E. Gnos et M. Perrin, FORMATION AND EVOLUTION OF THE MASIRAH OPHIOLITE CONSTRAINED BY PALEOMAGNETIC STUDY OF VOLCANIC-ROCKS, Tectonophysics, 253(1-2), 1996, pp. 53-64
The extrusive rocks of the lower ophiolitic nappe of Masirah Island (O
man) were paleomagnetically studied. Four mean directions of magnetiza
tion were isolated, one at low temperature, the others at high tempera
ture, The low-temperature component, found in most samples, correspond
s to a recent viscous and/or chemical remagnetization. ?he high-temper
ature component, found at three sites in the Centre area, is interpret
ed as a possible primary magnetization acquired during extrusion or, m
ore probably, as an early remagnetization related to subsequent hydrot
hermal alteration and indicates formation of the Masirah ophiolite aro
und a paleolatitude of 40 degrees S, close to the present position of
the West Somali basin, A second high-temperature component, found in t
hree other sample sites in the Hakl and in the Thumi areas, is probabl
y a chemical remagnetization related to the emplacement of the upper o
phiolite nappe in late Maastrichtian to Paleocene times, Finally a las
t high-temperature component, found only in the two sites from Naft ar
ea, could be a post-tectonic remagnetization acquired in Oligocene or
Miocene times or represents differential tilting of pillows and sedime
ntary blocks. The high-temperature components are usually fairly scatt
ered due to the very complex tectonic history of the area. Nevertheles
s, the relation between the defined paleopoles and the Indian polar wa
nder is unambiguous and the evolution of the Masirah ophiolite from fo
rmation up to the emplacement of the second ophiolitic nappe is clearl
y related to the northward movement of the Indian plate. This new pale
omagnetic study rules out the possibility of a common or related origi
n for the Masirah and the Semail ophiolites.