
INFRARED REFLEXION SPECTROMETRY OF MINERALS
AND GEMS
|
MIJAIL
OSTROUMOV ([email protected])
BERNARD LASNIER
SERGE LEFRANT
EMMANUEL FRITSCH
Introduction.
The
infrared absorption, reflexion or emission spectrum of a single mineral is a characteristic of its kind. That is why the
spectra can give the structural formula without neccessity to have the chemical analysis
data (Lazarev, 1966).
The
qualitative analysis of a unknown substance (e.g. mineral) can be in general, without
knowing the mechanism details of interacci?n between infrared energy and the sample. By utilizing this method, one also
acomplishes this semi quantitative analysis of the minerals and their mixture (Marfunin,
1974, 1975).
The characteristic of each spectrum is determined by vibrations of the atomic
groups of the crystalline structure of minerals. There
exist complicated relations between interatomic distances, the angle and the force of the
relative masses of atoms (Niquist, and Kagel,
1971). All the infrared spectra
characteristics of minerals are related with the chemical composition and the crystalline
structure of the compounds (Farmer, 1974). We
first of all would like to make note the practical use of the infrared reflexion
spectrometry that is very important tool for mineralogists and gemologists.
This
study was undertaken to compensate the absence of research about the infrared reflexion
spectrometry of minerals, particularly gemological materials and gems. Indeed, the research of international
literature permits only to find a few studies which spectrometric investigation was used
for a few minerals and gems.
An analogical study was undertaken a few years ago to present new possibilities of
the Raman spectrometry that is another non-destructive method with a great future in
mineralogy and gemology. A catalog of the
Raman spectra of gemological gems was proposed by Maestrati (1989), then by Pinet et al.
(1992). A more complete Raman spectra catalog
of minerals is in the press in France, result of a collective work (Beny and Lasnier,
2001).
The
infrared reflexion spectrometry completes very well the Raman spectrometry, in particular
to demonstrate the presence of some cations, like (OH) that are present in many minerals
and the less easily detectable in Raman spectrometry (Plyusnina, 1977; Povernnikh, 1978). It is also a non-destructive and can be used to
determiner the nature of minerals.
It
is evident of the urgent necessity to create infrared reflexion spectra of minerals and
gems catalog.
Analytical results.
The
infrared range is subdivided into three ranges:
near infrared (PIR: 13333-4000 cm -1 or 0.8-2.5 �m);
mid infrared (IRM: 4000-400 cm -1 or 2.5-25 �m);
far infrared (IRL: 400-10 cm -1 or 25-1000 �m).
The region of the near infrared is favorable for the identification of the typical bands
of some chemical groups or ions such as Fe 2+ (0.8-1 mm), H2O (1.4;1.9 mm), OH (2.2; 2.7
mm),
and CO3 2 - (1.9; 2.0; 2. 17; 2.3 mm).
Thus these absorption bands use for the qualitative or semi quantitative analysis of these
groups and also to determine some elements.
In the mid infrared range, the reflexion or absorption bands are normally due to the
various minerals atomic groups.
The mid infrared spectra of the mineral always bring significant information about the
functional groups that constitute it.
The majority of the mineral characteristic bands meet in the mid region of the infrared
spectrum. So, research on minerals and gems is numerous in this region.
In particular, a catalog of infrared reflexion spectrum of minerals and some gems are now
in the Internet (Ostroumov et al., 2000) because the infrared reflexion spectrometry
presents many comparative advantages compared with infrared absorption spectrometry of the
minerals (Ostroumov et al., 1995).
The far infrared region is a zone where the fundamental bands of basic frequencies of
various atomic groups are observed. At the present, this region is not yet well studied
for minerals.
Experimental
methods
The observation of minerals by infrared spectrometry can be done into two general ways: by
absorption or reflection.
The mineral frequency vibrations are generally measured by infrared absorption
spectrometry.
But the absorption spectrometry has a series of limitations: firstly, it is a destructive
method.
During the preperation, it sometimes influences the crystal structure of the minerals and
its elemental cell structure (e.g. opal, phyllosilicates).
The spectrum obtained from powder is an average spectrum and one loses part of diagnostic
information on the structure of anisotropic minerals.
This method does not guarantee the cleanliness of the preparation, which is why in the
spectrum one can observe false bands.
The minerals often have very broad absorption bands. There are also many problems with the
dimension of crystals; the degree of pulverization, the quantity of minerals and the
presence of inert compound (the potassium bromide used for the preparation of samples).
In general, the preparation of samples for the absorption spectrometry requires very much
time, expenses and materials.
Thus, we prefer the reflexion infrared spectrometry. Currently the infrared measurements
of the reflexion spectra of minerals are likely to extend since the appearance of stable
and practical spectrophotometers with the complementary reflexion equipment.
The
advantages of the infrared reflexion spectrometry are numerous. It is a non-destructive
investigation method that can be applied:
For
minerals with natural surface (the crystallographic faces, planes of cleavage, non uniform
surfaces),
For cut and mounted gems, it can constitute a test of identification for these stones.
The usable surface of samples can be variable, from a few cm2 to a few mm2 .
The acquisition of a spectrum is a one-minute command. This method is much easier to
implement than the absorption spectrometry.
The reflexion spectra show many narrow bands; sometimes the number of the reflexion bands
is more significant than the number of the absorption bands.
Thus, the infrared reflexion spectra always bring more information on the functional
groups that constitute them.
The reflexion and absorption bands seldom coincide. The law Kramers-Kroning has explained
the displacement of the absorption maximum.
In general, this displacement depends of the position and configuration of the reflexion
band. For example, carbonates, the maximum intense reflection (nearly 1400 cm-1) are
placed in a more shorter wavelengths, but the weak maximum nearly 800 cm-1 is placed in
more longer wavelengths.
By
this, the direction of displacement depends of the intensity absorption:
For the intense vibrations : l abs > l ref.,
For the weak vibrations: l abs < l ref.
Mid
infrared reflexion spectra relate directly with the structure of the mineral matter, that
is to say, with the constant physics of the same (crystal lattice, and in particular, the
index of refraction).
For that reason, this spectrum has the characteristics that allow identifying the mineral
species.
To determine the natural or synthetic origin of gem materials, it is necessary to analyze
them in the near and far infrared ranges, even in the visible region. Each mineral,
natural or synthetic gem presents a quite particular infrared reflexion spectrum, which
allows a fast identification of the mineral species.
For
the exact determination, it is necessary to take into account the effect of the
orientation of mineral crystals and rough stones.
For most of these minerals, the orientation modifies the relative intensities of the bands
of the spectrum. But the general character of the spectrum does not change, that is to
say, that this parameter does not intervene in the identification.
Sometimes one observes the displacement of some bands according to the orientation of the
crystals. The displacement of the characteristic bands is typical for the solid solutions
(isomorphous series). Therefore, we have the spectra that were registered for the crystals
with a well-known orientation.
Sampling.
The creation of an infrared reflexion spectra catalog it necessitates the need for
obtaining spectra on samples with the greatest possible of purity.
Keeping in mind these imperatives, we have selected nearly 200 mineral species of enough
dimensions to be guided, carved and refined.
These samples of the greatest purity were identified by the traditional gemological and
mineralogical methods.
Each " standard " sample has been analyzed quantitatively with the electron
probe microanalyser CAMECA SX 51 at the Saint Petersburg Geological Institute (Russia).
The results of these analysis have been deposited at the Mineralogical Department
(University of Michoacan, Mexico) and at the Mineralogical and Gemological Laboratory
(University of Nantes, France).
These " standards " will also be in the disposition of the researchers who could
request them to compare their own mineralogical and gemological samples.
The infrared reflection spectra were obtained with the specific equipment that we have in
our disposition for the spectrometric groups installed at:
1. Mineralogical Laboratory of the Saint Petersburg Mining Institute (Russia).
2. Mineralogical and Gemological Laboratory of the Mainz University (Germany)
3. Crystal Physics Laboratory of the Institute of Materials, of the Nantes University
(France).
Instruments used.
We have used various spectrometric apparatuses:
- Spectrometer IRS-29 (Russia)
- Spectrometer UR-20 (Germany)
- Spectrometer Perkin-Elmer FTIR (Germanny)
- Spectrometer Bruker IFS-28 (France)
We had the possibility of using these various apparatus to compare our results and to
benefit from their complementarities.
The mineralogical and gemological samples have been guided and mounted on the universal
accessory of reflexion with retro-mirror (Harrick Scientific Corporation).
The samples needed one, two or three different orientations according to their crystal
system.
The calibration of the spectrometer has been systematically verified at the beginning of
each register by putting on the apparatus a pure natural quartz crystal (the deposit
Cholodnya, Ural Polar, KOMI Republic, Russia) according to two orientations: parallel and
perpendicular to the axis of order 3.
The same spectra were obtained for the verification in various laboratories and with
different spectrometric equipment.
The spectra have been recorded on diskettes and are available at the Mineralogical
Laboratory (University of Michoacan, Mexico) and at the Mineralogical and Gemological
Laboratory (University of Nantes, France).
In the above-mentioned it will be proposed the program of the automatic identification
that this based on this spectrometry database on the medium infrared region of reflection.
Model of card of the catalog.
As for the other catalogs of the infrared spectra already published we have proposed a
double-sided card wich contains the following information:
Front
side: information on materials taken as standard (natural, source, etc.) and experimental
conditions
Back side: the spectrum records has a scale standardized allowing an immediate easy
comparison for the spectrum registered under the similar conditions.
Infrared reflexion spectra
of minerals of various cristallochemical classes
This work is the first systematic intent of the reflexion infrared catalog of minerals and
gems. Approximately 220 species minerals, natural and artificial gems have been
investigated in this work.
We have used at least the same presentation of the spectrometric data that of the Raman
catalog (Pinet et al., 1992).
We also propose two modes of presentation: one by mineralogical group and the other by
alphabetical order.
We initially give a general spectrometric characteristics of the crystallochemical
classes. Then, the catalog itself is presented in the form of cards classified by
mineralogical groups.
These cards contain: the apparatus and the experimental conditions, the orientation of the
sample taken as a standard, the obtained spectra and the position of the principal lines
in cm-1 .
The scale of intensity have been eliminated since it depends on the operative conditions.
The relative intensities of the peaks are without doubt more important.
Conclusion.
The infrared reflexion spectrometry in the far region supplements a well spectrometry in
the mid infrared zone for the various crystallochemical classes of minerals.
With Raman spectrometry, this non-destructive method makes it possible to determine the
mineral species and varieties.
In our opinion, the infrared reflexion spectrometry in the different regions will be able
to contribute to the resolution of the current problems of mineralogy, such as for
example, the determination of close minerals by the chemical composition, the
characteristics of zonation, optical orientation, inclusions and pleochroism, etc
(Ostroumov, 1991; Ostroumov et al., 2000).
On one hand, this technique can lead to non-destructive identification of the gems and the
art objects, with separation between the natural and synthetic crystals, with the
identification of the treatment and the impregnation of the various substances of
gemological materials, etc.
Using this method one can identify remotely, near or far, the rough surface or cut
minerals, of gems and rocks in cosmic geology, astronomy, planetology, volcanology.
Beny C., Lasnier B. (2001). Catalogue des spectres Raman des mineraux. Edition BRGM, France.
Farmer V.C. (1974). The infared spectra of minerals. Mineralogical Society. London.
Lazarev A.N. (1966). Vibrational spectra and structure of silicates. Edition Science.
Moscow.
Maestrati R. (1989). Contribution a l'edification du
catalogue Raman des gemmes. Diplome d'Universite de Gemmologie. Universite de Nantes.
Marfunin A.S.
(1974). Introduction a la physique des mineraux. Edition Nedra, Moscou.
Marfunin A.S. (1975). Spectroscopie, luminescence et centres radiogeniques dans les
mineraux. Edition Nedra, Moscou.
Niquist R.P., and R.O. Kagel (1971). Infared spectra of inorganic compounds (3800-45
cm-1). Academic Press, New York.
Ostroumov M. (1991). Methode de determination du degre dordre-desordre dans la structure
cristalline des feldspaths alcalins par leur spectres infarouges de reflexion.
Memoires de la Societe Mineralogique de l'URSS, vol. 120,
No.5, 94-99.
Ostroumov M.,
Lasnier B., Lefrant S. (1995). Infrared reflection spectrometry of gem materials. Analusis
23, 39-45.
Ostroumov M., Lasnier B., Lefrant S., Fritsch E. (2000). Infrared reflection spectrometry
of minerals and gemological materials. Internet: http://mineral.virtualave.net
Pinet M., Smith D., et Lasnier B. (1992). Utilite de la
microsonde Raman pour l'identification non destructive des gemmes. Revue de Gemmologie
A.F.G. No. hors serie.
Plyusnina I.I. (1977). Spectres infrarouges des mineraux. Edition
Universite de Moscou.
Povarennykh A.S. (1978). The use of infared spectra for the determination of minerals.
American Mineralogist, vol. 63, 956-959.
LISTES DES SPECTRES INFRAROUGES DE REFLECTION PAR FAMILLE MINERALOGIQUE.
| COMPOSITIONS
SYNTHETIQUES 1. Opal 2. Emeraude Hydrothermal 3. Emeraude Chatham 4. Emeraude Lechleitner 5. Emeraude Gilson 6. Alexandrite 7. Spinelle rouge 8. Spinelle bleu 9. Spinelle incolor 10. Fianite 11. Fabulite 12. Corindon + V 13. Corindon + Cr 14. Corindon + Ti 15. Corindon incolor 16. Y.A.G 17. G.G.G 18. Quartz 19. Turquoise 20. Nd-verre 21. Verre Bleu 22. Verre jaune |
I. ELEMENTS NATIFS. 1. Diamant |
II. SULFURES
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III. HALOGENURES
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IV. COMPOSITIONS DE OXYGENE |
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| IV.1. OXYDES 1. Rubi 2. Saphire 3. Chrysoberyl 4. Alexandrite 5. Cristal de roche 6. Amethyste 7. Citrine 8. Quartz rose 9. Chrysoprase 10. Chalcedony 11. Perelivte 12. Spinelle 13. Rutile 14. Cassiterite 15. Hematite 16. Opal |
IV.2. SELS OXYGENES. |
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| IV.2.1. CARBONATES 1. Calcite 2. Rhodochrosite 3. Aragonite 4. Cerusite 5. Dolomite 6. Magnesite 7. Siderite 8. Malachite 9. Azurite IV.2.2. BORATES |
IV.2.3. SULFATES 1. Gypse 2. Anhydrite 3. Aryte 4. Celestine 5. Alunite IV.2.4. CHROMATES IV.2.5. MOLYBDATES |
IV.2.6. PHOSPHATES ET VANADATES 1. Apatite 2. Variscite 3. Beryllonite 4. Turquoise 5. Pyromorphite 6. Lazulite 7. Vanadinite |
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IV.2.7. SILICATES |
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| IV.2.7.1.
NESOSILICATES 1. Phenacite 2. Olivine (chrysolite) 3. Grenat 3.1. Almandin 3.2. Pyrope 3.3. Spessartite 3.4. Grossulaire vert 3.5. Grossulaire tsavorite 3.6. Andradite melanite 3.7. Andradite demantoide 3.8. Uvarovite 4. Zircon (brun, bleu) 5. Haut zircon 6. Chondrodite 7. Andalousite 8. Disthene 9. Sillimanite 10. Sphene 11. Staurotide 12. Topaz 13. Dumortierite 14. Kornerupine IV.2.7.2. SOROSILICATES |
IV.2.7.3. CYCLOSILICATES 1. Benitoite 2. Beryl - Emeraude - Aigue-marine - Heliodore 3. Beryl vert 4. Cordierite 5. Axinite 6. Tourmaline - Rubellite - Olenite - Dravite - Indigolite - Verdelite - Shorlite 7. Eudialyte 8. Sugilite 9. Sogdianite |
IV.2.7.5. PHYLLOSILICATES 1. Muscovite 2. Phlogopite 3. Biotite 4. Lepidolite 5. Chlorite 6. Serpentine 7. Antigorite 8. Talc |
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| IV.2.7.4. INOSILICATES 1. Augite 2. Hedenbergite 3. Diopside vert 4. Cr-diopside 5. V-diopside 6. Spodumene - Kunzite - Hiddenite 7. Aegirine 8. Jadeite 9. Tremolite 10. Actinolite 11. Hornblende 12. Nephrite 13. Rhodonite 14. Charoite 15. Bustamite |
IV.2.7.6. TECTOSILICATES 1. Sanidine 2. Orthose 3. Microcline 4. Amazonite bleu 5. Amazonite vert 6. Albite 7. Oligoclase 8. Belomorite (Albite-Oligoclase) 9. Labrador 10. Bytownite 11. Moonstone 12. Adulaire 13. Scapolite 14. Glaucolite 15. Nepheline 16. Sodalite 17. Lazurite 18. Cancrinite |
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