Orthographic projection in cartography has been used since antiquity. Like the stereographic projection and gnomonic projection, orthographic projection is a perspective projection in which the sphere is projected onto a tangent plane or secant plane. The point of perspective for the orthographic projection is at infinite distance. It depicts a hemisphere of the globe as it appears from outer space, where the horizon is a great circle. The shapes and areas are distorted, particularly near the edges.
History The orthographic projection has been known since antiquity, with its cartographic uses being well documented. Hipparchus used the projection in the 2nd century BC to determine the places of star-rise and star-set. In about 14 BC, Roman engineer Marcus Vitruvius Pollio used the projection to construct sundials and to compute sun positions. Vitruvius also seems to have devised the term orthographic (from the Greek orthos (= “straight”) and graphē (= “drawing”)) for the projection. However, the name analemma, which also meant a sundial showing latitude and longitude, was the common name until François d'Aguilon of Antwerp promoted its present name in 1613. The earliest surviving maps on the projection appear as crude woodcut drawings of terrestrial globes of 1509 (anonymous), 1533 and 1551 (Johannes Schöner), and 1524 and 1551 (Apian). A highly-refined map, designed by Renaissance polymath Albrecht Dürer and executed by Johannes Stabius, appeared in 1515. Photographs of the Earth and other planets from spacecraft have inspired renewed interest in the orthographic projection in astronomy and planetary science.
Mathematics The formulas for the spherical orthographic projection are derived using trigonometry. They are written in terms of longitude (λ) and latitude (φ) on the sphere. Define the radius of the sphere R and the center point (and origin) of the projection (λ0, φ0). The equations for the orthographic projection onto the (x, y) tangent plane reduce to the following:
x = R cos φ sin ( λ − λ 0 ) y = R ( cos φ 0 sin φ − sin φ 0 cos φ cos ( λ − λ 0 ) ) {\displaystyle {\begin{aligned}x&=R\,\cos \varphi \sin \left(\lambda -\lambda _{0}\right)\\y&=R{\big (}\cos \varphi _{0}\sin \varphi -\sin \varphi _{0}\cos \varphi \cos \left(\lambda -\lambda _{0}\right){\big )}\end{aligned}}}
Latitudes beyond the range of the map should be clipped by calculating the angular distance c from the center of the orthographic projection. This ensures that points on the opposite hemisphere are not plotted:
cos c = sin φ 0 sin φ + cos φ 0 cos φ cos ( λ − λ 0 ) . {\displaystyle \cos c=\sin \varphi _{0}\sin \varphi +\cos \varphi _{0}\cos \varphi \cos \left(\lambda -\lambda _{0}\right)\,.}
The point should be clipped from the map if cos(c) is negative. That is, all points that are included in the mapping satisfy:
− π 2 < c < π 2 . {\displaystyle -{\frac {\pi }{2}}<c<{\frac {\pi }{2}}.}
The inverse formulas are given by:
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