| Volume 21, Number 01, January - March 2001 |
(Follow this link for abstracts of past issues) TOURMALINE AND AQUAMARINE DEPOSITS FROM BRAZIL J. César-Mendes1, H.
Jort-Evangelista1, R. Wegner2 ABSTRACT JADE: OCCURRENCE AND METASOMATIC ORIGIN G.E.
Harlow1, S.S. Sorensen2 ABSTRACT BRAZILIAN GEM PROVINCES C.P.
Pinto1, A,C. Pedrosa-Soares.2 ABSTRACT
EMERALD DEPOSITS - A REVIEW D.
Schwarz1, G. Giuliani 2 ABSTRACT The juxtaposition of Cr/V and Be, in nature, requires exceptional geological and geochemical conditions. The principal mechanisms responsible for emerald crystallization are fluid-rock interactions, which allow the combination of the incompatible elements. Formation of most emerald deposits in the world are associated with granitic intrusions. Hydrothermal processes related to granitic-pegmatitic systems lead to the crystallization of emeralds in mafic-ultramafic or in (meta-)sedimentary rocks. In general, the mafic-ultramafic hosts of emeralds are schistose rocks of varying composition (e.g. in most African and Brazilian deposits, as well as in the Ural Mountains.) In Eidsvoll (Norway) and Emmaville-Torrington (Australia), emeralds are hosted by (meta-)sedimentary rocks. A second group of emerald deposits is not directly related to granitic intrusions. In these, tectonic phenomena (thrust faults and shear zones) are the controlling factors for the formation of emerald mineralisations. Circulation of fluids along these regional tectonic structures resulted in emerald formation in volcano-sedimentary series, e.g. Santa Terezinha (Brazil), Habachtal (Austria), or in oceanic suture zones such as the Swat Valley (Pakistan), and the Panjsher Valley (Afghanistan). The famous deposits in the Colombian Cordillera Oriental have a unique formation through the thermochemical reduction of evaporitic sulphate brines, with the participation of organic matter from the surrounding black shales in the reactions. GEM TOURMALINE CHEMISTRY AND PARAGENESIS W.B. Simmons, K.L. Webber, A.U. Falster, J.W. Nizamoff ABSTRACT All the tourmalines are dominantly elbaite or liddicoatite. Darker coloured varieties contain a minor schorl component. Y-site chemistry strongly correlates with colour and appears to be strongly influenced by the chemical characteristics of the pegmatites in which the tourmaline occurs. X-site vacancies of all tourmalines are less than 0.3 apfu. Fe and to a lesser extent Mn, Ti and Cu are the principal chromophores. Pink and green tourmalines from Transbaikalia are essentially elbaites, however, yellow zones within these crystals show a substantial liddicoatite component, coupled with elevated Ti and Mn contents. Tourmalines from the Antandrokomby pegmatite, Madagascar, are members of the schorl-elbaite series with significant Mg and Ca contents. Even though the pegmatite occurs in a metadolomite, tourmaline Ca content is less than that of tourmaline from the classic Fianarantsoa and Anjanabonoina regions of Madagascar, where the tourmaline is liddicoatite and the pegmatites occur in pelitic country rocks. Tourmalines from both Madagascar locations have the lowest Y-site Al content. Tourmalines from San Diego County, California, and Newry, Maine, USA, are very similar chemically and belong to the schorl-elbaite series, with lighter coloured, gemmy varieties approaching end-member elbaite. Paraiba tourmaline from Brazil is elbaitic in composition but contains significant Cu, which imparts a vivid blue colour. ORIGIN OF GEM CORUNDUMS FROM BASALTIC FIELDS F.L.
Sutherland1, D. Schwatz2 ABSTRACT Magmatic sapphires contain diverse, but characteristic, mineral inclusions. Co-existing zircon yields uranium-lead isotope formation ages and presumably also the sapphire crystallisation ages. These ages are usually close to host basaltic eruption ages. Rare sapphire-bearing felspathic xenoliths suggest a coarse syenitic origin. Crystallisation of magmatic sapphires has been variously ascribed to mid-crustal carbonatitic-silicic hybrid melt interactions or to lower crust/mantle felsic melts. Low volume melting of hydrous mantle to produce such syenitic melts was proposed from zircon/basalt dating within Australian sapphire fields. Growth from buffered high pressure syenitic melts undergoing fugitive alkali carbonatitic volatile loss is supported by recent studies in Scotland. Metamorphic sapphire and ruby suites incorporate mineral inclusions and trace element contents that indicate a range of metamorphic source assemblages. Rare corundum-bearing metamorphic xenoliths suggest contact metamorphic, alumino- silicate regional metamorphic and lower crust granulitic sources. In eastern Australia, trace element contents in corundums sampled from a 3000km long basaltic tract differentiate corundums into several separate magmatic and metamorphic fields. A few corundum suites show intermediate geochemical characteristics between those of ‘magmatic’ and ‘metamorphic’ origin and their precise origin requires further study. THE GEOLOGY OF AUSTRALIAN OPAL DEPOSITS I.J. Townsend ABSTRACT Host rocks contained a variety of voids formed by the weathering process; leaching of carbonate from boulders, nodules, fossils, along with existing cracks, hollow centres of ironstone nodules and horizontal seams. Most opaline silica deposited is common opal (or potch). It does not show a play of colour. Opal also fills pore space in sand size sediments cementing the grains together forming deposits known as matrix or opalised sandstone. Opal is often associated with lineaments or faults which break up the rock providing waterways for the movement of ground water. These have been found useful in locating opal at Lightning Ridge in New South Wales (NSW) and pursued in other states. In addition, opal has been found associated with ancient palaeochannels in Queensland, and Lightning Ridge (NSW) often adjacent to these channels, which provide water channels. Variations in the types of opal depend on a number of factors. Firstly the climate provides alternating wet and dry periods, creating a rising or importantly falling water table which concentrates silica in solution. The silica itself is formed by deep weathering of Cretaceous clay sediments producing both silica and kaolin. Silica spheres are deposited in a regular array in voids from a receding water table forming precious opal in a variety of host materials. VIEWPOINT W.Wm.Hanneman ABSTRACT
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DISPERSION
MEASUREMENT WITH THE GEMMOLOGISTS REFRACTOMETER
Part 1
D. B. Hoover
Missouri, USA
T. Linton
Wellington Point, Queensland, Australia
ABSTRACT
In the past, the practicing
gemmologist has had little interest in measuring the dispersion of gemstones. In part,
this is because the property, dispersion, has little apparent use for the gemmologist.
This lack of interest is evidenced by the scarcity of published papers discussing such
measurements.
This paper reviews the history of the critical angle refractometer; which may be used to
measure dispersion; the use of dispersion by gemmologists; and develops theory from which
the critical angle refractometer may be calibrated to measure dispersion. Errors in prior
published papers are explained. In Part 2, to follow, the practical aspects and problems
of such measurements will be addressed.
NovaDiamond
TM
COLOUR ENHANCED YELLOW AND YELLOW-GREEN DIAMONDS
Amanda S. Barnard
Melbourne, Victoria
ABSTRACT
Presented is a summary of
properties and a discussion of mechanism of treatment of the NovaDiamondTM colour enhanced yellow and yellow-green diamonds.
Also included is an independent spectral examination of a specimen supplied courtesy of
Novatek. It is intended that this paper should provide the reader with information
necessary to assist in the effective identification of NovaDiamondsTM, and other treated yellow-green diamonds.
RARE
AUSTRALIAN GEMSTONES
MOONSTONE
A rare Queensland gemstone
Hylda Bracewell
Brisbane, Queensland
ABSTRACT
While the feldspars are chemically
and structurally diverse minerals that are mined extensively throughout the world, any
colourless variety that displays a bluish schiller is commonly termed moonstone, and is
comparatively rare. Queensland gemmologists, members of the jewellery trade, and
fossickers, are fortunate to have a small, yet prolific deposit of one of these rare gem
feldspars readily available to them at Moonstone Hill, north of Hughenden in North
Queensland. This paper describes this deposit and provides the gemmological properties and
features of the moonstone that can be fossicked from this deposit.
RUSSIAN
COLOURLESS SYNTHETIC DIAMOND
Now available in the market
Joe C. C. Yuan
New York
ABSTRACT
Colourless to near colourless synthetic diamonds, manufactured in Russia in the 'split
sphere' apparatus, are now available on the US market. These type lla diamonds have a
cubo-octahedral habit. When cut and polished they yield diamonds with colours mostly in
the G-K range. The diamonds have identifying metallic inclusions, are magnetic, display
ultraviolet luminescence that differs from that of natural diamonds, and yield a
cross-shaped pattern of strain birefringence. Members of the trade, who do not have access
to De Beers DiamondViewTM will
have to rely on the observed presence of metallic inclusions, magnetism, and these
diamonds un-natural fluorescence and phosphorescence, for identifying these synthetic
diamonds.
AUSTRALIA'S GEMSTONE RESOURCES & THEIR MARKETS
Grahame Brown
Editor of The Australian Gemmologist
ABSTRACT
In this review Australias major gemstone resources were specified. Australias
commercial production of diamond, opal, cultured South Sea pearls, chrysoprase, sapphire,
and nephrite were detailed. Additional detail was provided about man-made gem materials
presently being produced in Australia, and the support services available to
Australias gemstone and related jewellery manufacturing industries. This review was
presented to the APEC Gems & Jewellery Trade Y Technology Seminar that was held in
Beijing during May 2000.