The gnomonic projection is from the centre of a sphere to a plane tangent to the sphere (Fig 1 below). The sphere and the plane touch at the tangent point. Great circles transform to straight lines via the gnomonic projection. Since
meridians (lines of longitude) and the
equator are great circles, they are always shown as straight lines on a gnomonic map. Since the projection is from the centre of the sphere, a gnomonic map can represent less than half of the area of the sphere. Distortion of the scale of the map increases from the centre (tangent point) to the periphery. • If the tangent point is one of the
poles then the meridians are radial and equally spaced (Fig 2 below). The equator cannot be shown as it is at
infinity in all directions. Other
parallels (lines of latitude) are depicted as concentric
circles. • If the tangent point is on the equator then the meridians are parallel but not equally spaced (Fig 3 below). The equator is a straight line perpendicular to the meridians. Other parallels are depicted as
hyperbolae. • If the tangent point is not on a pole or the equator, then the meridians are radially outward straight lines from a pole, but not equally spaced (Fig 4 below). The equator is a straight line that is perpendicular to only one meridian, indicating that the projection is not
conformal. Other parallels are depicted as
conic sections. As with all
azimuthal projections, angles from the tangent point are preserved. The map distance from that point is a function of the
true distance , given by r(d) = R\,\tan \frac d R where is the radius of the Earth. The radial scale is r'(d) = \frac{1}{\cos^2\frac d R} and the
transverse scale \frac{1}{\cos\frac d R} so the transverse scale increases outwardly, and the radial scale even more. ==Use==