New data for the characterization of Milos obsidians | INSTITUT DE PHYSIQUE DU GLOBE DE PARIS

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  New data for the characterization of Milos obsidians

Type de publication:

Journal Article

Source:

Journal of Radioanalytical and Nuclear Chemistry, Volume 268, Ticket 2, p.371-386 (2006)

ISBN:

0236-5731

Mots-clés:

GLASSES; ARTIFACTS; SIO2-NAALO2; ELEMENTS; NETWORK; MELTS

Résumé:

Newly produced fission track (FT), instrumental neutron activation analysis (INAA) and micro-Raman spectrometry data have been used to characterize the classical source areas of the Milos obsidians better and to check the provenance of obsidian artefacts. The Bombarda-Adhamas and Demenegaki obsidians yielded indistinguishable FT ages 1.57 +/- 0.12 and 1.60 +/- 0.06 My, respectively, in agreement with previous FT data. By INAA analyses it was possible to discriminate between the three obsidian sources on Milos: Bombarda-Adhamas, Demenegaki and A. Ioannes. Raman spectroscopy has been found to be a valuable technique to gain a chemico-structural characterization of a given obsidian population in terms of dissolved water content and microlite distribution/composition.

Notes:

J. Radioanal. Nucl. Chem.ISI Document Delivery No.: 049OCTimes Cited: 1Cited Reference Count: 45Cited References:*NAT I SCI TECHN, 1979, 1633A SRM NAT I SCI*NBS, 1981, 278 SRM NBSACQUAFREDDA P, 1999, J ARCHAEOL SCI, V26, P315ARIAS C, 1986, CIENCIA CULTURA, V38, P285ARIAS C, 1986, SCI METHODOLOGIES AP, P151ASPINALL A, 1972, NATURE, V237, P333BELLOTGURLET L, 1999, RADIAT MEAS, V31, P639BIGAZZI G, 1986, J RADIOAN NUCL CH AR, V98, P353BIGAZZI G, 1986, RIV SCI PREIST, V36, P223BOWER NW, 1992, GEOSTANDARD NEWSLETT, V16, P27BURNHAM CW, 1994, REV MINERAL, V30, P123CARPENTER SB, 1984, NBS SPEC PUBL, V260, P92DEFARIA DLA, 1997, J RAMAN SPECTROSC, V28, P873DIMURO A, IN PRESS GEOCHIM COSDIPAOLA GM, 1974, B VOLCANOL, V38, P944DURRANI SA, 1971, NATURE, V233, P242FYTIKAS M, 1976, TECTONOPHYSICS, V31, P29GLASCOCK MD, 2003, MEAS SCI TECHNOL, V14, P1516GOFFER Z, 1980, ARCHAEOLOGICAL CHEMJAFFREZIC H, 1976, TALANTA, V23, P497KELLER J, 1990, ACT AT EUR RAV LOUV, P57KILIKOGLOU V, 1997, J RADIOANAL NUCL CH, V216, P87KINGMA KJ, 1994, AM MINERAL, V79, P269LINNEN RL, 2002, GEOCHIM COSMOCHIM AC, V66, P3292LONG DA, 1977, RAMAN SPECTROSCOPYMCMILLAN P, 1984, AM MINERAL, V69, P645MCMILLAN PF, 1986, AM MINERAL, V71, P772MICHEL A, 2003, GEOSTANDARD NEWSLETT, V27, P163MYSEN BO, 1988, STRUCTURE PROPERTIESNEUVILLE DR, 1996, GEOCHIM COSMOCHIM AC, V60, P1727ODDONE M, 2000, J RADIOANAL NUCL CH, V243, P673OKUNO M, 1996, EUR J MINERAL, V8, P1257PERNICKA E, 1996, P 29 INT S ARCH ANK, P515POIDEVIN JL, 1998, BAR INT SERIES, V738, P105PRINCIPE C, 2003, SAAVA 2003 MIL C CTRRENFREW C, 1973, NEOLITHIC GREECERINALDI M, 2003, B VOLCANOL, V65, P282RUST AC, 2004, GEOLOGY, V32, P349SEIFERT F, 1982, AM MINERAL, V67, P696SHELFORD P, 1982, ISLAND POLITY ARCHAE, P182STORZER D, 1969, EPSL, V5, P463STORZER D, 1973, CR ACAD SCI D NAT, V276, P137SYLVER LA, 1990, CONTRIB MINERAL PETR, V104, P142YEGINGIL Z, 2002, TERRA NOVA, V14, P169ZOTOV N, 1989, PHYS CHEM MINER, V16, P774