Mercator projection


In a Mercator Projection the point on the sphere (of radius R) with longitude L (positive East) and latitude λ (positive North) is mapped to the point in the plane with coordinatesMathworldPlanetmathPlanetmath x,y:

x=R⁢L
y=R⁢ln⁡(tan⁡(π4+λ2))

The Mercator projection satisfies two important properties: it is conformal, that is it preserves angles, and it maps the sphere’s parallelsMathworldPlanetmathPlanetmathPlanetmath into straight line segments of length 2⁢π⁢R. (A parallel of latitude means a small circle comprised of points at a specified latitude).

Starting from these two properties we can derive the Mercator Projection. First note that a parallel of latitude λ has length 2⁢π⁢R⁢cos⁡(λ). To make the projections of the parallels all the same length a stretching factor in longitude of 1cos⁡(λ) will have to be applied. For the mapping to be conformal, the same stretching factor must be applied in latitude also. Note that the stretching factor varies with λ so to map a specified latitude λ0 to an ordinate y we must evaluate an integral.

y=∫0λ0(1/cos⁡(λ))⁢𝑑λ

Early mapmakers such as Mercator evaluated this integral numerically to produce what is called a Table of Meridional Parts that can be used to map λ0 into y. Later it was noticed that the integral of one over cosine actually has a closed form, leading to the expression for y shown above.

Title Mercator projection
Canonical name MercatorProjection
Date of creation 2013-03-22 15:19:53
Last modified on 2013-03-22 15:19:53
Owner acastaldo (8031)
Last modified by acastaldo (8031)
Numerical id 5
Author acastaldo (8031)
Entry type Definition
Classification msc 86A30
Related topic RiemannSphere
Related topic ConformalityOfStereographicProjection
Related topic InverseGudermannianFunction