanic minerals andElemental analysis of volcanic minerals and volcanic glass, where available.
Most tephrostratigraphy research uses glass alone. This is impossible at Olduvai, where glass is rarely preserved.
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Tuff1.7Age (Ma)
ed II Nephelinite/ Foidite
Rock Type
0
GPTSOlduvai
Stratigraphy
Tuff IIA
Tuff IF
Ng'eju Tuff
?
Low
er B
e
Trachyte
Basalt
Rhyolite
Ndutu andNaisiusiu Beds
Masek Beds
Bed IV
0
0.5
PLE
ISTO
CE
NE
Bru
nhes
1.8Ngeju TuffTuff IE
Tuff IDTuff IC
Tuff IB?
?
Upp
er B
ed I
TrachyandesiteBed III
Bed II
1.0
P
atuy
ama
Tim
e (M
a)
GPTS after Berggren et al., Bed I lavas
Mafic Tuff?
1.9
wer
Bed
I
Bed I
1.5
2.0
Tuff IIATuff IFTuff IB
CN
2M
a T
1995. Correlation to the GPTS and specific ages for the Bed I tuffs are based on dates from Hay, 1976, Walter et al 1992 Hay and
Tuff IA
CFCT
?2.0
Naabi Ignimbrite
Low
NgorongoroVolcanics
2.5
LIO
CE
NE
uss
Walter et al., 1992, Hay and Kyser, 2001; and Blumenschine et al., 2003. Olduvai magnetics of Tamrat et al., 1995.
2.1
Naabi Ignimbrite
3.0
PL
Gau
Bed I tuffs in context.
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Sample Sites
Loc 200
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Fresh glass: Great where you’ve got it!
(TiO2 vs. Al2O3)
Tuff IBTuff ICTuff ICTuff IDTuff IENg'eju Tuff (Lower)Ng'eju Tuff (Upper)Tuff IF SurgeTuff IF LapilliTuff IF Lapilli
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Feldspar: Great everywhere!
Tuff IB (Junction)Tuff ID (Junction)Tuff IE (Junction)
Ng’eju lower
Ng’eju lower
Tuff IE (Junction)
Tuff IB (Lake)Tuff ID (Lake)Tuff IE (Lake)Ng'eju Lower (Lake)
Ng'eju Lower (Junction)
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Bed I tuff correlations within Olduvai
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Stratigraphic placement of Olduvai hominid 65
Tuff IF
g p p
Ng’eju Tuff
Figure 2 from Blumenschine et al., 2003
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Part 2: GeochemistryPart 2: GeochemistryA serious limitation of the method used forA serious limitation of the method used for tephrostratigraphy at Olduvai is that volcanic minerals don’t vary much in composition.minerals don t vary much in composition.
Analyzing fresh glass would be ideal, but it is no longer preserved at Olduvai.
W ld it b ibl t th “b lk” itiWould it be possible to use the “bulk” composition of the altered volcanic ash for fingerprinting?
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Part 2: GeochemistryPart 2: GeochemistryS l t ( Al Ti Z Nb Th T )Some elements (e.g. Al, Ti, Zr, Nb, Th,Ta) are considered “immobile” during weathering.
However, most studies have involved materials lt d d t l li htl idi ditialtered under neutral or slightly acidic conditions.
Are the same elements immobile during zeoliticAre the same elements immobile during zeolitic alteration under saline-alkaline conditions, such as at Olduvai?as at Olduvai?
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McHenry, 2001
The target: a single layer of Tuff IF1 A j Old i G k ff b 1 79 M1. A major Olduvai Gorge marker tuff, at about 1.79 Ma.2. Preserved and easily identified over a broad area.
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Sample sites, in relation to the “paleo-lake” environments of Upper Bed Ienvironments of Upper Bed I.
Paleoenvironments after Hay, 1976
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MethodsMethodsLapilli hand-picked and cleaned
XRF of powdered lapilli separates for major and minor elements.
ICP-MS of powdered lapilli separates for trace elements
XRD of powdered lapilli separates for phase identificationXRD of powdered lapilli separates for phase identification
SEM of intact lapilli for textural imaging.
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Volcanic glass is replaced by zeolites in the lake
5 μm5 μm
center, and by clay minerals in the lake margin.
Phillipsite laths, intermittently dry saline lake.
Clay and minor analcime, lake margin.
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Major element mobility during alteration of Tuff IF lapilli: zeolitic vs. clay alterationIF lapilli: zeolitic vs. clay alteration
SiO2
TiO2
zeolitizedfreshclay alteredTiO2
Al2O3
O
Si, Ti, Al, Fe, Mn little
clay-altered
FeO
MnO
changed in either.
MgO
CaO Ca leached in both
Mg enriched in both
Na2O
K2O
Na slightly enriched
K leached-80 -60 -40 -20 0 20 40 60 80 %
diff
% difference compared to “fresh” sample from Locality 40 (MCK)
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Trace element mobility during alteration of Tuff IF lapilliNbNb
Hf
T
Nb enriched in zeolitic, depleted in most clay-alteredTa
Th
U
most clay altered samples
Hf Th and ZrU
Sc
Hf, Th, and Zr depleted in zeolitic, conserved (or
Sr
Zr
enriched) in clay-altered samples
Cs
Rb zeolitizedfreshl l d
-60 -40 -20 0 20 40 60
Ba
%diff
% difference compared to “fresh” sample from Locality 40 (MCK)
clay-altered
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C l iConclusionsUnfortunately, the generally “immobile” elements Ti and Zr appear to be mobile under the saline-alkaline conditions at Olduvaiconditions at Olduvai.
Of the elements analyzed, only Al and Ta appear toOf the elements analyzed, only Al and Ta appear to remain immobile (within 10%) across all alteration environments studied.
Bulk composition of altered ash is thus NOT a viable th d f t h t ti h i thi i tmethod for tephrostratigraphy in this environment.
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An interesting, and unexpected, discovery d d i hi d
Jarosite and phillipsite in the saline-
made during this study:
alkaline lake sample (Loc 80)
XRD (K-jarosite peaks in red)
and this leads us to…
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Part 3: Mars
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Initial observations:
Some altered ashes from the paleo-lake contain jarosite in a deposit otherwise dominated by phillipsitedeposit otherwise dominated by phillipsite.
Conventionally, jarosite indicates acidic conditions (pH < 5). Its presence on Mars is a leading line of evidence in support of a wet, acidic past.
Conversely, phillipsite is a zeolite characteristic of K-rich, saline-alkaline conditions (pH > 8, usually >9).
Question:
How could these two phases coexist?
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L 80Locs 77, 78
Loc 80
Loc 54
Map of sampled localities and Olduvai paleoenvironments atMap of sampled localities and Olduvai paleoenvironments at time of Tuff IF deposition. Figure after Hay, 1976
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Methods:
• XRD of all samples: phase identification.
XRF f l i h d i h j i C i i l diff ?• XRF of samples with and without jarosite. Compositional difference?
• SEM and EPMA of a few confirmed jarosite occurrencesj- Crystal shape, association, qualitative composition
f f j i b i l• NIR spectroscopy of a few jarosite-bearing samples.
• Mössbauer analysis of a few jarosite-bearing samples, using MER-össb ue ys s o ew j os e be g s p es, us glike Mössbauer Spectrometer at Mainz.
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Occurrence of Jarosite: 10 / 58 samples, from four sites, i d bl j i All d i d b hilli icontained measurable jarosite. All were dominated by phillipsite.
Example: Loc 80
6% jarosite41% hilli i
Example: Loc 80
41% phillipsite20% authigenic K-spar4% analcimecontains smectite
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Jarosite and phillipsite in saline-alkaline lake altered phonolitic Tuff IF, Loc 80
5 μm
Jarositepscp
Phillipsite
XRD (K-jarosite peaks in red, hilli it i bl )
S
cps
phillipsite in blue) SEM SE image
K
Fe
EDS spectra (S, K, and Fe labeled)
Energy (keV)
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Olduvai vs. Martian jarosite: M össbauer results
Meridiani Planum jarosite and hematite
Olduvai jarosite and smectite
Klingelhöfer et al. (2004), Science 306, 1740-1745; Morris et al. (2006), JGR 111, E12S15
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sites where jarosite has been identified by XRDsites where Tuff IF has been XRDed, no jarosite
Jarosite is limited to the most altered samples, formed under the most saline-alkaline conditions.
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Is the modern groundwater saline-alkaline, or idi ?acidic?
Evidence for modern saline-alkaline groundwater:• Na-bicarbonate spring precipitates (dominantly trona)
Hi h H (9 29 9 54)• High pH (9.29-9.54)
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Hypothesis: The jarosite is younger than the zeolites formed by recent pyrite oxidationzeolites, formed by recent pyrite oxidation.
Phillipsite and pyrite formed initially in high-pH, reducing lakewater.
More recently, pyrite was oxidized. This process can lead to locally acidic conditions:FeS2 + 15/4 O2 + 7/2 H2O = Fe(OH)3 + 2H2SO4
XRF data confirms: higher Fe S in jarosite bearing samplesXRF data confirms: higher Fe, S in jarosite-bearing samples
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Conclusion
The presence of jarosite alone does not require widespread acidic conditions Jarosite can exist at least locally under dominantlyconditions. Jarosite can exist, at least locally, under dominantly saline-alkaline and other non-acidic conditions.
O M dditi l li f id d d t b t iOn Mars, additional lines of evidence are needed to be certain that jarosite-bearing sediments and rocks were formed under exclusively acidic conditions.
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Dedicated to the memory of Dr Richard Hay 1929 2006Dedicated to the memory of Dr. Richard Hay, 1929-2006