In cartography, a **map projection** is a way to flatten a globe's surface into a plane in order to make a map. This requires a systematic transformation of the latitudes and longitudes of locations from the surface of the globe into locations on a plane.^{ [1] } All projections of a sphere on a plane necessarily distort the surface in some way and to some extent. Depending on the purpose of the map, some distortions are acceptable and others are not; therefore, different map projections exist in order to preserve some properties of the sphere-like body at the expense of other properties. The study of map projections is the characterization of the distortions. There is no limit to the number of possible map projections.^{ [2] }^{:1} Projections are a subject of several pure mathematical fields, including differential geometry, projective geometry, and manifolds. However, "map projection" refers specifically to a cartographic projection.

- Metric properties of maps
- Distortion
- Design and construction
- Choosing a projection surface
- Aspect of the projection
- Notable lines
- Scale
- Choosing a model for the shape of the body
- Classification
- Projections by surface
- Cylindrical
- Pseudocylindrical
- Hybrid
- Conic
- Pseudoconic
- Azimuthal (projections onto a plane)
- Projections by preservation of a metric property
- Conformal
- Equal-area
- Equidistant
- Gnomonic
- Retroazimuthal
- Compromise projections
- Which projection is best?
- See also
- References
- Citations
- Sources
- External links

Despite the name's literal meaning, projection is not limited to perspective projections, such as those resulting from casting a shadow on a screen, or the rectilinear image produced by a pinhole camera on a flat film plate. Rather, any mathematical function that transforms coordinates from the curved surface distinctly and smoothly to the plane is a projection. Few projections in practical use are perspective.^{[ citation needed ]}

Most of this article assumes that the surface to be mapped is that of a sphere. The Earth and other large celestial bodies are generally better modeled as oblate spheroids, whereas small objects such as asteroids often have irregular shapes. The surfaces of planetary bodies can be mapped even if they are too irregular to be modeled well with a sphere or ellipsoid.^{ [3] } Therefore, more generally, a map projection is any method of flattening a continuous curved surface onto a plane.^{[ citation needed ]}

A model globe does not distort surface relationships the way maps do, but maps can be more useful in many situations: they are more compact and easier to store; they readily accommodate an enormous range of scales; they are viewed easily on computer displays; they can be measured to find properties of the region being mapped; they can show larger portions of the Earth's surface at once; and they are cheaper to produce and transport. These useful traits of maps motivate the development of map projections.

The best known map projection is the Mercator projection.^{ [2] }^{:45} Despite its important conformal properties, it has been criticized throughout the twentieth century for enlarging area further from the equator.^{ [2] }^{:156–157} Equal area map projections such as the Sinusoidal projection and the Gall–Peters projection show the correct sizes of countries relative to each other, but distort angles. The National Geographic Society and most atlases favor map projections that compromise between area and angular distortion, such as the Robinson projection or the Winkel tripel projection ^{ [2] }^{ [4] }

Many properties can be measured on the Earth's surface independent of its geography:

Map projections can be constructed to preserve some of these properties at the expense of others. Because the curved Earth's surface is not isometric to a plane, preservation of shapes inevitably leads to a variable scale and, consequently, non-proportional presentation of areas. Vice versa, an area-preserving projection can not be conformal, resulting in shapes and bearings distorted in most places of the map. Each projection preserves, compromises, or approximates basic metric properties in different ways. The purpose of the map determines which projection should form the base for the map. Because many purposes exist for maps, a diversity of projections have been created to suit those purposes.

Another consideration in the configuration of a projection is its compatibility with data sets to be used on the map. Data sets are geographic information; their collection depends on the chosen datum (model) of the Earth. Different datums assign slightly different coordinates to the same location, so in large scale maps, such as those from national mapping systems, it is important to match the datum to the projection. The slight differences in coordinate assignation between different datums is not a concern for world maps or other vast territories, where such differences get shrunk to imperceptibility.

Carl Friedrich Gauss's Theorema Egregium proved that a sphere's surface cannot be represented on a plane without distortion. The same applies to other reference surfaces used as models for the Earth, such as oblate spheroids, ellipsoids and geoids. Since any map projection is a representation of one of those surfaces on a plane, all map projections distort.

The classical way of showing the distortion inherent in a projection is to use Tissot's indicatrix. For a given point, using the scale factor *h* along the meridian, the scale factor *k* along the parallel, and the angle *θ′* between them, Nicolas Tissot described how to construct an ellipse that characterizes the amount and orientation of the components of distortion.^{ [2] }^{:147–149}^{ [5] } By spacing the ellipses regularly along the meridians and parallels, the network of indicatrices shows how distortion varies across the map.

Many other ways have been described for characterizing distortion in projections.^{ [6] }^{ [7] } Like Tissot's indicatrix, the **Goldberg-Gott indicatrix** is based on infinitesimals, and depicts *flexion* and *skewness* (bending and lopsidedness) distortions.^{ [8] }

Rather than the original (enlarged) infinitesimal circle as in Tissot's indicatrix, some visual methods project finite shapes that span a part of the map. For example, a small circle of fixed radius (e.g., 15-degrees angular radius).^{ [9] } Sometimes spherical triangles are used.^{[ citation needed ]} In the first half of the 20th century, projecting a human head onto different projections was common to show how distortion varies across one projection as compared to another.^{ [10] } In dynamic media, shapes of familiar coastlines and boundaries can be dragged across an interactive map to show how the projection distorts sizes and shapes according to position on the map.^{ [11] }

Another way to visualize local distortion is through grayscale or color gradations whose shade represents the magnitude of the angular deformation or areal inflation. Sometimes both are shown simultaneously by blending two colors to create a bivariate map.^{ [12] }

The problem of characterizing distortion globally across areas instead of at just a single point is that it necessarily involves choosing priorities to reach a compromise. Some schemes use distance distortion as a proxy for the combination of angular deformation and areal inflation; such methods arbitrarily choose what paths to measure and how to weight them in order to yield a single result. Many have been described.^{ [8] }^{ [13] }^{ [14] }^{ [15] }^{ [16] }

The creation of a map projection involves two steps:

- Selection of a model for the shape of the Earth or planetary body (usually choosing between a sphere or ellipsoid). Because the Earth's actual shape is irregular, information is lost in this step.
- Transformation of geographic coordinates (longitude and latitude) to Cartesian (
*x*,*y*) or polar plane coordinates. In large-scale maps, Cartesian coordinates normally have a simple relation to eastings and northings defined as a grid superimposed on the projection. In small-scale maps, eastings and northings are not meaningful, and grids are not superimposed.

Some of the simplest map projections are literal projections, as obtained by placing a light source at some definite point relative to the globe and projecting its features onto a specified surface. Although most projections are not defined in this way, picturing the light source-globe model can be helpful in understanding the basic concept of a map projection.

A surface that can be unfolded or unrolled into a plane or sheet without stretching, tearing or shrinking is called a * developable surface *. The cylinder, cone and the plane are all developable surfaces. The sphere and ellipsoid do not have developable surfaces, so any projection of them onto a plane will have to distort the image. (To compare, one cannot flatten an orange peel without tearing and warping it.)

One way of describing a projection is first to project from the Earth's surface to a developable surface such as a cylinder or cone, and then to unroll the surface into a plane. While the first step inevitably distorts some properties of the globe, the developable surface can then be unfolded without further distortion.

Once a choice is made between projecting onto a cylinder, cone, or plane, the **aspect** of the shape must be specified. The aspect describes how the developable surface is placed relative to the globe: it may be *normal* (such that the surface's axis of symmetry coincides with the Earth's axis), *transverse* (at right angles to the Earth's axis) or *oblique* (any angle in between).

The developable surface may also be either * tangent * or * secant * to the sphere or ellipsoid. Tangent means the surface touches but does not slice through the globe; secant means the surface does slice through the globe. Moving the developable surface away from contact with the globe never preserves or optimizes metric properties, so that possibility is not discussed further here.

Tangent and secant lines (*standard lines*) are represented undistorted. If these lines are a parallel of latitude, as in conical projections, it is called a *standard parallel*. The *central meridian* is the meridian to which the globe is rotated before projecting. The central meridian (usually written *λ*_{0}) and a parallel of origin (usually written *φ*_{0}) are often used to define the origin of the map projection.^{ [17] }^{ [18] }

A globe is the only way to represent the Earth with constant scale throughout the entire map in all directions. A map cannot achieve that property for any area, no matter how small. It can, however, achieve constant scale along specific lines.

Some possible properties are:

- The scale depends on location, but not on direction. This is equivalent to preservation of angles, the defining characteristic of a conformal map.
- Scale is constant along any parallel in the direction of the parallel. This applies for any cylindrical or pseudocylindrical projection in normal aspect.
- Combination of the above: the scale depends on latitude only, not on longitude or direction. This applies for the Mercator projection in normal aspect.
- Scale is constant along all straight lines radiating from a particular geographic location. This is the defining characteristic of an equidistant projection such as the Azimuthal equidistant projection. There are also projections (Maurer's Two-point equidistant projection, Close) where true distances from
*two*points are preserved.^{ [2] }^{:234}

Projection construction is also affected by how the shape of the Earth or planetary body is approximated. In the following section on projection categories, the earth is taken as a sphere in order to simplify the discussion. However, the Earth's actual shape is closer to an oblate ellipsoid. Whether spherical or ellipsoidal, the principles discussed hold without loss of generality.

Selecting a model for a shape of the Earth involves choosing between the advantages and disadvantages of a sphere versus an ellipsoid. Spherical models are useful for small-scale maps such as world atlases and globes, since the error at that scale is not usually noticeable or important enough to justify using the more complicated ellipsoid. The ellipsoidal model is commonly used to construct topographic maps and for other large- and medium-scale maps that need to accurately depict the land surface. Auxiliary latitudes are often employed in projecting the ellipsoid.

A third model is the geoid, a more complex and accurate representation of Earth's shape coincident with what mean sea level would be if there were no winds, tides, or land. Compared to the best fitting ellipsoid, a geoidal model would change the characterization of important properties such as distance, conformality and equivalence. Therefore, in geoidal projections that preserve such properties, the mapped graticule would deviate from a mapped ellipsoid's graticule. Normally the geoid is not used as an Earth model for projections, however, because Earth's shape is very regular, with the undulation of the geoid amounting to less than 100 m from the ellipsoidal model out of the 6.3 million m Earth radius. For irregular planetary bodies such as asteroids, however, sometimes models analogous to the geoid are used to project maps from.^{ [19] }^{ [20] }^{ [21] }^{ [22] }^{ [23] }

Other regular solids are sometimes used as generalizations for smaller bodies' geoidal equivalent. For example, Io is better modeled by triaxial ellipsoid or prolated spheroid with small eccentricities. Haumea's shape is a Jacobi ellipsoid, with its major axis twice as long as its minor and with its middle axis one and half times as long as its minor. See map projection of the triaxial ellipsoid for further information.

A fundamental projection classification is based on the type of projection surface onto which the globe is conceptually projected. The projections are described in terms of placing a gigantic surface in contact with the Earth, followed by an implied scaling operation. These surfaces are cylindrical (e.g. Mercator), conic (e.g. Albers), and plane (e.g. stereographic). Many mathematical projections, however, do not neatly fit into any of these three conceptual projection methods. Hence other peer categories have been described in the literature, such as pseudoconic, pseudocylindrical, pseudoazimuthal, retroazimuthal, and polyconic.

Another way to classify projections is according to properties of the model they preserve. Some of the more common categories are:

- Preserving direction (
*azimuthal or zenithal*), a trait possible only from one or two points to every other point^{ [24] } - Preserving shape locally (
*conformal*or*orthomorphic*) - Preserving area (
*equal-area*or*equiareal*or*equivalent*or*authalic*) - Preserving distance (
*equidistant*), a trait possible only between one or two points and every other point - Preserving shortest route, a trait preserved only by the gnomonic projection

Because the sphere is not a developable surface, it is impossible to construct a map projection that is both equal-area and conformal.

The three developable surfaces (plane, cylinder, cone) provide useful models for understanding, describing, and developing map projections. However, these models are limited in two fundamental ways. For one thing, most world projections in use do not fall into any of those categories. For another thing, even most projections that do fall into those categories are not naturally attainable through physical projection. As L.P. Lee notes,

No reference has been made in the above definitions to cylinders, cones or planes. The projections are termed cylindric or conic because they can be regarded as developed on a cylinder or a cone, as the case may be, but it is as well to dispense with picturing cylinders and cones, since they have given rise to much misunderstanding. Particularly is this so with regard to the conic projections with two standard parallels: they may be regarded as developed on cones, but they are cones which bear no simple relationship to the sphere. In reality, cylinders and cones provide us with convenient descriptive terms, but little else.

^{ [25] }

Lee's objection refers to the way the terms *cylindrical*, *conic*, and *planar* (azimuthal) have been abstracted in the field of map projections. If maps were projected as in light shining through a globe onto a developable surface, then the spacing of parallels would follow a very limited set of possibilities. Such a cylindrical projection (for example) is one which:

- Is rectangular;
- Has straight vertical meridians, spaced evenly;
- Has straight parallels symmetrically placed about the equator;
- Has parallels constrained to where they fall when light shines through the globe onto the cylinder, with the light source someplace along the line formed by the intersection of the prime meridian with the equator, and the center of the sphere.

(If you rotate the globe before projecting then the parallels and meridians will not necessarily still be straight lines. Rotations are normally ignored for the purpose of classification.)

Where the light source emanates along the line described in this last constraint is what yields the differences between the various "natural" cylindrical projections. But the term *cylindrical* as used in the field of map projections relaxes the last constraint entirely. Instead the parallels can be placed according to any algorithm the designer has decided suits the needs of the map. The famous Mercator projection is one in which the placement of parallels does not arise by projection; instead parallels are placed how they need to be in order to satisfy the property that a course of constant bearing is always plotted as a straight line.

A normal cylindrical projection is any projection in which meridians are mapped to equally spaced vertical lines and circles of latitude (parallels) are mapped to horizontal lines.

The mapping of meridians to vertical lines can be visualized by imagining a cylinder whose axis coincides with the Earth's axis of rotation. This cylinder is wrapped around the Earth, projected onto, and then unrolled.

By the geometry of their construction, cylindrical projections stretch distances east-west. The amount of stretch is the same at any chosen latitude on all cylindrical projections, and is given by the secant of the latitude as a multiple of the equator's scale. The various cylindrical projections are distinguished from each other solely by their north-south stretching (where latitude is given by φ):

- North-south stretching equals east-west stretching (sec
*φ*): The east-west scale matches the north-south scale: conformal cylindrical or Mercator; this distorts areas excessively in high latitudes (see also transverse Mercator). - North-south stretching grows with latitude faster than east-west stretching (sec
^{2}*φ*): The cylindric perspective (or central cylindrical) projection; unsuitable because distortion is even worse than in the Mercator projection. - North-south stretching grows with latitude, but less quickly than the east-west stretching: such as the Miller cylindrical projection (sec 4/5
*φ*). - North-south distances neither stretched nor compressed (1): equirectangular projection or "plate carrée".
- North-south compression equals the cosine of the latitude (the reciprocal of east-west stretching): equal-area cylindrical. This projection has many named specializations differing only in the scaling constant, such as the Gall–Peters or Gall orthographic (undistorted at the 45° parallels), Behrmann (undistorted at the 30° parallels), and Lambert cylindrical equal-area (undistorted at the equator). Since this projection scales north-south distances by the reciprocal of east-west stretching, it preserves area at the expense of shapes.

In the first case (Mercator), the east-west scale always equals the north-south scale. In the second case (central cylindrical), the north-south scale exceeds the east-west scale everywhere away from the equator. Each remaining case has a pair of secant lines—a pair of identical latitudes of opposite sign (or else the equator) at which the east-west scale matches the north-south-scale.

Normal cylindrical projections map the whole Earth as a finite rectangle, except in the first two cases, where the rectangle stretches infinitely tall while retaining constant width.

Pseudocylindrical projections represent the *central* meridian as a straight line segment. Other meridians are longer than the central meridian and bow outward, away from the central meridian. Pseudocylindrical projections map parallels as straight lines. Along parallels, each point from the surface is mapped at a distance from the central meridian that is proportional to its difference in longitude from the central meridian. Therefore, meridians are equally spaced along a given parallel. On a pseudocylindrical map, any point further from the equator than some other point has a higher latitude than the other point, preserving north-south relationships. This trait is useful when illustrating phenomena that depend on latitude, such as climate. Examples of pseudocylindrical projections include:

- Sinusoidal, which was the first pseudocylindrical projection developed. On the map, as in reality, the length of each parallel is proportional to the cosine of the latitude.
^{ [26] }The area of any region is true. - Collignon projection, which in its most common forms represents each meridian as two straight line segments, one from each pole to the equator.

The HEALPix projection combines an equal-area cylindrical projection in equatorial regions with the Collignon projection in polar areas.

The term "conic projection" is used to refer to any projection in which meridians are mapped to equally spaced lines radiating out from the apex and circles of latitude (parallels) are mapped to circular arcs centered on the apex.^{ [27] }

When making a conic map, the map maker arbitrarily picks two standard parallels. Those standard parallels may be visualized as secant lines where the cone intersects the globe—or, if the map maker chooses the same parallel twice, as the tangent line where the cone is tangent to the globe. The resulting conic map has low distortion in scale, shape, and area near those standard parallels. Distances along the parallels to the north of both standard parallels or to the south of both standard parallels are stretched; distances along parallels between the standard parallels are compressed. When a single standard parallel is used, distances along all other parallels are stretched.

Conic projections that are commonly used are:

- Equidistant conic, which keeps parallels evenly spaced along the meridians to preserve a constant distance scale along each meridian, typically the same or similar scale as along the standard parallels.
- Albers conic, which adjusts the north-south distance between non-standard parallels to compensate for the east-west stretching or compression, giving an equal-area map.
- Lambert conformal conic, which adjusts the north-south distance between non-standard parallels to equal the east-west stretching, giving a conformal map.

- Bonne, an equal-area projection on which most meridians and parallels appear as curved lines. It has a configurable standard parallel along which there is no distortion.
- Werner cordiform, upon which distances are correct from one pole, as well as along all parallels.
- American polyconic and other projections in the polyconic projection class.

Azimuthal projections have the property that directions from a central point are preserved and therefore great circles through the central point are represented by straight lines on the map. These projections also have radial symmetry in the scales and hence in the distortions: map distances from the central point are computed by a function *r*(*d*) of the true distance *d*, independent of the angle; correspondingly, circles with the central point as center are mapped into circles which have as center the central point on the map.

The mapping of radial lines can be visualized by imagining a plane tangent to the Earth, with the central point as tangent point.

The radial scale is *r′*(*d*) and the transverse scale *r*(*d*)/(*R* sin *d*/*R*) where *R* is the radius of the Earth.

Some azimuthal projections are true perspective projections; that is, they can be constructed mechanically, projecting the surface of the Earth by extending lines from a point of perspective (along an infinite line through the tangent point and the tangent point's antipode) onto the plane:

- The gnomonic projection displays great circles as straight lines. Can be constructed by using a point of perspective at the center of the Earth.
*r*(*d*) =*c*tan*d*/*R*; so that even just a hemisphere is already infinite in extent.^{ [28] }^{ [29] } - The orthographic projection maps each point on the Earth to the closest point on the plane. Can be constructed from a point of perspective an infinite distance from the tangent point;
*r*(*d*) =*c*sin*d*/*R*.^{ [30] }Can display up to a hemisphere on a finite circle. Photographs of Earth from far enough away, such as the Moon, approximate this perspective. - Near-sided perspective projection, which simulates the view from space at a finite distance and therefore shows less than a full hemisphere, such as used in
*The Blue Marble 2012*).^{ [31] } - The General Perspective projection can be constructed by using a point of perspective outside the Earth. Photographs of Earth (such as those from the International Space Station) give this perspective. It is a generalization of near-sided perspective projection, allowing tilt.
- The stereographic projection, which is conformal, can be constructed by using the tangent point's antipode as the point of perspective.
*r*(*d*) =*c*tan*d*/2*R*; the scale is*c*/(2*R*cos^{2}*d*/2*R*).^{ [32] }Can display nearly the entire sphere's surface on a finite circle. The sphere's full surface requires an infinite map.

Other azimuthal projections are not true perspective projections:

- Azimuthal equidistant:
*r*(*d*) =*cd*; it is used by amateur radio operators to know the direction to point their antennas toward a point and see the distance to it. Distance from the tangent point on the map is proportional to surface distance on the Earth (;^{ [33] }for the case where the tangent point is the North Pole, see the flag of the United Nations) - Lambert azimuthal equal-area. Distance from the tangent point on the map is proportional to straight-line distance through the Earth:
*r*(*d*) =*c*sin*d*/2*R*^{ [34] } - Logarithmic azimuthal is constructed so that each point's distance from the center of the map is the logarithm of its distance from the tangent point on the Earth.
*r*(*d*) =*c*ln*d*/*d*_{0}); locations closer than at a distance equal to the constant*d*_{0}are not shown.^{ [35] }^{ [36] }

Conformal, or orthomorphic, map projections preserve angles locally, implying that they map infinitesimal circles of constant size anywhere on the Earth to infinitesimal circles of varying sizes on the map. In contrast, mappings that are not conformal distort most such small circles into ellipses of distortion. An important consequence of conformality is that relative angles at each point of the map are correct, and the local scale (although varying throughout the map) in every direction around any one point is constant. These are some conformal projections:

- Mercator: Rhumb lines are represented by straight segments
- Transverse Mercator
- Stereographic: Any circle of a sphere, great and small, maps to a circle or straight line.
- Roussilhe
- Lambert conformal conic
- Peirce quincuncial projection
- Adams hemisphere-in-a-square projection
- Guyou hemisphere-in-a-square projection

Equal-area maps preserve area measure, generally distorting shapes in order to do that. Equal-area maps are also called *equivalent* or *authalic*. These are some projections that preserve area:

- Albers conic
- Bonne
- Bottomley
- Collignon
- Cylindrical equal-area
- Eckert II, IV and VI
- Equal Earth
- Gall orthographic (also known as Gall–Peters, or Peters, projection)
- Goode's homolosine
- Hammer
- Hobo–Dyer
- Lambert azimuthal equal-area
- Lambert cylindrical equal-area
- Mollweide
- Sinusoidal
- Strebe 1995
- Snyder's equal-area polyhedral projection, used for geodesic grids.
- Tobler hyperelliptical
- Werner

If the length of the line segment connecting two projected points on the plane is proportional to the geodesic (shortest surface) distance between the two unprojected points on the globe, then we say that distance has been preserved between those two points. An **equidistant projection** preserves distances from one or two special points to all other points. The special point or points may get stretched into a line or curve segment when projected. In that case, the point on the line or curve segment closest to the point being measured to must be used to measure the distance.

- Plate carrée: Distances from the two poles are preserved, in equatorial aspect.
- Azimuthal equidistant: Distances from the center and edge are preserved.
- Equidistant conic: Distances from the two poles are preserved, in equatorial aspect.
- Werner cordiform Distances from the North Pole are preserved, in equatorial aspect.
- Two-point equidistant: Two "control points" are arbitrarily chosen by the map maker; distances from each control point are preserved.

Great circles are displayed as straight lines:

Direction to a fixed location B (the bearing at the starting location A of the shortest route) corresponds to the direction on the map from A to B:

- Littrow—the only conformal retroazimuthal projection
- Hammer retroazimuthal—also preserves distance from the central point
- Craig retroazimuthal
*aka*Mecca or Qibla—also has vertical meridians

Compromise projections give up the idea of perfectly preserving metric properties, seeking instead to strike a balance between distortions, or to simply make things look right. Most of these types of projections distort shape in the polar regions more than at the equator. These are some compromise projections:

The mathematics of projection do not permit any particular map projection to be best for everything.^{ [37] } Something will always be distorted. Thus, many projections exist to serve the many uses of maps and their vast range of scales.

Modern national mapping systems typically employ a transverse Mercator or close variant for large-scale maps in order to preserve conformality and low variation in scale over small areas. For smaller-scale maps, such as those spanning continents or the entire world, many projections are in common use according to their fitness for the purpose, such as Winkel tripel, Robinson and Mollweide.^{ [38] } Reference maps of the world often appear on compromise projections. Due to distortions inherent in any map of the world, the choice of projection becomes largely one of aesthetics.

Thematic maps normally require an equal area projection so that phenomena per unit area are shown in correct proportion.^{ [39] } However, representing area ratios correctly necessarily distorts shapes more than many maps that are not equal-area.

The Mercator projection, developed for navigational purposes, has often been used in world maps where other projections would have been more appropriate.^{ [40] }^{ [41] }^{ [42] }^{ [43] } This problem has long been recognized even outside professional circles. For example, a 1943 * New York Times * editorial states:

The time has come to discard [the Mercator] for something that represents the continents and directions less deceptively ... Although its usage ... has diminished ... it is still highly popular as a wall map apparently in part because, as a rectangular map, it fills a rectangular wall space with more map, and clearly because its familiarity breeds more popularity.

^{ [2] }^{:166}

A controversy in the 1980s over the Peters map motivated the American Cartographic Association (now Cartography and Geographic Information Society) to produce a series of booklets (including *Which Map Is Best*^{ [44] }) designed to educate the public about map projections and distortion in maps. In 1989 and 1990, after some internal debate, seven North American geographic organizations adopted a resolution recommending against using any rectangular projection (including Mercator and Gall–Peters) for reference maps of the world.^{ [45] }^{ [46] }

The **Gall–Peters projection** is a rectangular map projection that maps all areas such that they have the correct sizes relative to each other. Like any equal-area projection, it achieves this goal by distorting most shapes. The projection is a particular example of the cylindrical equal-area projection with latitudes 45° north and south as the regions on the map that have no distortion.

In geography, **latitude** is a geographic coordinate that specifies the north–south position of a point on the Earth's surface. Latitude is an angle which ranges from 0° at the Equator to 90° at the poles. Lines of constant latitude, or *parallels*, run east–west as circles parallel to the equator. Latitude is used together with longitude to specify the precise location of features on the surface of the Earth. On its own, the term latitude should be taken to be the *geodetic latitude* as defined below. Briefly, geodetic latitude at a point is the angle formed by the vector perpendicular to the ellipsoidal surface from that point, and the equatorial plane. Also defined are six *auxiliary latitudes* that are used in special applications.

The **Mercator projection** is a cylindrical map projection presented by Flemish geographer and cartographer Gerardus Mercator in 1569. It became the standard map projection for navigation because it is unique in representing north as up and south as down everywhere while preserving local directions and shapes. The map is thereby conformal. As a side effect, the Mercator projection inflates the size of objects away from the equator. This inflation is very small near the equator but accelerates with increasing latitude to become infinite at the poles. So, for example, landmasses such as Greenland and Antarctica appear far larger than they actually are relative to landmasses near the equator, such as Central Africa.

A **geographic coordinate system** (**GCS**) is a coordinate system associated with positions on Earth. A GCS can give positions:

The **transverse Mercator** map projection is an adaptation of the standard Mercator projection. The transverse version is widely used in national and international mapping systems around the world, including the Universal Transverse Mercator. When paired with a suitable geodetic datum, the transverse Mercator delivers high accuracy in zones less than a few degrees in east-west extent.

**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.

A **gnomonic map projection** displays all great circles as straight lines, resulting in any straight line segment on a gnomonic map showing a geodesic, the shortest route between the segment's two endpoints. This is achieved by casting surface points of the sphere onto a tangent plane, each landing where a ray from the center of the sphere passes through the point on the surface and then on to the plane. No distortion occurs at the tangent point, but distortion increases rapidly away from it. Less than half of the sphere can be projected onto a finite map. Consequently, a rectilinear photographic lens, which is based on the gnomonic principle, cannot image more than 180 degrees.

The **scale** of a map is the ratio of a distance on the map to the corresponding distance on the ground. This simple concept is complicated by the curvature of the Earth's surface, which forces scale to vary across a map. Because of this variation, the concept of scale becomes meaningful in two distinct ways.

The **equirectangular projection** (also called the **equidistant cylindrical projection** or **la carte parallélogrammatique projection**, and which includes the special case of the **plate carrée projection**, is a simple map projection attributed to Marinus of Tyre, who Ptolemy claims invented the projection about AD 100. The projection maps meridians to vertical straight lines of constant spacing, and circles of latitude to horizontal straight lines of constant spacing. The projection is neither equal area nor conformal. Because of the distortions introduced by this projection, it has little use in navigation or cadastral mapping and finds its main use in thematic mapping. In particular, the plate carrée has become a standard for global raster datasets, such as Celestia, NASA World Wind, and Natural Earth, because of the particularly simple relationship between the position of an image pixel on the map and its corresponding geographic location on Earth. In addition it is frequently used in panoramic photography to represent a spherical panoramic image.

The **oblique Mercator** map projection is an adaptation of the standard Mercator projection. The oblique version is sometimes used in national mapping systems. When paired with a suitable geodetic datum, the oblique Mercator delivers high accuracy in zones less than a few degrees in arbitrary directional extent.

The **universal polar stereographic** (**UPS**) coordinate system is used in conjunction with the universal transverse Mercator (UTM) coordinate system to locate positions on the surface of the earth. Like the UTM coordinate system, the UPS coordinate system uses a metric-based cartesian grid laid out on a conformally projected surface. UPS covers the Earth's polar regions, specifically the areas north of 84°N and south of 80°S, which are not covered by the UTM grids, plus an additional 30 minutes of latitude extending into UTM grid to provide some overlap between the two systems.

In cartography, a **Tissot's indicatrix** is a mathematical contrivance presented by French mathematician Nicolas Auguste Tissot in 1859 and 1871 in order to characterize local distortions due to map projection. It is the geometry that results from projecting a circle of infinitesimal radius from a curved geometric model, such as a globe, onto a map. Tissot proved that the resulting diagram is an ellipse whose axes indicate the two principal directions along which scale is maximal and minimal at that point on the map.

A **Lambert conformal conic projection** (**LCC**) is a conic map projection used for aeronautical charts, portions of the State Plane Coordinate System, and many national and regional mapping systems. It is one of seven projections introduced by Johann Heinrich Lambert in his 1772 publication *Anmerkungen und Zusätze zur Entwerfung der Land- und Himmelscharten*.

In cartography, the **Lambert cylindrical equal-area projection**, or **Lambert cylindrical projection**, is a cylindrical equal-area projection. This projection is undistorted along the equator, which is its standard parallel, but distortion increases rapidly towards the poles. Like any cylindrical projection, it stretches parallels increasingly away from the equator. The poles accrue infinite distortion, becoming lines instead of points.

In cartography, a **conformal map projection** is one in which every angle between two curves that cross each other on Earth is preserved in the image of the projection, i.e. the projection is a conformal map in the mathematical sense. For example, if two roads cross each other at a 39° angle, then their images on a map with a conformal projection cross at a 39° angle.

In cartography, the **cylindrical equal-area projection** is a family of cylindrical, equal-area map projections.

The **central cylindrical projection** is a perspective cylindrical map projection. It corresponds to projecting the Earth's surface onto a cylinder tangent to the equator as if from a light source at Earth's center. The cylinder is then cut along one of the projected meridians and unrolled into a flat map.

In geodesy, a **map projection of the triaxial ellipsoid** maps Earth or some other astronomical body modeled as a triaxial ellipsoid to the plane. Such a model is called the reference ellipsoid. In most cases, reference ellipsoids are spheroids, and sometimes spheres. Massive objects have sufficient gravity to overcome their own rigidity and usually have an oblate ellipsoid shape. However, minor moons or small solar system bodies are not under hydrostatic equilibrium. Usually such bodies have irregular shapes. Furthermore, some of gravitationally rounded objects may have a tri-axial ellipsoid shape due to rapid rotation or unidirectional strong tidal forces.

The **stereographic projection**, also known as the **planisphere projection** or the **azimuthal conformal projection**, is a conformal map projection whose use dates back to antiquity. Like the orthographic projection and gnomonic projection, the stereographic projection is an azimuthal projection, and when on a sphere, also a perspective projection.

- ↑ Snyder, J.P. (1989).
*Album of Map Projections, United States Geological Survey Professional Paper*. United States Government Printing Office. 1453. - 1 2 3 4 5 6 7 Snyder, John P. (1993).
*Flattening the earth: two thousand years of map projections*. University of Chicago Press. ISBN 0-226-76746-9. - ↑ Hargitai, Henrik; Wang, Jue; Stooke, Philip J.; Karachevtseva, Irina; Kereszturi, Akos; Gede, Mátyás (2017), "Map Projections in Planetary Cartography",
*Lecture Notes in Geoinformation and Cartography*, Springer International Publishing, pp. 177–202, doi:10.1007/978-3-319-51835-0_7, ISBN 978-3-319-51834-3 - ↑ "Which is the best map projection?".
*Geoawesomeness*. 25 April 2017. - ↑ Snyder. Working Manual, p. 24.
- ↑ Karen A. Mulcahy and Keith C. Clarke (2001) "Symbolization of Map Projection Distortion: A Review",
*Cartography and Geographic Information Science*, 101.28, No.3, pp.167-181 - ↑ Frank Canters (2002),
*Small-Scale Map Projection Design*, CRC Press - 1 2 Goldberg, David M.; Gott III, J. Richard (2007). "Flexion and Skewness in Map Projections of the Earth" (PDF).
*Cartographica*.**42**(4): 297–318. arXiv: astro-ph/0608501 . doi:10.3138/carto.42.4.297. S2CID 11359702 . Retrieved 2011-11-14. - ↑ "Real-time projection visualisation with Indicatrix Mapper QGIS Plugin" (PDF).
- ↑ "Strange Maps: This is your brain on maps". 18 September 2013.
- ↑ "Mercator Puzzle Redux" . Retrieved 2018-01-24.
- ↑ "A cornucopia of map projections".
- ↑ Peters, A. B. (1978). "Uber Weltkartenverzerrunngen und Weltkartenmittelpunkte".
*Kartographische Nachrichten*: 106–113. - ↑ Gott, III, J. Richard; Mugnolo, Charles; Colley, Wesley N. (2006). "Map projections for minimizing distance errors". arXiv: astro-ph/0608500v1 .
- ↑ Laskowski, P. (1997). "Distortion-spectrum fundamentals: A new tool for analyzing and visualizing map distortions".
*Cartographica*.**34**(3). doi: 10.3138/Y51X-1590-PV21-136G . - ↑ Airy, G.B. (1861). "Explanation of a projection by balance of errors for maps applying to a very large extent of the Earth's surface; and comparison of this projection with other projections".
*London, Edinburgh, and Dublin Philosophical Magazine*. 4.**22**(149): 409–421. doi:10.1080/14786446108643179. - ↑ "Projection parameters".
- ↑ "Map projections".
- ↑ Cheng, Y.; Lorre, J. J. (2000). "Equal Area Map Projection for Irregularly Shaped Objects".
*Cartography and Geographic Information Science*.**27**(2): 91. doi:10.1559/152304000783547957. S2CID 128490229. - ↑ Stooke, P. J. (1998). "Mapping Worlds with Irregular Shapes".
*The Canadian Geographer*.**42**: 61. doi:10.1111/j.1541-0064.1998.tb01553.x. - ↑ Shingareva, K.B.; Bugaevsky, L.M.; Nyrtsov, M. (2000). "Mathematical Basis for Non-spherical Celestial Bodies Maps" (PDF).
*Journal of Geospatial Engineering*.**2**(2): 45–50. - ↑ Nyrtsov, M.V. (August 2003). "The Classification of Projections of Irregularly-shaped Celestial Bodies" (PDF).
*Proceedings of the 21st International Cartographic Conference (ICC)*: 1158–1164. - ↑ Clark, P. E.; Clark, C. S. (2013). "CSNB Mapping Applied to Irregular Bodies".
*Constant-Scale Natural Boundary Mapping to Reveal Global and Cosmic Processes*. SpringerBriefs in Astronomy. p. 71. doi:10.1007/978-1-4614-7762-4_6. ISBN 978-1-4614-7761-7. - ↑ Snyder, John Parr (1987).
*Map Projections – a Working Manual*. U.S. Government Printing Office. p. 192. ISBN 9780318235622. - ↑ Lee, L.P. (1944). "The nomenclature and classification of map projections".
*Empire Survey Review*.**VII**(51): 190–200. doi:10.1179/sre.1944.7.51.190. p. 193 - ↑ Weisstein, Eric W. "Sinusoidal Projection".
*MathWorld*. - ↑ Carlos A. Furuti. "Conic Projections"
- ↑ Weisstein, Eric W. "Gnomonic Projection".
*MathWorld*. - ↑ "The Gnomonic Projection" . Retrieved November 18, 2005.
- ↑ Weisstein, Eric W. "Orthographic Projection".
*MathWorld*. - ↑ "Near-sided perspective".
*PROJ 7.1.1 documentation*. 2020-09-17. Retrieved 2020-10-05. - ↑ Weisstein, Eric W. "Stereographic Projection".
*MathWorld*. - ↑ Weisstein, Eric W. "Azimuthal Equidistant Projection".
*MathWorld*. - ↑ Weisstein, Eric W. "Lambert Azimuthal Equal-Area Projection".
*MathWorld*. - ↑ Snyder, John P. "Enlarging the Heart of a Map". Archived from the original on July 2, 2010. Retrieved April 14, 2016.
- ↑ Snyder, John P. "Enlarging the Heart of a Map (accompanying figures)". Archived from the original on April 10, 2011. Retrieved November 18, 2005. (see figure 6-5)
- ↑
*Choosing a map projection*. Lapaine, Miljenko,, Usery, E. Lynn (Eddy Lynn), 1951-. Cham, Switzerland. 2017-04-04. ISBN 978-3-319-51835-0. OCLC 981765011.CS1 maint: others (link) - ↑
*Choosing a World Map*. Falls Church, Virginia: American Congress on Surveying and Mapping. 1988. p. 1. ISBN 0-9613459-2-6. - ↑ Slocum, Terry A.; Robert B. McMaster; Fritz C. Kessler; Hugh H. Howard (2005).
*Thematic Cartography and Geographic Visualization*(2nd ed.). Upper Saddle River, NJ: Pearson Prentice Hall. p. 166. ISBN 0-13-035123-7. - ↑ Bauer, H.A. (1942). "Globes, Maps, and Skyways (Air Education Series)". New York. p. 28
- ↑ Miller, Osborn Maitland (1942). "Notes on Cylindrical World Map Projections".
*Geographical Review*.**32**(3): 424–430. doi:10.2307/210384. JSTOR 210384. - ↑ Raisz, Erwin Josephus. (1938).
*General Cartography*. New York: McGraw–Hill. 2d ed., 1948. p. 87. - ↑ Robinson, Arthur Howard. (1960).
*Elements of Cartography*, second edition. New York: John Wiley and Sons. p. 82. - ↑ American Cartographic Association's Committee on Map Projections, 1986.
*Which Map is Best*p. 12. Falls Church: American Congress on Surveying and Mapping. - ↑ Robinson, Arthur (1990). "Rectangular World Maps—No!".
*Professional Geographer*.**42**(1): 101–104. doi:10.1111/j.0033-0124.1990.00101.x. - ↑ "Geographers and Cartographers Urge End to Popular Use of Rectangular Maps".
*American Cartographer*.**16**: 222–223. 1989. doi:10.1559/152304089783814089.

- Fran Evanisko, American River College, lectures for Geography 20: "Cartographic Design for GIS", Fall 2002
- Map Projections—PDF versions of numerous projections, created and released into the Public Domain by Paul B. Anderson ... member of the International Cartographic Association's Commission on Map Projections

- "An Album of Map Projections" (PDF). (12.6 MB), U.S. Geological Survey Professional Paper 1453, by John P. Snyder (USGS) and Philip M. Voxland (U. Minnesota), 1989.
- A Cornucopia of Map Projections, a visualization of distortion on a vast array of map projections in a single image.
- G.Projector, free software can render many projections (NASA GISS).
- Color images of map projections and distortion (Mapthematics.com).
- Geometric aspects of mapping: map projection (KartoWeb.itc.nl).
- Java world map projections, Henry Bottomley (SE16.info).
- Map Projections (MathWorld).
- MapRef: The Internet Collection of MapProjections and Reference Systems in Europe
- PROJ.4 – Cartographic Projections Library.
- Projection Reference Table of examples and properties of all common projections (RadicalCartography.net).
- "Understanding Map Projections" (PDF). (1.70 MB), Melita Kennedy (Esri).
- World Map Projections, Stephen Wolfram based on work by Yu-Sung Chang (Wolfram Demonstrations Project).
- Compare Map Projections

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