Volume 21 / No. 8 / 1989

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Volume 21 / No. 8 / 1989 Volume 21 No. 8. October 1989 TheJournalof Gemmology 63 GEMMOLOGICAL ASSOCIATION OF GREAT BRITAIN OFFICERS AND COUNCIL President: *Sir Frank Claringbull, Ph.D., EInst.E, FGS Vice-President: R. K. Mitchell, FGA Chairman: *D. J. Callaghan, FGA Vice-Chairman: *N. W Deeks, FGA Honorary Treasurer: *N. B. Israel, FGA Members elected to Council: *A. J. Allnutt, M.Sc, J. W Harris, B.Sc, *J. B. Nelson, Ph.D., Ph.D., FGA M.Sc, Ph.D. FRMS, ElnstE, FGA C. R. Burch, B.Sc, J. A. W Hodgkinson, FGA W Nowak, CEng., FGS D. Inkersole, FGA ER.Ae.S., FGA *C. R. Cavey, FGA B. Jackson, FGA M. J. O'Donoghue, E J. E. Daly, B.Sc, *E. A. Jobbins, B.Sc, C.Eng., MA, FGS, FGA FGA FIMM, FGA R. J. Peace, FGA *A. E. Farn, FGA *G. H. Jones, B.Sc, Ph.D., *EG. Read, CEng., A. J. French, FGA FGA MIEE, MIERE, FGA G. Green, FGA D. G. Kent, FGA *K. Scarratt, FGA *R. R. Harding, B.Sc, D. M. Larcher, FGA E. Stern, FGA D.Phil, FGA A. D. Morgan, FIBF, FGA *C. H. Winter, FGA ^Members of the Executive Committee Branch Chairmen: Midlands Branch: J. Leek, FGA North-West Branch: R. Perrett, FGA Examiners: A. J. Allnutt, M.Sc, Ph.D., FGA D. G. Kent, FGA E. M. Bruton, FGA P Sadler, B.Sc, FGS, FGA A. E. Farn, FGA K. Scarratt, FGA R. R. Harding, B.Sc, D.Phil., FGA E. Stern, FGA E. A. Jobbins, B.Sc, C.Eng., FIMM, FGA M. Virkkunen, M.Phil., FGA G. H. Jones, B.Sc, Ph.D., FGA C.Woodward, B.Sc, FGA Editor: E. A. Jobbins, B.Sc, C.Eng., FIMM, FGA Editorial Assistant: Mary A. Burland Curator: C. R. Cavey, FGA Secretary: Jonathan P. Brown, FGA, Barrister Saint Dunstan's House, Carey Lane, London EC2V 8AB (By Goldsmith's Hall) Telephone: 01-726 4374 The Journal of Gemmology VOLUME 21 NUMBER EIGHT OCTOBER 1989 Cover Picture Irridescent glass with botryoidal form, exhibiting spectral colours due to interference on thin layers, f See 'Iridescent natural glass from Mexico', p.488. ) ISSN: 0022-1252 466 J. Gemm., 1989,21,8 F.G.A Three initials that could change your career The Gemmological recognised and respected Association of Great by companies and Britain has been actively organisations throughout involved in the very the gemmological world. beginning of Gemmology Indeed, each year many of as an independent them invest in the future by science. sponsoring their own Today, the Association candidates. takes pride in its The Gemmological international reputation as Association's course has a learned society been specially compiled into dedicated to the a series of teaching modules promotion of that are both readable and gemmological education lavishly illustrated. and the spread of Together they provide a gemmological knowledge. comprehensive step-by-step The Association's guide to the fascinating coveted Fellowship is a world of gemmology. And an mark of excellence only Gemrndk^icalAsscxiation opportunity to earn the bestowed upon individuals coveted initials FGA— who successfully undertake of Great Britain Fellow of the Gemmological the association's written Association of Great Britain. and practical examinations covering all aspects of To find out more complete the coupon below and gemmology as a science. we will immediately forward the Association's Not surprisingly, this prestigious diploma is prospectus giving full details of this unique course. Please complete and return to: Gemmological Association Training Scheme, Saint Dunstan's House, Carey Lane, London EC2V8AB. Tel: 01-7264374 n Name Position Company_ Address . Telephone. J. Gemm., 1989,21,8 467 Star sapphire from Kenya N. R. Barot*, A. Flamini**, G. Graziani*** and E.J. Gübelin**** *Ruby Centre (Kenya) Ltd, Fedha Tower, 2nd Floor, Miundi Mbingu St., PO Box 47928, Nairobi, Kenya **1st Teoria Struttura Elettronica CNR, Via Salaria km 29.500, PO Box 10, 00016 Monterotondo Stazione, Italy ***Dip. Scienze della Terra, Università degli Studi di Roma 'La Sapienza', P. le A. Moro 5, 00185 Roma, Italy ****Benzeholzstrasse 11, 6045 Meggen, Lucerne, Switzerland Abstract well-shaped crystals. In the sapphire lots there are Various cabochon-cut star sapphire samples from the some pieces of dark brown to black obsidian, North-West of Kenya were examined to determine all brown zircon and translucent to opaque dark green the inclusions which may contribute to cause the epidote. asterism effect. Optical observations, electron microprobe and X-ray diffraction analyses were carried out. The inclusions Location and geology recognized were: cloudy areas, acicular inclusions, Corundum appears in Kenya as patches in meta- 'silk', tube-like inclusions, transparent crystals, 'feathers' morphic rocks (gneisses) which are believed to and healed fractures. The acicular inclusions responsiblehav e been desilicated by a dunite (Parkinson, for the asterism are separated into micro-striae 1947). The same applies to the corundum of the and needle-like inclusions. nepheline-syenite dyke-like bodies in the valleys Genetic growth considerations of these star sapphires (Joubert, 1966). are deduced. Usually the crystals are of dirty-brown colour and sometimes fractured. Introduction In the North-Western region, corundum is The world's main sources of star sapphire, up to found in Tertiary volcanic olivine basalts or in this time, have been Burma and Sri Lanka. Kenya secondary deposits (Bridges, 1982). is now entering the list and becoming the third The actual, geologically important, deposit is country and indeed the first country in Africa to not identified. Sapphires are being picked up from produce and supply star sapphire. the large desert type sandy area in the North­ Kenya and Tanzania, in addition to the many western region of Kenya. This is in the Turkana unusual gemstones, have been known to produce district of the Northern Rift Valley Province, and corundum in all possible colours and qualities lies on the West side of Lake Turkana (formerly from numerous occurrences. However, none of the Lake Rudolph) (Figure 1). sources ever supplied rough which can produce This region is part of the Mozambique orogenic star stones in commercial quantity. belt extending southwards to Malagasy and Several years ago, a small lot of blue sapphires Mozambique and northwards through the Sudan appeared on the Kenyan gem market of which and Ethiopia (Bridges, 1982). some samples produced a star. However, the source The area is in the middle of the Y-shape of the was never made known and similar or larger lots fault systems, and stretches from the turn off the never appeared on the gem market. main Lodwar road to the Sudan. This is a second­ Now the source has been relocated, and sapphire ary road (dirt road) leading to the Ethiopian border rough has started appearing on the local market through Murangering and Lokitaung villages (see since mid 1987. Hence the rough is available in map). commercially acceptable quality and quantity. Sapphires are mined from the top soil of desert Some other rough with a fair amount of trans­ type plains (Quaternary sediments) caused by the parency can be faceted to produce nice blue to erosion and peneplanation of hills, namely bluish-green gems. Lower grade rough can be used Pelekesh (1794m) and Mornerith (1438m). The to produce cabochons (without a star) and even primary source of the star sapphires and their beads. original occurrence is yet to be investigated. Most of the rough samples are slightly worn However, areas from which sapphires are probably crystals with frosted surfaces and a very low collected are shown by the dashed area in the map percentage (1-5%) of either completely rounded or (Figure 1). © Copyright the Gemmological Association ISSN: 0022-1252 468 J. Gemm., 1989,21,8 gemmologist an ETHIOPIA metal disc wit gemstones o ETHIOPIA gemstone is illuminated for both the spectroscop ETHIOPIA ETHIOPIA ETHIOPIA ETHIOPIA ETHIOPIETHIOPIAA ETHIOPIA ETHIOPIA ETHIOPIA ETHIOPIETHIOPIAA ETHIOPIA ETHIOPIETHIOPIAA ETHIOPIA ETHIOPIA ETHIOPIA ETHIOPIA ETHIOPIETHIOPIA A ETHIOPIETHIOPIA A ETHIOPIA Fig. 1. This map shows the location of the star sapphires in the North-western region of Kenya. The mining area, dashed area in the map, is located in the Turkana district of the Northern Rift Valley Province on the west side of Lake Turkana. Rough sapphire: its grading and cutting star which displays six equally narrow rays, with The examined samples are in the form of ten characteristic angles intersecting at 60°; of equal cabochon-cut star sapphires (total weight: 1.253 length and brightness, extending fully in each gm). They cover various shades of body colour viz. specimen. A weak star not extending fully is blue, brownish-blue, greenish-blue, greenish- displayed by the cabochons nos. 3, 5, 6, and 8. yellow, and blackish-brown. This different behaviour is ascribable to devi­ They range in size from 3.6 x 3.8 x 1.7 mm to ations from the crystallographic arrangement of 5.9 x 5.3 x 3.0 mm; the weight of each specimen the elongated systems of inclusions in the body of was measured to be a minimum 0.060 to maximum the host sapphire, intergrown with the basal plane 0.782 gm. and aligned parallel to the prisms of first or second 'Silk' occurs in all the cabochons, but in eight of order. them it traverses the whole of the host sapphire and causes 6- and 12-rayed asterism. Nevertheless, Gemmological investigation in samples 9 and 10, the 'silk' appears densely The cabochon sapphires were subjected to woven, causing only 'silky-spots'. standard gemmological tests, and the results are The samples nos. 1, 2, 4, and 7 present a perfect discussed below. J. Gemm., 1989, 21,8 469 Visual appearance and absorption spectra segregated into five categories: The samples range in clarity and are classified as 1) Cloudy areas sapphires from medium transparent (diaphane) to 2) Acicular inclusions opaque.
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