AbstractThe parameters of the Everest spheroid were obtained by George Everest by an arc-measuring method. In this method, sections of meridional arcs are measured by triangulation. Astronomical observations are made at selected points along the arc between the terminals. The differences between geodetic and astronomical latitudes are found out on a preliminary reference spheroid. The position of the arcs on the preliminary reference spheroid and the parameters of the spheroid are then changed to minimise the differences between geodetic and astronomic latitudes. Each separate arc gives a separate solution. Several arc measurements are then combined to give a common spheroid. Everest deduced the parameters of his spheroid from consideration of the arcs Punnae–Kalianpur and Greenwich–Formentera.