The Mollweide projection is an equal-area, pseudocylindrical map projection generally used for global maps of the world or night sky. It is also known as the Babinet projection, homalographic projection, homolographic projection, and elliptical projection. The projection trades accuracy of angle and shape for accuracy of proportions in area, and as such is used where that property is needed, such as maps depicting global distributions.
The projection was first published by mathematician and astronomer Karl (or Carl) Brandan Mollweide (1774 – 1825) of Leipzig in 1805. It was reinvented and popularized by Jacques Babinet in 1857, who gave it the name homalographic projection. The variation homolographic arose from frequent nineteenth century usage in star atlases.
The Mollweide is a pseudocylindrical projection in which the equator is represented as a straight horizontal line perpendicular to a central meridian one-half its length. The other parallels compress near the poles, while the other meridians are equally spaced at the equator. The meridians at 90 degrees east and west form a perfect circle, and the whole earth is depicted in a proportional 2:1 ellipse. The proportion of the area of the ellipse between any given parallel and the equator is the same as the proportion of the area on the globe between that parallel and the equator, but at the expense of shape distortion, which is significant at the perimeter of the ellipse, although not as severe as in the sinusoidal projection.
Shape distortion may be diminished by using an interrupted version. A sinusoidal interrupted Mollweide projection discards the central meridian in favor of alternating half-meridians which terminate at right angles to the equator. This has the effect of dividing the globe into lobes shape. In contrast, a parallel interrupted Mollweide projection uses multiple disjoint central meridians, giving the effect of multiple ellipses joined at the equator. More rarely, the project can be drawn obliquely to shift the areas of distortion to the oceans, allowing the continents to remain truer to form.
The projection transforms from latitude and longitude to map coordinates through the following equations:
where is an auxiliary angle defined by
and λ is the longitude, λ0 is the central meridian, and φ is the latitude.
If φ = ±π/2, then also θ = ±π/2. In that case the iteration should be bypassed; otherwise, division by zero may result.
where θ can be found by the relation
The inverse transformations allow one to find the latitude and longitude corresponding to the map coordinates x and y.
- Flattening the Earth: Two Thousand Years of Map Projections, John P. Snyder, 1993, pp. 112–113, ISBN 0-226-76747-7.
- Gannon, Megan (December 21, 2012). "New 'Baby Picture' of Universe Unveiled". Space.com. Retrieved December 21, 2012.
- Bennett, C.L.; Larson, L.; Weiland, J.L.; Jarosk, N.; Hinshaw, N.; Odegard, N.; Smith, K.M.; Hill, R.S.; Gold, B.; Halpern, M.; Komatsu, E.; Nolta, M.R.; Page, L. (December 20, 2012). Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results. arXiv:1212.5225. Retrieved December 22, 2012.
- Map Projections – A Working Manual, USGS Professional Paper 1395, John P. Snyder, 1987, pp. 249–252
- Weisstein, Eric W., "Mollweide Projection", MathWorld.
|Wikimedia Commons has media related to Mollweide projection.|
- An interactive JAVA applet to study deformations (area, distance and angle) of the Mollweide Map Projection
- Mollweide Projection at Mathworld