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Original article
Discrimination between the authentic and fake Egyptian funerary
figurines “Ushabtis” via laser-induced breakdown spectroscopy
Amal Khedr a , Hamada Sadek b , Olodia Aied Nassef a , Mahmoud Abdelhamid a ,
Mohamed Abdel Harith a,∗
a
b
National Institute of Laser Enhanced Science, Cairo University, Cairo, Egypt
Faculty of Archaeology, Conservation Department, Fayoum University, Al Fayoum, Egypt
a r t i c l e
i n f o
Article history:
Received 7 February 2019
Accepted 15 May 2019
Available online xxx
Keywords:
Ancient Egypt
Ushabtis
Genuine and fake
LIBS
SEM-EDX
a b s t r a c t
The potential of laser-induced breakdown spectroscopy (LIBS) in differentiating between types of genuine and fake Ushabtis was studied. For this goal, the present study was initiated by a comprehensive
spectrochemical analytical study of four archeological Ushabti statues, dated back to the late Ptolemaic
period (332–330 B.C), which have been excavated south of El-Shawaf pyramid in Saqqara, Giza, Egypt.
This study was followed by performing the same investigations on several imitated Ushabtis, which were
purchased from the touristic marketplace in the region of the pyramids. For the archeological samples,
optimization of LIBS experimental parameters in terms of temporal detection conditions along with laser
wavelengths and their corresponding ablation rate was performed. The spectrochemical analyses of the
genuine archaeological samples were carried out both superficially and stratigraphically. Main surface
elements such as Ca, Na, Al, Si, Cu, Fe, and Mn were detected while large amounts of Ca and Sr represent
their bulk elements. The LIBS results were validated by results obtained by SEM-EDX technique, which
provided complementary information such as surface morphological images and quantitative composition of the samples’ constituents. Under the optimum experimental conditions, LIBS spectral emission
of the imitated samples was acquired and compared to those for true archeological ones for the sake
of possible discrimination between them. Successful utilization of LIBS in examining the authenticity of
suspect Ushabtis has been accomplished and presented. This study may suggest the need for archeologists to be equipped with portable LIBS systems in the excavation sites or museums, which facilitate the
immediate discrimination process when LIBS data of genuine samples are initially available.
© 2019 Elsevier Masson SAS. All rights reserved.
1. Introduction
In ancient Egyptian royal tombs, numerous funerary figurines
are typically found. Such figurines, called Ushabtis or Shabtis, are
supposed to act as servants or minions for the deceased person
[1]. The ancient Egyptians believed that Ushabtis would answer
for their master and perform the daily life routine chores for
the deceased, which gods required from him in the afterlife. One
Ushabti has to serve for one day of the year; hence, usually, around
360 Ushabtis are found in the tomb. As Shabtis represent the most
numerous of all ancient Egyptian antiquities to survive, they also
represent the most commonly displayed ancient Egyptian collections in museums of cultural heritage worldwide.
∗ Corresponding author. Tel.:/Fax: +202 35675335.
E-mail address: mharithm@niles.edu.eg (M.A. Harith).
Colors play a substantial role in ancient Egyptian art and belief.
Blue, for example, refer to life symbolized by the river Nile and
heaven. On the other hand, the green could exemplify vegetation’s
cycle, and consequently, revival and regeneration [2,3]. Certain
sacredness is added to any figurine by the application of meaningful
colors to it. Hence, most Shabtis were blue or green. One of the most
available coloring agents for Shabtis, dating back to the beginning of
the dynastic era, was copper compounds. Around the time of Thahtmus III (1479–1425 BC) in the new kingdom period, other colorants
such as lead, cobalt, antimony, tin, iron, and manganese oxides were
used for obtaining different colors such as white, green, purple,
yellow, and black respectively [3,4]. An archaeological Ushabti usually is made of faience coated with a shiny colored or transparent
thin glaze layer. Faience is produced in ancient Egypt by mixing up
to 99% of high-grade silica, produced by crushing quartz pebbles,
with alkali soda (Na2 O) 0.3 to 5%, and lime 1 to 5% at high temperature [5–9]. The shaping of the figurine is then performed via a
process of melting and casting. In these old times, the production
https://doi.org/10.1016/j.culher.2019.05.006
1296-2074/© 2019 Elsevier Masson SAS. All rights reserved.
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technology of the Egyptian faience has changed over time and from
place to place in the country. Such changes are relevant to faience’s
composition itself and the adopted production techniques [10]. For
example, by the beginning of the first millennium BC, natron has
been used instead of soda as a flux that helps in lowering the materials fusion temperature [11]. The lack of knowledge of the Ushabti
origin and the absence of inscriptions makes it difficult to conclude
whether or not a particular figurine is a copy or an original item.
However, careful analysis of the materials used in manufacturing
such Ushabtis can be decisive in this matter.
The knowledge of the elemental composition of the surface and
the core of the archaeological samples could help in constructing
scenarios for the production technology utilized by the craftsmen
and the row materials resources at such old eras. With such precious and unique objects, nondestructive analytical techniques are
the most appropriate. Many works have been reported using Raman
spectroscopy, Fourier transforms infrared spectroscopy (FTIR), and
X-ray fluorescence (XRF) [12–16]. Though these techniques are
nondestructive and, commercially available for several years ago,
the first two provide only superficial information about the molecular, and not the elemental, composition, and cannot go beneath
the surface like LIBS. On the other hand, though XRF can provide
limited elemental stratigraphic details on the sample, it is unable
in detecting elements lighter than magnesium.
During the past two decades, laser-induced breakdown
spectroscopy (LIBS) has emerged as a fast, simple and quasinondestructive spectrochemical analytical technique at a reasonable cost in the field of archaeology [17,18]. In LIBS, high power
laser pulses are focused onto the surface of the target material. Concentrating such a tremendous amount of energy on a tiny volume
causes the evaporation of few nanograms to micrograms of the target material. With continuous absorption of energy from the laser
pulse, the atoms in the vapor are excited then ionized and at the
end, a collection of ions and swirling electrons, at tremendously
high temperature (6000–60,000 K), will compose the so-called the
plasma plume. The laser-induced plasma cools down and gets rid of
the absorbed energy in the form of electromagnetic radiation emission. The radiation emitted in the optical range (UV, Vis, and IR)
is collected, dispersed spectroscopically, and the obtained spectra
are displayed on a suitable PC for further processing and analysis.
The LIBS spectra provide qualitative information about the elemental composition of the target material, where the identified
spectral lines represent the spectral fingerprint of the elements
existing in the plasma plume and consequently in the target material, in case of stoichiometric ablation. Quantitatively, the intensity
of the elements spectral lines is proportional to the concentration
of such elements in the target material, taking into consideration
the matrix effect and the self-absorption. LIBS does not need sample
preparation, where the sample is analyzed as is without dissolution,
digestion or any other preparation procedures. On the other hand,
LIBS is now available as commercial portable or mobile systems
that can be used in excavation sites or museums for archaeological
samples analysis.
Since the laser parameters significantly affect the ablation process, plume and plasma characteristics, and more importantly the
analytical performance of LIBS, the goal of the present paper was
to:
• find out the optimum detection conditions for a good LIBS spectroscopic practice;
Table 1
List of experimental parameters used to produce the same irradiance.
Laser wavelength (nm)
Pulse energy (mJ)
The lens focal length (cm)
Spatial filter
Irradiance (W/cm2 )
UV – 355
Green – 532
IR – 1064
25
65
225
10
10
20
With
With
Without
7.64 × 1011
Fig. 1. The archeological Ushabti samples, designated as S1–S4.
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• investigate the effect of laser wavelengths systematically on the
investigated Ushabtis to obtain a good insight on their characterizing surface and bulk elements under fixed laser irradiance;
• validate LIBS results with the SEM-EDX qualitative and quantitative analyses results;
• examine the authenticity of the Ushabtis by comparing the LIBS
spectra of the fake Ushabtis samples with that of the original ones
under the same adopted experimental conditions.
2. Experimental setup
The LIBS experimental setup used in the present work has been
explained in detail elsewhere [19,20]. A Q-switched Nd: YAG laser
(Brilliant Eazy, Quantel, France) was used as an excitation source
operated at its three harmonics of 1064 nm, 532 nm, and 355 nm
and pulse duration of 5 ns. The pulse energy was measured by a
power meter (SCIENTECH model AC5001, USA) at a repetition rate
of 10 Hz. The LIBS spectral emission was produced by focusing the
laser beam orthogonally onto the investigated sample, which is
mounted on an X-Y-Z micrometric translation stage for fresh spot
irradiation. A 1.5 m-fiber optic cable of 600 m core diameter was
used to collect the emission from the laser-induced plasma to be fed
to an echelle spectrometer (Mechelle7500, Multichannel, Sweden),
coupled to an ICCD camera, DiCAM-PRO (PCO-computer optics,
Germany). The control of both acquisition time and delay with
respect to the onset of laser pulse was performed using the echelle
spectrometer software. LIBS spectra were acquired and stored for
analysis using LIBS++ software [21].
3
In order to carry out a comparison among samples’ characteristic spectral emission, the same irradiance for the three used laser
wavelengths (1064, 532, and 355 nm) is allowed to be incident on
all investigated samples. This has been performed by controlling
the experimental parameters of each laser wavelength, including
the laser pulse energy, laser beam diameter (via a spatial filter),
and the focusing conditions. Table 1 displays a list of the controlled
experimental parameters that were applied throughout the whole
measurements. For LIBS surface study, single laser pulse operational mode was allowed on fresh spots and accumulated for five
pulses while for bulk depth profiling, up to fifty successive pulses
were applied to the same spot of the sample and the spectrum was
saved after every single pulse.
Scanning Electron Microscope (Joel JSM-5410, Japan) in conjunction with Energy Dispersive X-Ray unit (OXFORD INCA Penta
FETx3, England) was used to investigate the Egyptian archeological
samples. SEM-EDX not only has been used to study the morphological structure but also utilized for the elemental analysis of the
samples; qualitatively and quantitatively, which was used for validation of the LIBS results.
3. Samples
Two sets of samples have been studied via LIBS. The first set
consists of four genuine archeological Ushabti samples dated back
to the Ptolemaic period collected from excavation sites in Saqqara,
Giza, Egypt and are designated as S1–S5 as shown in Fig. 1. The
second set, including six selected fake samples, was purchased from
the tourists’ marketplace in the region of the pyramids. Their shapes
and colors will be displayed in a following section. All the samples’
height ranges from approximately, 4 cm to 6 cm.
4. Results and discussion
This section is divided into two main sections starting with comprehensive study of the archeological Ushabtis samples through
an optimization of the LIBS experimental conditions in terms of
detection parameters and the applied wavelengths [The three
harmonics of Q-switched Nd-YAG laser; the fundamental IR wavelength ( = 1064 nm), the visible green ( = 532 nm) and the UV
wavelength ( = 355 nm)]. This includes the LIBS qualitative analysis of the samples by identifying atomic and ionic emission lines
in the spectral range between 200 nm and 900 nm and studying
the craters formed by the application of each of the three wavelengths. This was followed by validating LIBS qualitative results
by results obtained via SEM-EDX technique, which provide complementary images of the morphology of the investigated samples
and their quantitative compositions. The second section investigates fake Ushabtis, using LIBS under the same previously obtained
optimum experimental conditions.
4.1. Study of archeological Ushabtis
Fig. 2. Laser-induced breakdown spectroscopy (LIBS) spectra at the three applied
laser wavelengths representing common elements such as Ca, Al, Na, Si, Mg, and Fe
(top) and zoomed spectra parts in two wavelength ranges.
At the early stage of the interaction of a Q-switched nanosecondlaser pulse with a solid sample, an initial intense continuum is
promptly emitted close to the target surface, which corresponds
to the emission of blackbody radiation from the dense hot plasma.
As the plasma cools down and expands away from the target, the
process of recombination of electrons and ions eventually results
in the production of spectral lines emission. Temporally, the radiation processes usually tend to be dominated with the highly ionized
lines being emitted close to the target (superimposed on the continuum) and, then, the atomic lines appear at a later time of the plume
lifetime. Line emission prolongs for a few microseconds compared
to that of the continuum emission, which lasts for ns time range.
Please cite this article in press as: A. Khedr, et al., Discrimination between the authentic and fake Egyptian funerary figurines “Ushabtis”
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Therefore, the exploitation of time-resolved LIBS (TR-LIBS) allows
obtaining a temporal variation of LIBS signal which enables the
choice of best detection time for the best signal to background (S/B)
ratios.
Moreover, the analytical signal intensity of an element in
the plasma, which is related to the ejected mass of the investigated sample mainly depends on laser radiation parameters (laser
energy and focusing). Any random changes of these parameters can
strongly affect the analytical precision and accuracy. Additionally,
the ablation rate may vary as a result of the laser pulse-to-pulse
energy fluctuations and the relevant laser irradiance changes.
Therefore, the laser irradiance incident on the solid surface has been
adjusted and kept the same under the conditions listed in Table 1.
Various approaches to analytical signal correction and characterization improvement have been reviewed [22]. A straightforward
method is to consider the ratio of the intensity of the analytical
spectral line to the intensity of a spectral line of another component of the material instead of considering the absolute intensity of
the spectral line. Despite the change in measured values, the intensity ratio remained almost the same. Two types of internal standard
lines can be used [23]:
• non-sensitive spectral line of the major component of the sample;
• sensitive line of an element that is not initially present, but added
to the sample.
In the present work, the intensity of the spectral emission
lines was analyzed either as it was measured under the specified
experimental conditions (laser pulse energy, laser wavelength) or
normalized with respect to an internal reference selected among
those major elements characteristic of the matrix of the Ushabtis’
material, as it will be mentioned.
Based on the former reasoning, under the adopted experimental
setup, Ushabtis’ LIBS spectral emissions were stored as a function
of the time window (gate width G) during which the spectral emission is acquired, and its delay from the onset of the laser pulse
(delay time D) under the application of the three adopted laser
wavelengths. For data analysis and manipulation, the line ratio of
the spectral line of Cu I at 327.3 nm was normalized to that of Ca
I at 428.9 nm (one major component of the sample) and plotted
at different acquisition and delay time values for the three laser
wavelengths. Nearly the same values of the optimum gate width (G)
and delay time (D) at 1064 nm, 532 nm, and 355 nm were obtained.
Under the adopted experimental conditions, the values of (G) and
(D) were set at fixed values; 2500 ns and 1500 ns, respectively,
throughout all measurements.
4.1.1. LIBS signal dependence on laser wavelength
The laser wavelength is an essential factor for the initiation of
plasma, and its choice is dependent on its analytical capability.
Elemental composition of Ushabti samples has been investigated
via LIBS under the application of three different laser wavelengths,
namely, the fundamental wavelength at 1064 nm, Green at 532 nm
and UV at 355 nm. Under the adopted optimum D/G time values,
spectral emission was recorded for the four archeological samples.
For all samples, surface elements such as Ca, Al, Na, and Fe were
easily detected, and a noticeable amount of Mn and Cu could be
observed for black and greenish blue pigmented regions in the samples, respectively. Moreover, Si and Mg spectral lines indicate a high
content of such elements, which may be attributed to their presence
in the ancient ground quartz or quartz sand. One selected example
of a LIBS spectrum covering a wide spectral range from ∼ 240 nm
to 650 nm under the applied three laser wavelengths is shown in
Fig. 2 (top). Spectral lines of Mn and Cu characterizing respective
black and blue pigmented regions are displayed in the zoomed sections in the wavelength ranges from 474 nm to 484 nm in Fig. 2
Table 2
A list of LIBS detected elements and their corresponding spectral lines.
Elements
Detected LIBS spectral lines
Ca
315.88 nm, 317.93 nm, 428.3 nm, 393.3 nm,
396.8 nm
308 nm, 309 nm
263.12 nm, 269.25 nm, 273.96 nm, 274.67 nm,
275.57 nm, 426.04 nm, 427.17 nm
324.75 nm, 327.39 nm, 510.58 nm, 515.32 nm,
521.80 nm
288.15 nm
470.11 nm, 472.74 nm, 473.91 nm, 475.20 nm,
476.27 nm, 476.67 nm, 478.38 nm, 482.43 nm
588.99 nm, 589.60 nm
279.55 nm, 280.27 nm, 285.16 nm, 516.74 nm,
517.31 nm, 518.39 nm
Al
Fe
Cu
Si
Mn
Na
Mg
LIBS: laser-induced breakdown spectroscopy.
(middle) and from 510 nm to 524 nm in Fig. 2 (bottom). For clarification, detected elements and their corresponding spectral lines
are listed in Table 2. To avoid the inherent fluctuations of LIBS spectral data; the intensity was normalized to the line intensity of Ca
(I) at 428.3 nm.
The effect of the laser wavelength on the intensity of some
selected elemental lines was studied for samples S1, S2, S3 and
S4 as shown in Fig. 3. It is clear that, for all samples, the normalized intensity for most elements is the highest when the UV
laser at 355 nm was applied. This effect may be explained given
the higher absorption of the UV in such type of targets and that
among the applied wavelengths, the high photon energy of the
UV laser induces plasma characterized by higher emissions, less
continuum, short lifetime and narrow emission lines. Additionally,
the signal intensity of the spectral emission lines is highly dependent on the optical penetration depth, which is high for IR laser
compared to that for UV laser. In the case of a UV laser, energy is
rapidly absorbed in the surface of the samples, which has been previously reported for substrates of high evaporation threshold such
as ceramics, stones and faience [24].
For all used wavelengths, the appearance of elements such
as Ca, Si and Al in all samples with higher abundance supports
publications reporting that major components of Ushabti samples are quartz and limestone. The Ca is derived from lime (CaO),
which comprises between 1–5% of the composition of faience
and can be extracted from natural resources such as limestone
or chalk. It is assumed that the ancient Egyptians may have had
lime in archaeological faience as an impurity in the used sand or
it was added deliberately from chalk and/or limestone. On the
other hand, analysis of the Egyptian sand has revealed that it
contains 2–6% calcareous material [25]. These findings may also
explain the unconscious existence of the lime on old manufactured
faience.
Moreover, when applying each of the three laser wavelengths,
the spectral emission lines of silicon suggest that it represents a
major constituent of the samples. It might be claimed that the
source of silicon may be the quartz used in producing the bulk body
of the Ushabti. As the quartz bulk object is finished, it may disintegrate. Therefore, the addition of alkali, such as P, Na, and K as well as
the lime can help in binding the quartz grains together during the
drying phase, which gives the produced faience higher mechanical
strength [26,27]. We believe that sodium might have been obtained
in the form of Natron (Na2 O) mined by ancient Egyptians from Wadi
El-Natrun, a valley northwest of Egypt and the Elkab area, eighty
kilometers south of Luxor, Upper Egypt [4].
Bearing in mind that the ablation rate is dependent on many
factors that include the laser parameters, surface conditions, and
laser absorption in the plasma [28], the cross-sectional profiles of
the craters produced by the three applied laser wavelengths are
Please cite this article in press as: A. Khedr, et al., Discrimination between the authentic and fake Egyptian funerary figurines “Ushabtis”
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Fig. 3. Normalized laser-induced breakdown spectroscopy (LIBS) intensity using three laser wavelengths; 1064 nm, 532 nm, and 355 nm on the Ushabti samples S1 (a), S2
(b), S3 (c) and S4 (d).
Fig. 4. The cross-sectional profiles of the craters obtained by the laser wavelengths at 1064 nm (a), 532 nm (b), and 355 nm (c).
obtained, as shown in Fig. 4. It shows typical features of ns-laser
surface interactions, a central crater with specific area and depth,
which change with the applied laser wavelength. For the three used
laser wavelengths, a list of depths and diameters for the produced
crates are given in Table 3. It is observed that the crater’s profile
produced by the UV laser is more symmetrical compared to those
produced by both the visible and IR lasers whose craters seem to
be irregular. At fixed laser irradiance, the difference in the craters’
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Table 3
A list of the values of both depths and diameters for the produced craters when
applying the three mentioned laser wavelengths.
Wavelength (nm)
1064
532
355
Depth (m)
Diameter (m)
65
45
46
62
24
19
profile can be attributed to the laser wavelengths and their corresponding optical penetration depths.
4.1.2. Surface LIBS versus stratigraphic LIBS
This section focuses on both the identification of Ushabti’s surface pigments, which can be inferred from their color in addition
to their obtained LIBS spectroscopic data (their characteristic spectral lines), and the LIBS stratigraphic measurements which provide
information about the composition of the glaze layer and the below
substrate (bulk) of the Ushabti sample. A comparison of LIBS spectra for the surface and the bulk of Ushabti’s head for the sample
(S3) is illustrated in Fig. 5. It is observed that different elements
are enabling the differentiation between the surface and the bulk.
While surface spectral analysis shows emission lines of Mn that is
responsible for the black color of the head, the bulk is characterized
by the large amount of Sr, and Ca. It is most probable that Mn comes
from Pyrolusite (MnO2 ) while the presence of Sr and Ca presumably
exist via the use of lime (CaO) and Celestine (SrSO4 ) that may be
originated from the clay co-existing with the faience components
and the higher Sr signal on the surface could be due to contaminants
from the burial environment. The high intensity of Cu spectral lines
was observed for the surface layers of the rest of the samples which
is supposed to be responsible for the blue/green color. The source
of Cu is the Egyptian blue pigment (CaCuSi4 O10 ), which was made
by heating a mixture of sand, Natron (Na2 CO3 •10H2 O) and a copper compound such as malachite. This scenario was explained by
the fact that the addition of sodium (in Natron) as a fluxing agent,
reduces the melting point of pure silica from 1700 ◦ C to less than
1000 ◦ C and the inclusion of limestone (calcium oxide) works as a
stabilizer [27]. Ultimately, with the aid of the pigments’ apparent
color in addition to their characteristic atomic and ionic LIBS spectral emission, one can successfully discriminate among different
pigments and their composition.
By applying UV laser at 355 nm on the Ushabti samples S3 and
S4, the depth profiling of two key elements, which are responsible for the color pigments are investigated in Fig. 6. This figure
shows the depth profiling plot of spectral emission lines of Mn and
Cu which are responsible for the black and blue/green colors in
samples S3 and S4, respectively. It is clear that the intensity of the
spectral emission line, Mn I 475.2 nm decreases with increasing
the depth. In other words, as the laser beam goes more in-depth in
the sample, the black pigment on the surface is gradually decreasing until it is nearly removed after about ten micrometers. On the
other hand, inspection of depth profiling of the emission line Cu
I 324.7 nm for sample S4 revealed that the color layer is almost
removed after about five micrometers. This observation indicates
that monitoring the characterizing elements for each pigment
allows the estimation of its thickness, which seems to be different
for each surface pigmented layer.
4.1.3. SEM-EDX measurements
Scanning electron microscopy and energy dispersive X-ray
(SEM-EDX) were used to validate LIBS results and to provide quantitative analyses for a comprehensive overview of the archeological
samples. Due to its finely focused high energetic e-beam, SEM can
scan around even rough surfaces producing clear morphological
images [29,30]. Fig. 7 shows the local surface elements for samples S1 and S4 at a particular position with their corresponding
weight percentage relative to the predominant concentration of
the expected and characteristic pigment’s elements. The insets in
the same figure depict the micrographs of the same analyzed parts
of the sample surface. Most of the results agree with LIBS analysis,
especially in accordance with the major constituent elements such
as Si, Al, and Ca. It should be noted that the emission lines of K, P,
Cl, and S were out of the spectral range considered in the present
LIBS study, but EDX has observed them. The source of such effective alkali elements may be found as rock salts or from ashes. For
Fig. 5. Laser-induced breakdown spectroscopy (LIBS) spectra of the surface and the bulk for sample (S3) at two wavelength ranges.
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Fig. 6. The intensity change against the depth in microns for Mn I 475.2 nm for sample S3 and Cu I 324.7 nm for sample S4.
Fig. 7. The elements weight percentage of the energy dispersive X-ray (EDX) analysis for both samples S1 (left), and S4 (right). The inset is the scanning electron microscopy
(SEM) micrograph of the analyzed surface.
example, P generally comes from bone ashes while K is believed
to come from the ashes of halophytic plants particularly Salicornia which was the major source of alkali until the Ptolemaic period
onwards [31].
The existence of relatively high weight percent of Br in both
samples may be originated from the raw materials found in several
types of clay, especially, carbonate-rich clays. It is worth mentioning here that it is challenging to detect bromine, as well as most
halogens, via LIBS due to its high excitation energy. Bromine is
usually accumulated in the seawater and because of its high reactivity; it volatilizes into the atmosphere, and precipitate to the land
surface where it is usually combined with other elements at various firing temperature. Since Br sustains its original formation in
burned objects up to 800 ◦ C, it is considered as firing temperature
indicator [32]. Therefore, Ushabti figurines were assumed to be
burnt below 800 C.
To that end, complementary results have been offered by SEMEDX technique, which, along with LIBS, provide more reliable
information about the surface pigments and the bulk elemental
composition of the archeological Egyptian Ushabti.
4.2. Examining the fake Ushabtis
Given the obtained significant results for the identification of
the pigments of the archaeological Ushabtis, the capability of the
LIBS technique in examining fake faience Ushabtis collected from
tourist bazaar in the vicinity of the Giza pyramids have been investigated. Under the optimum experimental conditions mentioned
above, the obtained LIBS spectra for the investigated fake Ushabtis,
mainly, their blue pigmented regions, have been recorded. Such
spectral data has been compared to those previously acquired for
the genuine archeological samples. Fig. 8 illustrates an example of
the obtained LIBS spectral emission of the blue pigment for the fake
Ushabtis. When performing a comparison between such spectral
data and those previously acquired for the ancient Ushabtis, some
elements such as Mg and Si coexist in both. However, they exist
in lower content in the fake samples. Also, the appearance of the
different elemental composition such as Co and Ti represents significant differentiating elements. The presence of cobalt, known to
be currently used for obtaining blue color faience, may explain the
appearance of the stable colorant giving the blue color on the surface of these imitated samples. According to the required selected
colors, cobalt compounds are recently used to produce two colors; the light purple of the cobalt carbonate (CoCO3 ) and the black
of the cobalt oxide (CoO). By adding very low quantity (one-fourth
percent) in glaze results in satisfactorily colored blue. However, the
blue color produced by cobalt oxide can be changed by the addition
of other coloring oxides. Moreover, the presence of Fe may justify
the yellowish brown color observed in the fake samples [33]. Furthermore, the presence of several recognizable Ti spectral lines in
the fake samples is believed to be commonly present as titanium
dioxide or titania, which is used to opacify the glaze by creating
small crystals within it, so it is well suited for macro-crystalline
glazes [34]. Titania may accentuate the color on the clay body, and
its high viscosity may stiffen the glaze. Insoluble sources of titania
that currently used are rutile and ilmenite (iron titanate).
As a result, one can conclude that fake samples constituted
different elemental composition than those contained in the
archaeological Ushabtis when the same color pigment is examined
for both types of samples. The LIBS elemental differentiation capability performed successful examination of the authenticity of the
suspect samples, and an indication of their fake entity was revealed.
Please cite this article in press as: A. Khedr, et al., Discrimination between the authentic and fake Egyptian funerary figurines “Ushabtis”
via laser-induced breakdown spectroscopy, Journal of Cultural Heritage (2019), https://doi.org/10.1016/j.culher.2019.05.006
G Model
CULHER-3601; No. of Pages 9
8
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Fig. 8. Zoomed laser-induced breakdown spectroscopy (LIBS) spectral emission for the fake Ushabtis showing some common elements like those found in the ancient
samples, but with lower content, such as Mg and Si and some differentiating elements such as Co and Ti.
5. Conclusion
As a quasi-nondestructive and fast spectrochemical analytical
technique, LIBS was used to identify the elemental composition
of the surface and bulk of four Ushabti samples dating back to the
Ptolemaic period. Three laser wavelengths (355, 532, and 1064 nm)
were exploited to study the effect of the wavelength on the analytical results. It has been demonstrated that the UV laser wavelength
at 355 nm is the most appropriate as for the dynamic spectral range
and the signal to noise (S/N) ratio in the obtained LIBS spectra. The
superficial colors could be justified by the presence of specific element appearing in the relevant spectra such as Mn and black color,
as well as Cu and green color. Stratigraphic measurements depicted
the elemental structure of the glaze layer and the beneath bulk
layer too. The LIBS results were validated successfully via EDX-SEM
measurements, which also provided a complementary image that
may help infer the old techniques adopted by the Egyptians back
then. Moreover, to make use of these measurements, a comparison
between the LIBS spectra of the archaeological Ushabti and that
of two fake Ushabti samples was performed. An apparant discrepancy in the elemental composition was observed that indicates the
possibility of using LIBS in the authentication of the archaeological samples. Future work is planned for in situ measurements, in
museums and excavation sites using portable LIBS systems, to save
time and preserve the precious ancient samples.
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Please cite this article in press as: A. Khedr, et al., Discrimination between the authentic and fake Egyptian funerary figurines “Ushabtis”
via laser-induced breakdown spectroscopy, Journal of Cultural Heritage (2019), https://doi.org/10.1016/j.culher.2019.05.006