Abstract
Peridotite xenoliths from southern Texas consist of spinel lherzolite, harzburgite and minor dunite. Based on phase relations and temperature of equilibration, Knippa xenoliths come from the uppermost mantle, 40-70 km deep. Knippa xenoliths provide rare snapshots of upper mantle processes and compositions beneath south-central Laurentia. They preserve olivine a-axis fiber fabrics with a strong concentration of [100] and girdles of [010] and [001]. Assuming a lithospheric mantle having a horizontal flow direction parallel to fast directions, the mantle lithospheric fabric revealed by the xenoliths mostly explains the magnitude of observed shear-wave splitting observed along the southern margin of the Laurentian craton.
| Original language | English |
|---|---|
| Article number | L20312 |
| Pages (from-to) | L20312-1-L20312-5 |
| Number of pages | 5 |
| Journal | Geophysical Research Letters |
| Volume | 37 |
| Issue number | 20 |
| DOIs | |
| Publication status | Published - 1 Oct 2010 |
| Externally published | Yes |
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