Naomi Porat Geological Survey of Israel
Transcript of Naomi Porat Geological Survey of Israel
Naomi Porat
Geological Survey of Israel
Geoff Duller and Helen Roberts, Aberystwyth University
• Principles of luminescence dating
• Sampling and lab work
• Obtaining precise and accurate ages
• The results
• Usefulness
The “clock”:
� Uses a physical property that grows
over time as a result of natural
environmental ionizing radiation.
� This radiation creates a signal
(electrons trapped in the crystal
lattice) whose intensity is proportional
to time and radiation.
� In the lab we measure these electrons
that accumulated over time.
� The signals are rapidly reset by
sunlight or heat.
� The method dates the last exposure to
sunlight (or to high temperature).
Physical model
Energy level in the atom
trap photons
Energetically deeper traps will be more stable over geological time scale
Signal measurement
Luminescence TL/OSL Reader (Risø DA-12)
The luminescence signals:
Optically stimulated luminescence (OSL) signal Thermoluminescence (TL) signal
� OSL of quartz, excitation in the green-blue and emission in the near UV.
� Infrared stimulated luminescence (IRSL) of alkali feldspar, excitation in
the infrared and emission in the blue-violet
Bleaching experiments of quartz and feldspar grains
(150-180 µm from southern Israel
The quartz OSL signal is reduced by 90% within 2-3 seconds.
The feldspar IRSL signal is reduced by 90% within 50-80 seconds.
After 10 minutes there is still 5% signal remaining in the feldspar.
0 10 20 30 40
Bleaching time (s)
0
0.2
0.4
0.6
0.8
1
Luminescence (normalized)
18-6 KF
18-10 KF
18-6 QZ
18-10 QZ
0 100 200 300 400 500 600
0
0.2
0.4
0.6
0.8
1
OSL signal
Thermoluminescence signal
Quartz
Feldspar
Experiments in solar signal resetting (“bleaching”)
� Two values are required to obtain an age:
1. The equivalent dose, De.
2. The environmental dose rate, D.
� The age is the ratio between these values De/D
The age equation
The Equivalent dose (Archaeological dose; Paleodose)
Measured by reconstructing the signal by a known laboratory dose
extrapolation - Added dose interpolation - Regenerative dose
From: Duller,G. A. T. 2008, Luminescence Dating: guidelines on using
luminescence dating in archaeology. Swindon: English Heritage.
A 10 mm disc
covered with several
thousands of grains.
Dose-response curve
The single aliquot
regenerative (SAR) dose
protocol (Murray & Wintle
2000).
• De is measured for a large number of aliquots from the same sample.
• Aliquot size varies, may contain from thousands to a few tens of
grains.
• Also single grains can be measured in the same manner.
• The smaller the samples size the greater the scatter.
Errors on individual measurements
include:
• Counting statistics.
• Signal to noise ratio.
• Beta source calibration uncertainties.
• Goodness of fit to the dose response
curve.
• Errors on De values are a measure of
inhomogeneity. Can be reduced by
large number of measurements and
statistics.
Dose distribution
Palaeodose(Gy)3.6 4.0 4.4 4.8 5.2
Relative Probability
N=20
De=4.2±0.1 Gy
Environmental Dose rates:
� Can be measured in the field or the
lab.
� Need to know the sum of
radioactivity from the decay of U, Th
and K in the sediment, and from
cosmic radiation.
� There are α, β and γ particles, each
with different penetration range.
� Burial depth is important for
calculating cosmic dose contribution.
� Water content needs to be known for
calculating γ absorption.
Summary:
� A dosimetric method.
� Usually uses quartz or alkali feldspar in the fine-sand size range.
� OSL is used for dating sediments reset by sunlight, such as aeolian,
fluvial, alluvial and colluvial sediments.
� TL is used for heated material such as burned flint from prehistoric sites
or ceramics from archaeological sites.
� The age range is from several hundred years to several hundred-
thousand years.
� Errors range from 5-10 % of the age.
The complex history of a quartz grain in Megiddo
• There is no quartz in the chalk, limestone and basalt constructing the local
geology of Megiddo.
• The soils in the Jezerael valley soils contains wind-blown quartz; this could
blow onto the site during dust storms or brought by man.
• Quartz may also be blown from far away during dust storms.
• Dust arriving in storms travels long distances and the OSL signal of the
quartz is most likely well bleached.
• The dust settles on the site and then accumulates in open spaces.
• In the case of local source, the quartz might carry a residual OSL signal.
• Another sources of unbleached quartz could be recycled local sediments
(when leveling an area for construction).
• Yet another source is from bricks, which are made of local material,
perhaps brought from the wadi nearby. The quartz in bricks is not
bleached.
• Very likely the quartz at the site has had a complex depositional history.
• The samples collected for OSL dating may have more than one source of
quartz, with varied bleaching histories.
Where to sample?
� Archaeologically, destruction layers are best dated.
� These could have been heated during destruction and then exposed at
the surface before the next layer was deposited.
� Sediment between building stones. This was either placed during
construction or accumulated later from wind, and in this case is well
bleached. Will give a minimum age.
� Sediment from living floors and court yards.
� Sediment from water-lain features.
M 8/M615
ca. 1000 BCEM 414,16
ca. 850 BCEL 313
800-732 BCEL 212
ca. 3000 BCEJ 411
Destruction ca. 1130 BCEK 610
1300-1200 BCEK 89
1400-1300 BCEK 98
Radiocarbon ca. 1400 BCEF 10B7
700-600 BCEH 16
Destruction 732; life, say, 750 BCEH 35
ca. 850 BCEH 54
ca. 900 BCEH 73
ca. 1000 BCEH 92
ca. 1100 BCE H 111
Known datesSample
location
Lab
No.
(MGD)
List of samples
� Samples were drilled from the sections under cover, to prevent
exposure to sunlight.
� Sample preparation was carried out under subdued light.
� The sediment was sieved 74-125 µm. Carbonates were dissolved,
organic matter oxidized, the fines washed, and the quartz fraction
was extracted by magnetic separation. It was then etched with
concentrated HF to remove any feldspars and remove the α-affected
rim.
� Dose rate (d) was evaluated in the field and by chemical analyses.
The concentrations of U, Th and K (the radioactive elements) in the
sediments were measured by ICP-MS or ICP-AES. The gamma and
cosmic dose rates were measured in the field using aluminum oxide
dosimeters or calculated from the radioactive elements and burial
depth.
� The OSL signal was measured and De was determined using the
SAR protocol.
� Up to 42 aliquots were measured from each sample, to obtain dose
distribution.
Laboratory work
Preheat plateau:
Preheat is used to isolate the stable
signal. The De should not be
affected by the selected preheat
over a range of temperatures.
Quality assurance
Recycling Ratio:
One dose point is repeated at the end of
the measurements. It should fall within
5% of the first point. This shows that
the corrections to signal sensitivity
changes have worked.
280
Beta (s x 100)
Lx/T
x
MGD-3
De=163.3±4.5 s
Sample MGD-11, from EB wall, J4
N=18
De = 7.87±0.08 Gy
Age = 4530±180 years (before 2010)
(archaeological age: 3000 BC)
4% error on the age
OSL measurement results:
The OSL signal decays rapidly,
indicating the dominance of a
fast (easily bleached) component.
Sample MGD-12,
from stable floor in L2
N=41
De = 5.8±0.3 Gy
Age = 5100±310 years (before 2010)
Archaeological age: 8th C BC
Using statistics, 20/41
De = 4.76±0.08 Gy
Age = 4150±150 years (before 2010)
Second look – full of collapsed brick
material
Scatter in De results:
• The signal of the Megiddo samples is dominated by the
fast OSL component and is bright, reducing measurement
uncertainties.
• Quality assurance results are very satisfactory, indicating
that the SAR protocol is appropriate and that a thermally
stable signal is measured.
• The main uncertainty is from scatter between individual
De measurements (aliquots).
Solution:
• Measurements of small aliquots and the use of
component statistics allows to isolate the better-bleached
grain population.
• Single grain measurements could improve on this.
Uncertainties in dose rate estimates:
• Has dose rate been constant over time?
• Change in burial depth (affects the cosmic dose).
• Change in moisture contents (probably minor).
• Diagenesis (minor).
• Non-homogenous gamma field (30 cm radius) due to the juxtaposition of
limestone with low radioactivity and soil with high radioactivity.
• Only in-situ measurements can estimate the gamma dose so that these
inhomogeneities are taken into account.
• Aluminum oxides: new type of dosimeters which are light sensitive and can
detect very low doses (short time in the field).
• Dosimeters brought by Geoff Duller and Helen Roberts from
Aberystwyth University.
• Placed in copper tubes in each of the sampling points at a depth of
~30 cm.
• Left there for ~ 6 weeks.
• Removed and measured at the GSI.
• Entails very special calibration of the beta source.
gamma & cosmic
300
400
500
600
700
800
900
1000
300 400 500 600 700 800 900 1000
Al oxides
chemistry+depth 11
5
• A systematic offset for 10 of 12 aluminum oxide dosimeters,
where they give values which are ~ 90 microgray lower than the
chemistry values..
• Could be from source calibration, travel dosimenters or other
factors.
• The gamma+cosmic dose is ~ 50% of the total dose rate. A
change in 10% in this component would change the age by 5%.
Comparison between the dosimeters and dose rate
calculated from chemistry & depth
•Sample MGD-11 taken from soil between
stones. This sediment was also given for
chemistry.
•There are very large differences in dose
rates between stone and sediment: the
limestone is low, the sediment (with clays)
is high.
•Gamma dose rate calculated only from the
sediment would be too high, giving a too-
young age.
•In this case the Al oxide measurements
were used, giving an OSL age of 4530±180
years.
•No clear reason for sample MGD-5.
22304240±150M 8/M615
7702780±130ca. 1000M 414
20304040±130ca. 850L 313
20704080±150800-732L 212
25204530±180ca. 3000J 411
12303240±150Destruction ca. 1130 K 610
19103920±1201300-1200K 89
11903200±1601400-1300K 98
31105120±170Radiocarbon ca. 1400 F 10B7
5602570±150700-600H 16
16603670±140Destruction 732; life 750H 35
18603870±130ca. 850H 54
13903400±120ca. 900H 73
7402750±80ca. 1000H 92
10703080±100ca. 1100H 111
OSL ages
BCE
OSL ages
Before 2010
‘known dates’
BCE
Sample
location
Lab No.
(MGD)
OSL age results
Megiddo ages
2000
2500
3000
3500
4000
4500
5000
5500
2000 2500 3000 3500 4000 4500 5000 5500
Calendar (archaeological) age
OSL age
Only 8 of 15 samples fall
within ±10 % of the
archaeological age (green
lines).
The deviation is mostly
towards older OSL ages.
Could be the result of
incorporation of older
material, such as unfired
bricks.
Comparison between OSL and archaeological ages
123032401130K6
770, 7402780, 2750ca. 1000M4, H9
13903400ca. 900H7
2030, 18604040, 3870ca. 850L3, H5
1660, 20703670, 4080ca. 732H3, L2
OSL ages
BCE
OSL ages
Before 2010
‘known dates’
BCE
Levels:
Destruction layers:
MGD-1
H-11
3080±100
(1100) BC
MGD-3
H-7
3400±120
(900 BC)
MGD-2
H-9
2750±80
(1000 BC)
MGD-5
H-3
3670±140
(750 BC)
AREA H
MGD-4
H-5
3870±130
(850 BC)
AREA K
MGD-8
K-9
3200±160
(1300-1400 BC)
MGD-10
K-6
3240±150
(1130 BC)
MGD-9
K-8
3920±120
(1200-1300 BC)
• There is no particular depositional environment which gives a
better agreement between the OSL and archaeological ages.
• Some destruction layers are better behaved than others.
• Water lain sediments could be OK.
• A large component of the sediments in Megiddo was brought in
from outside, or it has been sitting around for a long time and
constantly reused.
• Need to beware of collapsed brick beds.
Summary
The way forward:
• Sample during excavation season when all sections are clean.
• Careful observations of sedimentary environments.
• Sample from courtyards, where dust collects directly or swept out
from the houses.
• Measure single grains, to isolate the best bleached grain
population.
• Perhaps be able to identify sources of recycled material.
• Measure dose rates by several methods.
• Pottery?