Lune (geometry)

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In geometry, a lune is either of two figures, both shaped roughly like a crescent Moon. The word "lune" derives from luna, the Latin word for Moon.

Plane geometry[edit]

In plane geometry, a lune is the concave-convex area bounded by two circular arcs, while a convex-convex area is termed a lens. [1]

Formally, a lune is the relative complement of one disk in another (where they intersect but neither is a subset of the other). Alternatively, if A and B are disks, then L = A - A \cap B is a lune.

Luno ebena geom 1.png Luno ebena geom 3.png Luno ebena geom 5.png
Luno ebena geom 2.png Luno ebena geom 4.png Luno ebena geom 6.png
In plane geometry, the crescent shape formed from two intersecting circles is called a lune (in gray). There are two lunes in each diagram only one of which is shaded

Lune of Hippocrates[edit]

In the 5th century BC, Hippocrates of Chios showed that certain lunes could be exactly squared by straightedge and compass. See Lune of Hippocrates.

Spherical geometry[edit]

A spherical lune. The two great circles are shown as thin black lines, whereas the lune itself (shown in green) is outlined in thick black lines, corresponding to its defining half great circles. The great circles bound three other lunes as well, and intersect at two polar opposite points, such as the North and South poles.

In spherical geometry, a lune is an area on a sphere bounded by two half great circles,[2] which is also called a digon or a diangle or (in German) a Zweieck. Great circles are the largest possible circles (circumferences) of a sphere; each one divides the surface of the sphere into two equal halves. Two great circles always intersect at two polar opposite points. Common examples of great quasi-circles are lines of longitude (meridians), which meet at the North and South Poles. Thus, the area between two meridians of longitude is a quasi-lune (slightly wider in the middle than a true lune due to the Earth being larger round the equator). The area of a spherical lune is 2θ R2, where R is the radius of the sphere and θ is the dihedral angle between the two half great circles. When this angle equals 2π — i.e., when the second half great circle has moved a full circle, and the lune in between covers the sphere — the area formula for the spherical lune gives 4πR2, the surface area of the sphere.

A hosohedron is a tessellation of the sphere by lunes. A n-gonal regular hosohedron has n equal lunes of π/n radians.

The crescent Moon is a spherical lune perceived as the intersection of a semicircle and semi-ellipse. Here, the blue and red portions may be taken equally as the sunlit and dark portions of the Moon visible from Earth or vice versa.

The lighted portion of the Moon visible from the Earth is a spherical lune. The first of the two intersecting great circles is the terminator between the sunlit half of the Moon and the dark half. The second great circle is a terrestrial terminator that separates the half visible from the Earth from the unseen half. This lighted, variable spherical (3D) lune is a crescent shape seen from Earth, the intersection of a semicircle and semi-ellipse (with the major axis of the ellipse coinciding with a diameter of the circle), as illustrated in the figure on the left.

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