The thermal structure of the lithosphere from shear wave velocities

• Published in: Earth and planetary science letters Vol. 244; no. 1; pp. 285 - 301
• Main Authors: Priestley, Keith, M cKenzie, Dan
• Format: Journal Article
• Language: English
• Published: Elsevier B.V 15.04.2006
• Subjects: Diamonds; Lithosphere; Mantle; mantle temperature; Melts; Position (location); Rayleigh wave tomography; Seismic phenomena; Sound waves; Surface waves; mantle temperature; lithosphere; diamonds; Rayleigh wave tomography
• ISSN: 0012-821X; 1385-013X
• DOI: 10.1016/j.epsl.2006.01.008

The low shear wave velocities V s observed beneath spreading ridges and in the low velocity zone beneath plates are commonly attributed to the presence of melt. But geochemical observations suggest that the amount of melt present in those parts of the mantle that are melting is about 0.1%, which is too small to produce a major decrease in V s. Furthermore laboratory measurements of V s at seismic frequencies, 1–10 − 2 Hz, show that V s is more strongly affected by temperature than by the presence of a few percentage of melt. It is, however, not straightforward to use laboratory experiments to relate V s to the temperature T because the grain size of most laboratory experiments is 100–1000 times smaller than that of the mantle. We combine thermal models of the Pacific lithosphere and pressure and temperature estimates from mantle nodules brought up by kimberlites with three dimensional models of V s from surface wave tomography to obtain an empirical relation for V s( P, T), where P is the pressure. This expression is then used to convert regional variations of V s as a function of depth to lithospheric thickness. The accuracy of the resulting maps is tested by comparison with the location of diamond-bearing kimberlites, which are in most places restricted to regions where the lower part of the lithosphere is in the diamond stability field.