The device consists of an arc of a circle, marked off in degrees, and a movable radial arm pivoted at the centre of the circle
The device consists of an arc of a circle, marked off in degrees, and a movable radial arm pivoted at the centre of the circle. A telescope, mounted rigidly to the framework, is lined up with the horizon. The radial arm, on which a mirror is mounted, is moved until the star is reflected into a half-silvered mirror in line with the telescope and appears, through the telescope, to coincide with the horizon. The angular distance of the star above the horizon is then read from the graduated arc of the sextant. Form this angle and the exact 160mm radius, designed to give maximum accuracy.