1. Genesis and preservation of uranium
mineralisations in Phanerozoic
Australian sedimentary basins
Pierre-Alain Wülser
Origin of Sandstone Uranium Deposits: A Global Perspective
IAEA – Vienna 29th of May – 1st of June 2012
AUSTRALP SARL, P.O. Box 72, 1292 Chambésy, Switzerland
pierre-alain.wulser@australp.ch
2. Objectives & plan
Most sandstone-hosted uranium occurrences in Australia share
common characteristics which may relate to similar genetic
histories in defined locations (X,Y,Z) and potentially to a same
metallogenic epoch (t)
Using these observations, can we restrict Sst-hosted U targets to
smaller geological objects, restricted strata?
To document this, we will review U occurrences in Phanerozoic
Australian basins and look at several aspects
Selected mineralisation description, depositional environment
of host formations
Sea level variations and paleoclimate
Geochronology of uranium ore in sandstones
We will then try to define the best periods of U mobility for
sandstone-hosted mineralisations
Giving new tools for exploration
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Genesis & Preservation of U mineralisation in Australian sed
3. Uranium in Phanerozoic Australian basins
Australia is a relatively low
standing continent
Sea level variations have
controlled the development of
sedimentary basins
Sst-hosted Uranium occurrences
in Australia are dominantly
located in Cretaceous –
Cainozoic strata
Less important resources occur
in Lower Carboniferous
sandstones units
Dominantly two types settings:
Intracontinental sandstone
plateau or molassic basins
Estuarine (deltaic) setting in
Selected Phanerozoic basins of Australia either marine or lacustrine
& Sandstone hosted occurrences environments
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Genesis & Preservation of U mineralisation in Australian sed
4. Uranium primary sources
Many U-rich Archean and
Proterozoic granites (>10
ppm)
The U-rich sources are
drained into
Closed intracontinental
sedimentary basins (Central
Australia, Eyre basin / fluvial
to lacustrine transition)
Open basin (fluvial to
marine transition)
Spatial link between
Sst-hosted U & sources
Source: Geoscience Australia
Radiometric map of Australia in ternary colors (U-Th-K)
& Sandstone hosted occurrences
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Genesis & Preservation of U mineralisation in Australian sed
5. Characteristics of Sst-hosted mineralisations
66% of Sst-U is located in Cretaceous-Eocene strata, only 21% in
Early Carboniferous and 13% in Miocene-Pliocene strata
54% of known Sst-U is located in South Australia
67% of U stands below actual sea level
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Genesis & Preservation of U mineralisation in Australian sed
6. Sea level variations & impact on Sst-hosted
uranium mineralisations
Lake Eyre
Basin
A sea level rise of 100 m provides a rough image of how
landscape must have looked like during Cainozoic sea
transgressions
Most deposits sit under present sea level and marine, lacustrine
estuarine protective caps developed on the top of the
sandstones formations during transgressions
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Genesis & Preservation of U mineralisation in Australian sed
7. Altitude & localisation of mineralisations
NT mineralisations
formed in
intracratonic
basin, were later
tectonically &
verticalized.
Mineralisations are
partly oxidised
and occur at
surface (carnotite,
U phosphates,
etc.)
Deposits with high standing U show evidence of Miocene-
Pliocene uplifting (e.g. Mulga Rocks, Four Mile W, Warrior,
Angela Pamela, Bigrlyi, Walbiri)
Miocene (and/or Pliocene) marine or lacustrine clayey formations
are overlying all mineralisations, except at Angela-Pamela, Walbiri
& Bigrlyi (NT)
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Genesis & Preservation of U mineralisation in Australian sed
8. “The coyote is always looking for what is odd;
like him, I am looking for what is not at its
normal location” Bernard Tagini, 1975
Several “chosen” deposits will be discussed
here:
1. Oobagooma (WA)
2. Mulga Rock (WA)
3. Mullaquanna (SA)
4. Beverley (SA) & Four Mile East (SA)
Initially low-standing (+50 to -50 m) sandstones seem to host
most of Sst-U in Australia
The odd: Mulga Rock (WA)
Early Cretaceous - Eocene strata seem to host most of Sst-U in
Australia.
Discussed exception: Oobagooma (WA) & Beverley (SA)
Can we use U-Pb geochronology of U ore to constrain our
understanding the age of uranium deposition?
New U-Pb isotopic geochronology studies on Beverley & Four Mile East
mineralisations
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Genesis & Preservation of U mineralisation in Australian sed
9. 1. Oobagooma deposit (NE Canning Basin)
Oobagooma is
West Kimberley
crystalline basement hosted by Early
Oobagooma Carboniferous
U Yampi Sst
-ri
c hs The sandstone is
Ki oun
ou exposed at the
S
ng d
rce surface in the
Robinson River
catchment
Yampi Sst were
deposited in a
fluvio-deltaic
environment
during warm,
humid tropical to
sub-tropical
Radiometric map of the West Kimberley region climate
Map based on Geoscience Australia data
Oobagooma: 9950 t @ 1200 ppm U3O8
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Genesis & Preservation of U mineralisation in Australian sed
10. 1. Detailed setting of Oobagooma deposit
r
Rive
son
Robin
Yampi Sst : Deltaic / fluvial sequence (strong tidal influence)
Currently connected with the Robinson River drainage
Fault-bounded basin
Mineralisation occur at a salinity transition (300 to 700 µΩ.cm-1)
between saline marine / fresh water from the Robinson drainage
Did uranium deposited during Palaeozoic?
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Genesis & Preservation of U mineralisation in Australian sed
11. 2. Mulga Rock (& Warrior), Eucla basin
Hou et al. (2008) Mulga Rock (& Warrior)
deposits are located in Eocene
paleovalleys on the internal
margins of the Cainozoic Eucla
Basin
The incised valleys were filled
Mulga Rock with fluvial Mid-Eocene
sandstones, lignitic sandstones
and locally lignite
Warrior
Mulga Rock
Warrior
Hou et al. (2008)
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Genesis & Preservation of U mineralisation in Australian sed
12. 2. Mulga Rock deposits (Eucla basin)
Energy Minerals Australia Pty Ltd
U is contained in (1) sandstone and (2) lignitic sandstones
(coffinite) and in (3) overlying lignite (organometallic binding
with UO2+ complexes)
The drainage is close to crystalline basement containing U-rich
Archean granites (& TTG)
Mulga Rock: 27100 t @ 560 ppm U3O8
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Genesis & Preservation of U mineralisation in Australian sed
13. 2. Mulga Rock cross-section & mineralogy
Organometallic complexes with lignite host most of U and Ti, V,
Co. Polymetallic concentrations are present in the lignite: Co-
Ni-Fe-Cu (as sulfides) and REE, Sc, Ti in complex speciation.
Uranium is hosted by coffinite in sandstones
A) Fe,Co sulfides in lignite
B & D) Chalcosite & covellite in clayey lignite
Ti-Si (Sc)-rich layers in lignite layers (Fig. C)
Fe,Co Cu
Cu
Ti-Si
13
Genesis & Preservation of U mineralisation in Australian sed
14. 2. Eucla Basin general & unequal uplifting
Uranium mineralisations from
Eucla basin have been subject to
differential uplifting from their
original elevation (+100-200 m for
the western Eucla Basin)
C’
Uplift occurred from 10 Ma (Late
C Miocene – Pliocene)
Hou et al. (2008)
Hou et al. (2008)
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Genesis & Preservation of U mineralisation in Australian sed
15. 2. Mulga Rock summary (Eucla Basin)
The Middle Eocene fluviatile paleovalley fill at Mulga Rock is
built on the Gunbarrel basin (Early Permian-Late Carboniferous
glaciogenic sedimentary basin) and on the Proterozoic / Archean
crystalline basement
The fluviatile Middle Eocene sequence is covered by oxidised Late
Eocene, Miocene to Pleistocene strata. Two major Miocene
transgressions (lacustrine turbidites and diamictites & estuarine
sandy, clayey successions) are recorded. The depositional
environment was mostly fluviatile /fluvio-lacustrine /marginal
marine.
The entire Eucla basin & Southern Yilgarn Craton was uplifted
during the Late Miocene-Pliocene (10 – 0 Ma)
The Miocene overlying basin consists of clay and sandy clay
formed in a estuarine, marginal marine environment (typical
Miocene transgression present all around Australia)
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Genesis & Preservation of U mineralisation in Australian sed
16. 3. Mullaquanna / Blackbush deposit (SA)
Mineralisation occurs in
coarse, reduced, lignite-
bearing, pyritic Eocene
sands and lignite beds
Fluvial incised paleo-valley
(marginal marine,
estuarine setting)
The deposit is located at
the margin of a U-rich
catchment from the Gawler
Craton (Archaean –
Proterozoic granites)
Mullaquanna: 19000 t @ 280 ppm U3O8
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Genesis & Preservation of U mineralisation in Australian sed
17. 4. Mineralisations from the Lake Eyre Basin
(Callabonna sub-basin)
The Callabonna sub-basin
contains most of Sst-hosted
Australian uranium resources
Mount Painter
Miocene tectonic uplift subdivided Domain
the Lake Eyre basin into sub-
basins at ~10 Ma
Past connection between the Tirari
sub-basin and Pirie-Torrens basins
existed until then
Major Recent-Pliocene uplift
increased and U-rich sources
exposure (Mt Painter Domain) and
triggered uranium mobility
Sea-level variations and climatic
conditions (humid or dry) have
impacted on Lake Eyre Basin, with
several sea transgressions
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Genesis & Preservation of U mineralisation in Australian sed
18. 4. Mineralisations from the Lake Eyre Basin
Extraordinary primary U sources from the Mt Painter Domain
with granites up to 150 ppm U (in white on radiometric map)
Dispersion of U-rich sediments into the Lake Eyre Basin ~150-200
meters over the sandstone-hosted mineralisations
20 km
Lac Frome
Beverley
Four Mile E
Pic
tu Four Mile W
re
vie
w
Geoscience Australia (2009) Beverley- 4 Mile district = 57000 t @ >2000 ppm U 3O8
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Genesis & Preservation of U mineralisation in Australian sed
19. The fate of 222Rn & its impact on U-Pb
geochronology : zoom in
Direct 238U measurement by prompt fission neutrons The duration of the
(PFN.) radon stage during
Bourdon et al. (2003)
radioactive decay is
highly changing fro the
three series
For 238U series, 222Rn
stage is 50000 x
longer than 219Rn stage
(235U decay series)
T1/2222Rn
T1/2219Rn
= 50000 ( = 1) T1/2220Rn
= 300 and for 232Th series,
T1/2219Rn 220
Rn stage is 300 x
longer than 219Rn stage
Radon loss is more
effective for 222Rn
Indirect U measurement U-Pb isotopic
on 214Bi γ emission measurement
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Genesis & Preservation of U mineralisation in Australian sed
20. Insights from Gamma (γ) vs. PFN log data –
Direct evidence for 222Rn leakage in ore
Comparison between calibrated
Gamma spectrometric log (214Bi)
& Prompt fission neutrons logs
(238U) assays
Average disequilibrium at 0.70
for 214Bi/238U
30% of the expected 206Pb
must have be lost (in average)
Measured 206Pb/238U isotopic ratio
(Gamma)
in whole-ore can be readjusted
Wülser et al. (2012) for 214Bi/238U disequilibrium
(PFN)
It is expected that 235U/207Pb ratios
are valid after common lead
deduction (204Pb-based or 208Pb
Equivalent U3O8 grades from correction if no 232Th is present)
gamma log versus grades from
PFN - Four Mile East deposit (SA)
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Genesis & Preservation of U mineralisation in Australian sed
21. Example 1: Shirley Basin, Wyoming, USA -
further evidence for 222Rn migration
Common Pb correction applied based
on 204Pb
Mineralisation hosted by Early Eocene
Wind River Formation
charcoal Evidence for 222Rn migration and
pyrite accumulation of 206Pb in “charcoal”
Overall identical 207Pb/235U ratio in whole
n
tio
Rn migration
ore, charcoal and pitchblende
ra
ig
m
Pb
Minor remobilisation of radiogenic Pb
ic
from pitchblende into pyrite
g en
io
222
d
Ra
Interpreted age of 24 ±3 Ma
Whole-ore
(Oligocene) for ore genesis (207Pb-235U-
Pitchblende based)
Ludwig 1978, Economic Geology, 73, 29-49
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Genesis & Preservation of U mineralisation in Australian sed
22. Example 2: U-Pb geochronology by ICPMS
at Beverley & Four Mile East
Pitchblende FME
Dense
Porous coffinite nodules
Qz
pitchblende in mudstone at Beverley
U
Pitchblende cement in
high-grade FME sands
Very reducing
microenvironments
Coffinite Beverley present in lacustrine silts
of Beverley, with
bacterial activity
Pitchblende yielded
concordant age of 6.7
Ma at Beverley
Coffinite Beverley
Whole-ore
Four Mile East
Pitchblende gives
207
Pb/235U ages of 12.8 to
2.8 Ma at FME
Coffinite gives 0.4 to
2.6 Ma 207Pb/235U ages at
Beverley
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Genesis & Preservation of U mineralisation in Australian sed
23. La-ICPMS U-Pb Geochronology at Four Mile
& Beverley. Miocene-Pliocene U migration
Carnotite Concordant carnotite at Beverley: 5.5 – 3.4 Ma
In summary, 207Pb-235U, common Pb corrected
ages on pitchblende & coffinite at Beverley & FME
give:
Beverley: 6.7 - 0.4 Ma
FME: 12.8 - 2.8 Ma
Denser pitchblende retain 222
Rn better and give
higher 206Pb/238U ratio
Late Miocene to Pliocene mineralising events
in the Lake Eyre Basin
Wülser et al. 2011, Economic Geology, 106, 835-867.
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Genesis & Preservation of U mineralisation in Australian sed
24. U-Pb geochronology of sandstone-hosted
uranium mineralisations: summary
Because of the longer half-life of 222Rn, radon leakage mostly, or
only affect the 238U-206Pb decay series
Porous U ores (coffinite coatings) allow important loss of 222Rn
(~30% at Four Mile East), possibly trapped by charcoal in the ore
(e.g. Shirley Basin, Wyoming)
U-206Pb system is partly open in most sandstone-hosted
238
uranium mineralisations, but radon loss (219Rn) has only limited
effect on 235U-207Pb decay series.
Dense pitchblende cement retain radon better and can provide
good 207Pb-235U ages after common lead correction Crystalline
minerals (e.g. carnotite) retain 100% of radon and can provide
concordant ages
U-Pb isotopic data need completely different interpretation from
classic U-Pb mineral dating (e.g. zircon) and the notion of
“concordance”, “207Pb/206Pb ages and “lead loss” is erroneous when
effective 222Rn loss is present.
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Genesis & Preservation of U mineralisation in Australian sed
25. Intermediate summary
A generally low standing altitude (-50 to + 50m)
Sea level variations / marine (lacustrine) transgressions have
generally capped the U-hosting formations
Problems met in geochronology can be solved
New U-Pb ages of mineralisations in SA indicate Late Miocene to
Pliocene ore deposition
Uranium in Australian Phanerozoic formations is dominantly
located in organic-rich Middle Eocene sandstones. This also
indicates most of uranium mineralisation formed from Late
Eocene to Pliocene)
Uplifting impacted on preservation and post-ore mobility
(oxidation & multiple remobilisations in deposits from central
Australia)
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Genesis & Preservation of U mineralisation in Australian sed
26. Influence of paleoclimate on uranium mobility
1. Middle
Eocene:
warmer &
wetter than
present
2. Early
Miocene:
warmer than
present
3. Middle
Miocene:
warmer than
present
Hou et al. (2008)
Wetter and warmer climate (Middle Eocene) was certainly not adequate for uranium
release without dispersion (excess of flowing, with deeper chemical alteration of rocks).
This period is responsible for large sandstone units generation, containing abundant
organic matter (presence of widespread rainforests) and that were later mineralised in
uranium
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Genesis & Preservation of U mineralisation in Australian sed
27. Cainozoic paleoclimate summary
Pliocene /Pleistocene increasing aridity, drying
up of the lake systems, cyclic arid / episodic wet
(following cycles of the Pleistocene glaciation)
Late Miocene progressive temperature decline
Miocene strong climatic warming, several sea
water influx into the Lake Eyre basins (dolphins fossils
& oolithic dolomite)
Oligocene to Early Miocene dominantly warm
and dry climate
Middle Eocene-Early Miocene drainage of the
Lake Eyre basin toward SW, into Pirie & Eucla basins
(zircon populations based). Early Eocene warming
Palaeocene-Middle Eocene much warmer than
present, warm sea influence with south-westerly
winds, development of temperate rainforest in South
Central Australia (Alley, 1998). Strongest warming in
the Middle Eocene
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Genesis & Preservation of U mineralisation in Australian sed
28. Uranium mobility – eustatic variations &
paleoclimate during Cainozoic
U was not deposited
during marine
transgression periods
Most of U is located
between -80 and 0
meters elevation
Three periods of low
sea level correspond to
max emerged / marginal
setting
U1 (0 – 5.3 Ma,
Pliocene-Pleistocene), U2
(5.5 – 12.6 Ma, Late
Miocene, U3 (23.4 – 28.6
Ma, Late Oligocene)
Modified from Hou et al. (2008)
First U-Pb ages on U ores confirm U1 & U2 (Bev. & FME)
suggesting low sea level periods & cooler climate were more
favourable to uranium mobility & combined trapping
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Genesis & Preservation of U mineralisation in Australian sed
29. REE distribution in uranium ores
High REE : REE are more soluble in the
source (apatite, bastnäsite, altered allanite)
(Mulga Rock)
Strong negative Eu/*Eu anomaly:
Proterozoic-Phanerozoic granitic sources
(Beverley, Four Mile, South Callabonna,
Mullaquanna)
Weak Eu/*Eu anomaly: typical Archean
granodioritic/greenstone cratons (Mulga
Rock, Yilgarn Craton)
Absence of Eu/*Eu anomaly: mantle
source (no examples)
Negative Ce anomaly: intensity of
oxidation process during primary U leaching
REE patterns document on under warm/humid (tropical) climate:
the source of uranium (Mullaquanna, Four Mile, South Callabonna)
and the processes of Absence of negative Ce anomaly: milder
weathering of uranium uranium release from source under cooler,
temperate cilmate, mild weathering
conditions (Beverley, Mulga Rock)
Absence of neg. Ce* at Beverley agrees with mild Pliocene weathering release
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Genesis & Preservation of U mineralisation in Australian sed
30. Summary and conclusion
Sea level variations seem to have played a key role in forming
the right sedimentological setting for U trapping
Adequate trapping Sst strata formed during warm and wet
paleoclimate (Middle Eocene) and located at the right
elevation are strongly prospective areas in Australia
U-Pb Geochronology works. 206Pb/238U system is fundamentally
different from 207Pb/235U system for Sst-U mineralisations because
of differential radon leakage
Integration of new geochronology to paleoclimate /sea level
reconstitutions define the best periods of U mineralising
events: (U1) Pliocene-Pleistocene, (U2) Late Miocene, (U3) Late
Oligocene)
Without surprise, the presence of U-rich exposed granitic sources
plays a fundamental role for uranium mineralisation genesis
REE patterns are useful indicators of the source rock of the ore
(intensity & curve)
Negative cerium anomalies can be used as a potential
paleoclimatic proxy for the conditions of U release
30
Genesis & Preservation of U mineralisation in Australian sed
31. Thank you for your attention
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Genesis & Preservation of U mineralisation in Australian sed