Quantifying the net rotation of the Earth's lithosphere remains an unsolved problem in geodynamics and plate tectonic reconstructions. Net rotation is the movement of the entire lithosphere as a solid body with respect to the Earth's mantle. It is therefore one component of the motion recorded with respect to the Earth's magnetic dipole, preserved in the palaeomagnetism of rocks. However, three other components of motion are also preserved in the palaeomagnetism (Jurdy, 1981): movement of individual plates (continental drift); rigid-body rotation of the lithosphere and mantle with respect to the Earth's spin axis (true polar wander; Duncan & Richards, 1991;Steinberger & Torsvik, 2008); and movement of the Earth's magnetic dipole relative to the Earth's spin axis. The contribution of these processes to palaeomagnetic data cannot be separated. In order to study any one of these components, for example when building absolute plate motion models, assumptions for the others must be made in order to reconstruct the movement of the lithosphere through geological history (Coltice et al., 2017;Tetley et al., 2019).The lithospheric net rotation (LNR) estimates require a stable reference point in the mantle. Mantle plumes and hotspots are generally used, as these are considered to have been roughly stable for the last few tens of millions of years (