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Spherical geometry

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Spherical geometry is the study of shapes on the surface of a sphere. While we usually think of geometry on flat planes, the rules change when a surface curves. This field, sometimes called spherics, examines two-dimensional surfaces of spheres or higher-dimensional spheres. It is essential for practical fields like astronomy, navigation, and geodesy. Scientists use these tools to understand the positions of stars and the shape of our planet.

Spherical triangle 3d
Spherical triangle 3d

To understand how this works, we must look at the basic building blocks. In flat Euclidean geometry, we use points and straight lines. In spherical geometry, the equivalent of a line is a great circle. A great circle is the intersection of a sphere with a plane passing through its center. You can also think of a great circle as a geodesic. A geodesic is the shortest path between two points on a curved surface.

Triangles (spherical geometry)
Triangles (spherical geometry)

These great circles behave differently than lines on a flat sheet of paper. On a plane, two lines might never meet if they are parallel. However, any two distinct great circles on a sphere will always intersect. They meet at exactly two points that are diametrically opposite each other. These points are called antipodal points. Because of this, spherical geometry does not follow the same rules as the geometry we learn in school. It is a type of non-Euclidean geometry.

One of the most striking differences involves the properties of triangles. In flat geometry, the interior angles of a triangle always sum to exactly 180 degrees. On a sphere, the sum of the angles of a spherical triangle is always greater than 180 degrees. This sum can actually reach up to 540 degrees. The specific sum depends on how much of the sphere's surface the triangle covers. If a triangle encloses a fraction of the surface, its angle sum increases accordingly.

Triangles (spherical geometry)
Triangles (spherical geometry)

History shows that many great thinkers have explored these curved surfaces. In the fourth century BC, Autolycus of Pitane wrote about the rotating sphere. Later, Greek mathematicians like Theodosius of Bithynia and Menelaus of Alexandria studied spherical trigonometry. Menelaus wrote a book called Sphaerica and developed Menelaus' theorem. In the Islamic world, Al-Jayyani wrote the Book of Unknown Arcs of a Sphere. This was the first treatise specifically on spherical trigonometry.

Spherical triangle 3d
Spherical triangle 3d

European mathematicians also contributed significantly to this field over the centuries. Around 1463, Regiomontanus wrote On Triangles, the first pure trigonometrical work in Europe. His work drew from the twelfth-century scholarship of Jabir ibn Aflah. Much later, the famous mathematician Leonhard Euler published many important memoirs. Between 1753 and 1815, Euler produced work on spherical trigonometry and the area of spherical triangles. His research helped formalize how we calculate measurements on curved objects.

Spherical geometry is closely related to other advanced mathematical concepts. It is a relative of elliptic geometry and hyperbolic geometry. These different systems arise from changing the parallel postulate, which is a fundamental rule in Euclidean math. Another connection is the real projective plane. This is created by identifying antipodal points on a sphere as being the same. While a sphere is easy to visualize in 3D space, the projective plane is non-orientable. This means it is a one-sided surface that cannot be drawn in 3D space without intersecting itself.

Triangles (spherical geometry)
Triangles (spherical geometry)
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