Hostname: page-component-74656f9884-npj9w Total loading time: 0 Render date: 2026-11-07T18:03:04.596Z Has data issue: false hasContentIssue false

Radiocarbon Dating of Legacy Music Instrument Collections: Example of Traditional Indian Vina from the Musée De La Musique, Paris

Published online by Cambridge University Press:  22 July 2019

M G Durier
Affiliation:
Centre de Recherche sur la Conservation (CRC), MNHN, CNRS USR 3224, Ministère de la Culture, 36 Rue Geoffroy Saint-Hilaire, 75005, Paris, France LSCE, UMR 8212 CEA, CNRS, UVSQ, Université Paris-Saclay, F-91198 Gif-sur-YvetteFrance
P Bruguière
Affiliation:
Musée de la musique, Équipe Conservation Recherche, CRC, MNHN, CNRS USR 3224, Ministère de la Culture, 36 Rue Geoffroy Saint-Hilaire, 75005, Paris, France
C Hatté*
Affiliation:
LSCE, UMR 8212 CEA, CNRS, UVSQ, Université Paris-Saclay, F-91198 Gif-sur-YvetteFrance
S Vaiedelich
Affiliation:
Laboratoire de Recherche et de Restauration, Musée de la Musique, Cité de la Musique, 221 Avenue Jean Jaurès, 75019 Paris, France
C Gauthier
Affiliation:
LSCE, UMR 8212 CEA, CNRS, UVSQ, Université Paris-Saclay, F-91198 Gif-sur-YvetteFrance
F Thil
Affiliation:
LSCE, UMR 8212 CEA, CNRS, UVSQ, Université Paris-Saclay, F-91198 Gif-sur-YvetteFrance
N Tisnérat-Laborde
Affiliation:
LSCE, UMR 8212 CEA, CNRS, UVSQ, Université Paris-Saclay, F-91198 Gif-sur-YvetteFrance
*
*Corresponding author. Email: Christine.Hatte@lsce.ipsl.fr.
Rights & Permissions [Opens in a new window]

Abstract

Although radiocarbon (14C) dating is commonly used for archeological music instruments, little research has been conducted on modern instruments (16th–19th centuries). New technology, based on the Mini Carbon Dating System (MICADAS), enables some of the recurring challenges (e.g. sampling size) to be circumvented and paves the way for a new field of investigation. We here address the Indian instrumentarium, about which very little is known. We investigate the making and the restoration phases of two vina, a kinnari vina (E.1444), and a rudra vina or bin (E.997.24.1). By comparing 14C measurements made on several samplings of elements of the instruments with museological information, we were able to specify a unique calibrated interval of ages [1666 AD–1690 AD] for the kinnari vina, with a restoration phase [1678 AD–1766 AD] for the upper nut. The bin is likely attributed to the [1650 AD–1683 AD] interval.

Information

Type
Conference Paper
Copyright
© 2019 by the Arizona Board of Regents on behalf of the University of Arizona 
Figure 0

Figure 1 Indian vina from the museum collections and sampling locations: (a) kinnari vina E.1444, (b) close up of sampling in a crack from kinnari vina E.1444, (c) schematic view of the kinnari vina E.1444 and location of the 8 samples, (d) bin or rudra vina E.997.24.1 and sample locations. Pictures by Claude Germain (a, d) and Stéphane Vaiedelich (b) © Musée de la musique-Philharmonie de Paris.

Figure 1

Table 1 List of samples from kinnari vina and rudra vina (refer to Figure 1 for locations).

Figure 2

Table 2 Conventional, calibrated and modeled 14C ages obtained for the kinnari vina E.1444. Statistical results of Bayesian modeling are shown in the last four columns: for all vina pieces first and for the original pieces of the vina thereafter. Individual agreement (Aind) and combined agreement (Acomb) are provided. Resulting modeling intervals are provided under the main part of the table.

Figure 3

Figure 2 Calibrated 14C ages of the kinnari vina E.1444. The upper probability distribution diagram, underlined in blue corresponds to the Bayesian modeling of the combination of the vina’s original parts. The probability distribution diagram of the restored piece (upper nut) is shown in the last line.

Figure 4

Table 3 Conventional, calibrated, and modeled 14C ages obtained for the bin E.997.24.1. Statistical results of Bayesian modeling are shown in the last two columns. Individual agreement (Aind) and combined agreement (Acomb) are provided. Resulting modeling intervals are provided under the main part of the table.

Figure 5

Figure 3 Calibrated 14C ages for the two gaseous micro-samples from the bin or rudra vina E.997.24.1. The upper probability distribution diagram, underlined in blue, corresponds to the Bayesian modeling obtained by combination of bin 14C results. (Please see electronic version for color figures.)