Editing Sphere

{{Short description|Set of points equidistant from a center}}
{{About|the concept in three-dimensional geometry}}
{{Distinguish|Ball (mathematics)}}
{{pp-move-indef}}
{{Use dmy dates|date=June 2021}}
{{Infobox polyhedron<!--Please add only parameters that make sense for a sphere.-->
| name         = Sphere
| image        = File:Sphere wireframe 10deg 6r.svg
| caption      = A [[3D projection#Perspective projection|perspective projection]] of a sphere
| euler        = 2
| symmetry     = [[Orthogonal group|{{math|O(3)}}]]
| surface_area = {{math|4πr<sup>2</sup>}}
| volume       = {{math|{{sfrac|4|3}}πr<sup>3</sup>}}
| type         = [[Smooth surface]]{{br}}[[Algebraic surface]]
}}

A '''sphere''' (from [[Ancient Greek|Greek]] {{wikt-lang|grc|σφαῖρα}}, {{grc-transl|σφαῖρα}})<ref>[https://www.perseus.tufts.edu/hopper/text?doc=Perseus%3Atext%3A1999.04.0057%3Aentry%3Dsfai%3Dra^ σφαῖρα], Henry George Liddell, Robert Scott, ''A Greek-English Lexicon'', on Perseus.</ref> is a [[surface (mathematics)|surface]] analogous to the [[circle]], a [[curve]]. In [[solid geometry]], a sphere is the [[Locus (mathematics)|set of points]] that are all at the same distance {{math|''r''}} from a given point in [[three-dimensional space]].<ref name=Albert54>{{harvnb|Albert|2016|loc=p. 54}}.</ref> That given point is the [[center (geometry)|''center'']] of the sphere, and the distance {{math|''r''}} is the sphere's ''[[radius]]''. The earliest known mentions of spheres appear in the work of the [[Greek mathematics|ancient Greek mathematicians]].

The sphere is a fundamental surface in many fields of [[mathematics]]. Spheres and nearly-spherical shapes also appear in nature and industry. [[Bubble (physics)|Bubble]]s such as [[soap bubble]]s take a spherical shape in equilibrium. The Earth is [[spherical Earth|often approximated as a sphere]] in [[geography]], and the [[celestial sphere]] is an important concept in [[astronomy]]. Manufactured items including [[pressure vessels]] and most [[curved mirror]]s and [[lens]]es are based on spheres. Spheres [[rolling|roll]] smoothly in any direction, so most [[ball]]s used in sports and toys are spherical, as are [[ball bearings]].

==Basic terminology==
[[File:Sphere and Ball.png|thumb|upright=1.1|Two orthogonal radii of a sphere]]

As mentioned earlier {{math|''r''}} is the sphere's radius; any line from the center to a point on the sphere is also called a radius. 'Radius' is used in two senses: as a line segment and also as its length.<ref name="EB" />

If a radius is extended through the center to the opposite side of the sphere, it creates a [[diameter]]. Like the radius, the length of a diameter is also called the diameter, and denoted {{math|''d''}}. Diameters are the longest line segments that can be drawn between two points on the sphere: their length is twice the radius, {{math|1=''d'' = 2''r''}}. Two points on the sphere connected by a diameter are [[antipodal point]]s of each other.<ref name="EB" />

A [[unit sphere]] is a sphere with unit radius ({{math|1=''r'' = 1}}). For convenience, spheres are often taken to have their center at the origin of the [[coordinate system]], and spheres in this article have their center at the origin unless a center is mentioned.

{{anchor|hemisphere}}
A ''[[great circle]]'' on the sphere has the same center and radius as the sphere, and divides it into two equal '''''hemispheres'''''.

Although the [[figure of Earth]] is not perfectly spherical, terms borrowed from geography are convenient to apply to the sphere.
A particular line passing through its center defines an ''[[Axis of symmetry|axis]]'' (as in Earth's [[axis of rotation]]).
The sphere-axis intersection defines two antipodal ''poles'' (''north pole'' and ''south pole''). The great circle equidistant to the poles is called the ''[[equator]]''. Great circles through the poles are called lines of [[longitude]] or [[meridian (geography)|''meridians'']]. Small circles on the sphere that are parallel to the equator are [[circle of latitude|circles of latitude]] (or ''parallels''). In geometry unrelated to astronomical bodies, geocentric terminology should be used only for illustration and noted as such, unless there is no chance of misunderstanding.<ref name="EB" />

Mathematicians consider a sphere to be a [[two-dimensional]] [[closed surface]] [[embedding|embedded]] in three-dimensional [[Euclidean space]]. They draw a distinction between a ''sphere'' and a ''[[Ball (mathematics)|ball]]'', which is a [[solid figure]], a three-dimensional [[manifold with boundary]] that includes the volume contained by the sphere. An ''open ball'' excludes the sphere itself, while a ''closed ball'' includes the sphere: a closed ball is the union of the open ball and the sphere, and a sphere is the [[Boundary (topology)|boundary]] of a (closed or open) ball. The distinction between ''ball'' and ''sphere'' has not always been maintained and especially older mathematical references talk about a sphere as a solid. The distinction between "[[circle]]" and "[[Disk (mathematics)|disk]]" in the [[Plane (geometry)|plane]] is similar.

Small spheres or balls are sometimes called ''spherules'' (e.g., in [[Martian spherules]]).

==Equations==
In [[analytic geometry]], a sphere with center {{math|(''x''<sub>0</sub>, ''y''<sub>0</sub>, ''z''<sub>0</sub>)}} and radius {{mvar|r}} is the [[Locus (mathematics)|locus]] of all points {{math|(''x'', ''y'', ''z'')}} such that
:<math> (x - x_0 )^2 + (y - y_0 )^2 + ( z - z_0 )^2 = r^2.</math>
Since it can be expressed as a quadratic polynomial, a sphere is a [[quadric surface]], a type of [[algebraic surface]].<ref name="EB" />

Let {{mvar|a, b, c, d, e}} be real numbers with {{math|''a'' ≠ 0}} and put
:<math>x_0 = \frac{-b}{a}, \quad y_0 = \frac{-c}{a}, \quad z_0 = \frac{-d}{a}, \quad \rho = \frac{b^2 +c^2+d^2 - ae}{a^2}.</math>
Then the equation
:<math>f(x,y,z) = a(x^2 + y^2 +z^2) + 2(bx + cy + dz) + e = 0</math>
has no real points as solutions if <math>\rho < 0</math> and is called the equation of an '''imaginary sphere'''. If <math>\rho = 0</math>, the only solution of <math>f(x,y,z) = 0</math> is the point <math>P_0 = (x_0,y_0,z_0)</math> and the equation is said to be the equation of a '''point sphere'''. Finally, in the case <math>\rho > 0</math>, <math>f(x,y,z) = 0</math> is an equation of a sphere whose center is <math>P_0</math> and whose radius is <math>\sqrt \rho</math>.<ref name=Albert54 />

If {{mvar|a}} in the above equation is zero then {{math|1=''f''(''x'', ''y'', ''z'') = 0}} is the equation of a plane. Thus, a plane may be thought of as a sphere of infinite radius whose center is a [[point at infinity]].<ref name=Woods266>{{harvnb|Woods|1961|loc=p. 266}}.</ref>

===Parametric===
A [[parametric equation]] for the sphere with radius <math>r > 0</math> and center <math>(x_0,y_0,z_0)</math> can be parameterized using [[trigonometric function]]s.
:<math>\begin{align}
x &= x_0 + r \sin \theta \; \cos\varphi \\
y &= y_0 + r \sin \theta \; \sin\varphi \\
z &= z_0 + r \cos \theta \,\end{align}</math><ref>{{harvtxt|Kreyszig|1972|p=342}}.</ref>

The symbols used here are the same as those used in [[spherical coordinates]]. {{mvar|r}} is constant, while {{mvar|θ}} varies from 0 to {{mvar|π}} and <math>\varphi</math> varies from 0 to 2{{mvar|π}}.

==Properties==
===Enclosed volume{{anchor|Volume}}===
[[File:Sphere and circumscribed cylinder.svg|thumb|upright=1.1|Sphere and circumscribed cylinder]]

In three dimensions, the [[volume]] inside a sphere (that is, the volume of a [[ball (mathematics)|ball]], but classically referred to as the volume of a sphere) is
:<math>V = \frac{4}{3}\pi r^3 = \frac{\pi}{6}\ d^3 \approx 0.5236 \cdot d^3</math>
where {{mvar|r}} is the radius and {{mvar|d}} is the diameter of the sphere. [[Archimedes]] first derived this formula (''[[On the Sphere and Cylinder]]'' c. 225 BCE) by showing that the volume inside a sphere is twice the volume between the sphere and the [[circumscribe]]d [[cylinder (geometry)|cylinder]] of that sphere (having the height and diameter equal to the diameter of the sphere).<ref>{{harvnb|Steinhaus|1969|loc=p. 223}}.</ref> This may be proved by inscribing a cone upside down into semi-sphere, noting that the area of a cross section of the cone plus the area of a cross section of the sphere is the same as the area of the cross section of the circumscribing cylinder, and applying [[Cavalieri's principle]].<ref>{{cite web|url=http://mathcentral.uregina.ca/QQ/database/QQ.09.01/rahul1.html|title=The volume of a sphere – Math Central|website=mathcentral.uregina.ca|access-date=2019-06-10}}</ref> This formula can also be derived using [[integral calculus]] (i.e., [[disk integration]]) to sum the volumes of an [[infinite number]] of [[Circle#Properties|circular]] disks of infinitesimally small thickness stacked side by side and centered along the {{mvar|x}}-axis from {{math|1=''x'' = −''r''}} to {{math|1=''x'' = ''r''}}, assuming the sphere of radius {{mvar|r}} is centered at the origin.
{{Collapse top|title=Proof of sphere volume, using calculus}}
At any given {{mvar|x}}, the incremental volume ({{mvar|δV}}) equals the product of the cross-sectional [[area of a disc#Onion proof|area of the disk]] at {{mvar|x}} and its thickness ({{mvar|δx}}):
:<math>\delta V \approx \pi y^2 \cdot \delta x.</math>

The total volume is the summation of all incremental volumes:
:<math>V \approx \sum \pi y^2 \cdot \delta x.</math>

In the limit as {{mvar|δx}} approaches zero,<ref name="delta"/> this equation becomes:
:<math>V = \int_{-r}^{r} \pi y^2 dx.</math>

At any given {{mvar|x}}, a right-angled triangle connects {{mvar|x}}, {{mvar|y}} and {{mvar|r}} to the origin; hence, applying the [[Pythagorean theorem]] yields:
:<math>y^2 = r^2 - x^2.</math>

Using this substitution gives
:<math>V = \int_{-r}^{r} \pi \left(r^2 - x^2\right)dx,</math>

which can be evaluated to give the result
:<math>V = \pi \left[r^2x - \frac{x^3}{3} \right]_{-r}^{r} = \pi \left(r^3 - \frac{r^3}{3} \right) - \pi \left(-r^3 + \frac{r^3}{3} \right) = \frac43\pi r^3.</math>

An alternative formula is found using [[spherical coordinates]], with [[volume element]]
:<math> dV=r^2\sin\theta\, dr\, d\theta\, d\varphi</math>
so
:<math>V=\int_0^{2\pi} \int_{0}^{\pi} \int_0^r r'^2\sin\theta\, dr'\, d\theta\, d\varphi
= 2\pi \int_{0}^{\pi} \int_0^r r'^2\sin\theta\, dr'\, d\theta
= 4\pi \int_0^r r'^2\, dr'\ =\frac43\pi r^3.</math>
{{Collapse bottom}}

For most practical purposes, the volume inside a sphere [[Inscribed figure|inscribed]] in a cube can be approximated as 52.4% of the volume of the cube, since {{math|1=''V'' = {{sfrac|{{pi}}|6}} ''d''<sup>3</sup>}}, where {{mvar|d}} is the diameter of the sphere and also the length of a side of the cube and {{sfrac|{{pi}}|6}}&nbsp;≈&nbsp;0.5236. For example, a sphere with diameter 1&nbsp;m has 52.4% the volume of a cube with edge length 1{{Spaces}}m, or about 0.524&nbsp;m<sup>3</sup>.

===Surface area{{anchor|Area}}===
<!--[[Surface area of a sphere]] is a redirect that points to this section.-->
The [[surface area]] of a sphere of radius {{mvar|r}} is:
:<math>A = 4\pi r^2.</math>

[[Archimedes]] first derived this formula<ref name=MathWorld_Sphere>{{MathWorld |title=Sphere |id=Sphere}}</ref> from the fact that the projection to the lateral surface of a [[circumscribe]]d cylinder is area-preserving.<ref>{{harvnb|Steinhaus|1969|loc=p. 221}}.</ref> Another approach to obtaining the formula comes from the fact that it equals the [[derivative]] of the formula for the volume with respect to {{mvar|r}} because the total volume inside a sphere of radius {{mvar|r}} can be thought of as the summation of the surface area of an infinite number of spherical shells of infinitesimal thickness concentrically stacked inside one another from radius 0 to radius {{mvar|r}}. At infinitesimal thickness the discrepancy between the inner and outer surface area of any given shell is infinitesimal, and the elemental volume at radius {{mvar|r}} is simply the product of the surface area at radius {{mvar|r}} and the infinitesimal thickness.

{{Collapse top|title=Proof of surface area, using calculus}}
At any given radius {{mvar|r}},{{NoteTag |{{mvar|r}} is being considered as a variable in this computation.}} the incremental volume ({{mvar|δV}}) equals the product of the surface area at radius {{mvar|r}} ({{math|''A''(''r'')}}) and the thickness of a shell ({{mvar|δr}}):
:<math>\delta V \approx A(r) \cdot \delta r. </math>

The total volume is the summation of all shell volumes:
:<math>V \approx \sum A(r) \cdot \delta r.</math>

In the limit as {{mvar|δr}} approaches zero<ref name="delta">{{cite book
|author1=E.J. Borowski |author2=J.M. Borwein |title=Collins Dictionary of Mathematics
|year=1989 |isbn=978-0-00-434347-1|pages=141, 149|publisher=Collins }}</ref> this equation becomes:
:<math>V = \int_0^r A(r) \, dr.</math>

Substitute {{mvar|V}}:
:<math>\frac43\pi r^3 = \int_0^r A(r) \, dr.</math>

Differentiating both sides of this equation with respect to {{mvar|r}} yields {{mvar|A}} as a function of {{mvar|r}}:
:<math>4\pi r^2 = A(r).</math>

This is generally abbreviated as:
:<math>A = 4\pi r^2,</math>
where {{mvar|r}} is now considered to be the fixed radius of the sphere.

Alternatively, the [[area element]] on the sphere is given in [[spherical coordinates]] by {{math|1=''dA'' = ''r''<sup>2</sup> sin ''θ dθ dφ''}}. The total area can thus be obtained by [[Integral|integration]]:
:<math>A = \int_0^{2\pi} \int_0^\pi r^2 \sin\theta \, d\theta \, d\varphi = 4\pi r^2.</math>
{{Collapse bottom}}

The sphere has the smallest surface area of all surfaces that enclose a given volume, and it encloses the largest volume among all closed surfaces with a given surface area.<ref>{{cite journal |last1=Osserman |first1=Robert |journal=Bulletin of the American Mathematical Society |title=The isoperimetric inequality |date=1978 |volume=84 |issue=6 |page=1187 |doi=10.1090/S0002-9904-1978-14553-4 |url=https://www.ams.org/journals/bull/1978-84-06/S0002-9904-1978-14553-4/ |access-date=14 December 2019 |ref=Osserman|doi-access=free }}</ref> The sphere therefore appears in nature: for example, bubbles and small water drops are roughly spherical because the [[surface tension]] locally minimizes surface area.

The surface area relative to the mass of a ball is called the [[specific surface area]] and can be expressed from the above stated equations as
:<math>\mathrm{SSA} = \frac{A}{V\rho} = \frac{3}{r\rho}</math>
where {{mvar|ρ}} is the [[density]] (the ratio of mass to volume).

===Other geometric properties===
A sphere can be constructed as the surface formed by rotating a [[circle]] one half revolution about any of its [[diameter]]s; this is very similar to the traditional definition of a sphere as given in [[Euclid's Elements]]. Since a circle is a special type of [[ellipse]], a sphere is a special type of [[ellipsoid of revolution]]. Replacing the circle with an ellipse rotated about its [[major axis]], the shape becomes a prolate [[spheroid]]; rotated about the minor axis, an oblate spheroid.<ref>{{harvnb|Albert|2016|loc=p. 60}}.</ref>

A sphere is uniquely determined by four points that are not [[coplanar]]. More generally, a sphere is uniquely determined by four conditions such as passing through a point, being tangent to a plane, etc.<ref>{{harvnb|Albert|2016|loc=p. 55}}.</ref> This property is analogous to the property that three [[collinear|non-collinear]] points determine a unique circle in a plane.

Consequently, a sphere is uniquely determined by (that is, passes through) a circle and a point not in the plane of that circle.

By examining the [[Circle of a sphere#Sphere-sphere intersection|common solutions of the equations of two spheres]], it can be seen that two spheres intersect in a circle and the plane containing that circle is called the '''radical plane''' of the intersecting spheres.<ref>{{harvnb|Albert|2016|loc=p. 57}}.</ref> Although the radical plane is a real plane, the circle may be imaginary (the spheres have no real point in common) or consist of a single point (the spheres are tangent at that point).<ref name=Woods267>{{harvnb|Woods|1961|loc=p. 267}}.</ref>

The angle between two spheres at a real point of intersection is the [[dihedral angle]] determined by the tangent planes to the spheres at that point. Two spheres intersect at the same angle at all points of their circle of intersection.<ref>{{harvnb|Albert|2016|loc=p. 58}}.</ref> They intersect at right angles (are [[Orthogonality|orthogonal]]) if and only if the square of the distance between their centers is equal to the sum of the squares of their radii.<ref name=Woods266 />

====Pencil of spheres====
{{Main|Pencil (mathematics)#Pencil of spheres}}
If {{math|1=''f''(''x'', ''y'', ''z'') = 0}} and {{math|1=''g''(''x'', ''y'', ''z'') = 0}} are the equations of two distinct spheres then
:<math>s f(x,y,z) + t g(x,y,z) = 0</math>
is also the equation of a sphere for arbitrary values of the parameters {{mvar|s}} and {{mvar|t}}. The set of all spheres satisfying this equation is called a '''pencil of spheres''' determined by the original two spheres. In this definition a sphere is allowed to be a plane (infinite radius, center at infinity) and if both the original spheres are planes then all the spheres of the pencil are planes, otherwise there is only one plane (the radical plane) in the pencil.<ref name=Woods266 />

===Properties of the sphere===
[[File:Sphere section.png|thumb|A normal vector to a sphere, a normal plane and its normal section. The curvature of the curve of intersection is the sectional curvature. For the sphere each normal section through a given point will be a circle of the same radius: the radius of the sphere. This means that every point on the sphere will be an umbilical point.]]

In their book ''Geometry and the Imagination'', [[David Hilbert]] and [[Stephan Cohn-Vossen]] describe eleven properties of the sphere and discuss whether these properties uniquely determine the sphere.<ref>{{cite book
|author1=Hilbert, David
|author-link=David Hilbert
|author2=Cohn-Vossen, Stephan
|title=Geometry and the Imagination
|url=https://archive.org/details/geometryimaginat00davi_0|url-access=registration|edition=2nd
|year=1952
|publisher=Chelsea
|isbn=978-0-8284-1087-8|chapter=Eleven properties of the sphere|pages=215–231}}</ref> Several properties hold for the [[plane (mathematics)|plane]], which can be thought of as a sphere with infinite radius. These properties are:
#''The points on the sphere are all the same distance from a fixed point. Also, the ratio of the distance of its points from two fixed points is constant.''
#: The first part is the usual definition of the sphere and determines it uniquely. The second part can be easily deduced and follows a similar [[Circle#Circle of Apollonius|result]] of [[Apollonius of Perga]] for the [[circle]]. This second part also holds for the [[plane (mathematics)|plane]].
#''The contours and plane sections of the sphere are circles.''
#: This property defines the sphere uniquely.
#''The sphere has constant width and constant girth.''
#: The width of a surface is the distance between pairs of parallel tangent planes. Numerous other closed convex surfaces have constant width, for example the [[Meissner body]]. The girth of a surface is the [[circumference]] of the boundary of its orthogonal projection on to a plane. Each of these properties implies the other.
#''All points of a sphere are [[umbilic]]s.''
#: At any point on a surface a [[Normal (geometry)|normal direction]] is at right angles to the surface because on the sphere these are the lines radiating out from the center of the sphere. The intersection of a plane that contains the normal with the surface will form a curve that is called a ''normal section,'' and the curvature of this curve is the ''normal curvature''. For most points on most surfaces, different sections will have different curvatures; the maximum and minimum values of these are called the [[principal curvature]]s. Any closed surface will have at least four points called ''[[umbilical point]]s''. At an umbilic all the sectional curvatures are equal; in particular the [[principal curvature]]s are equal. Umbilical points can be thought of as the points where the surface is closely approximated by a sphere.
#: For the sphere the curvatures of all normal sections are equal, so every point is an umbilic. The sphere and plane are the only surfaces with this property.
#''The sphere does not have a surface of centers.''
#: For a given normal section exists a circle of curvature that equals the sectional curvature, is tangent to the surface, and the center lines of which lie along on the normal line. For example, the two centers corresponding to the maximum and minimum sectional curvatures are called the ''focal points'', and the set of all such centers forms the [[focal surface]].
#: For most surfaces the focal surface forms two sheets that are each a surface and meet at umbilical points. Several cases are special:
#: * For [[channel surface]]s one sheet forms a curve and the other sheet is a surface
#: * For [[Cone (geometry)|cones]], cylinders, [[torus|tori]] and [[Dupin cyclide|cyclides]] both sheets form curves.
#: * For the sphere the center of every osculating circle is at the center of the sphere and the focal surface forms a single point. This property is unique to the sphere.
#''All geodesics of the sphere are closed curves.''
#: [[Geodesics]] are curves on a surface that give the shortest distance between two points. They are a generalization of the concept of a straight line in the plane. For the sphere the geodesics are great circles. Many other surfaces share this property.
#''Of all the solids having a given volume, the sphere is the one with the smallest surface area; of all solids having a given surface area, the sphere is the one having the greatest volume.''
#: It follows from [[isoperimetric inequality]]. These properties define the sphere uniquely and can be seen in [[soap bubble]]s: a soap bubble will enclose a fixed volume, and [[surface tension]] minimizes its surface area for that volume. A freely floating soap bubble therefore approximates a sphere (though such external forces as gravity will slightly distort the bubble's shape). It can also be seen in planets and stars where gravity minimizes surface area for large celestial bodies.
#''The sphere has the smallest total mean curvature among all convex solids with a given surface area.''
#: The [[mean curvature]] is the average of the two principal curvatures, which is constant because the two principal curvatures are constant at all points of the sphere.
#''The sphere has constant mean curvature.''
#: The sphere is the only [[Embedding|embedded]] surface that lacks boundary or singularities with constant positive mean curvature. Other such immersed surfaces as [[minimal surface]]s have constant mean curvature.
#''The sphere has constant positive Gaussian curvature.''
#: [[Gaussian curvature]] is the product of the two principal curvatures. It is an intrinsic property that can be determined by measuring length and angles and is independent of how the surface is [[embedding|embedded]] in space. Hence, bending a surface will not alter the Gaussian curvature, and other surfaces with constant positive Gaussian curvature can be obtained by cutting a small slit in the sphere and bending it. All these other surfaces would have boundaries, and the sphere is the only surface that lacks a boundary with constant, positive Gaussian curvature. The [[pseudosphere]] is an example of a surface with constant negative Gaussian curvature.
#''The sphere is transformed into itself by a three-parameter family of rigid motions.''
#: Rotating around any axis a unit sphere at the origin will map the sphere onto itself. Any rotation about a line through the origin can be expressed as a combination of rotations around the three-coordinate axis (see [[Euler angles]]). Therefore, a three-parameter family of rotations exists such that each rotation transforms the sphere onto itself; this family is the [[rotation group SO(3)]]. The plane is the only other surface with a three-parameter family of transformations (translations along the {{mvar|x}}- and {{mvar|y}}-axes and rotations around the origin). Circular cylinders are the only surfaces with two-parameter families of rigid motions and the [[Surface of revolution|surfaces of revolution]] and [[helicoid]]s are the only surfaces with a one-parameter family.

==Treatment by area of mathematics==
===Spherical geometry===
{{Main|Spherical geometry}}
[[File:Sphere halve.png|thumb|[[Great circle]] on a sphere]]

The basic elements of [[Euclidean plane geometry]] are [[Point (geometry)|points]] and [[line (mathematics)|lines]]. On the sphere, points are defined in the usual sense. The analogue of the "line" is the [[geodesic]], which is a [[great circle]]; the defining characteristic of a great circle is that the plane containing all its points also passes through the center of the sphere. Measuring by [[arc length]] shows that the shortest path between two points lying on the sphere is the shorter segment of the [[great circle]] that includes the points.

Many theorems from [[classical geometry]] hold true for spherical geometry as well, but not all do because the sphere fails to satisfy some of classical geometry's [[postulate]]s, including the [[parallel postulate]]. In [[spherical trigonometry]], [[angle]]s are defined between great circles. Spherical trigonometry differs from ordinary [[trigonometry]] in many respects. For example, the sum of the interior angles of a [[spherical triangle]] always exceeds 180&nbsp;degrees. Also, any two [[similar triangles|similar]] spherical triangles are congruent.

Any pair of points on a sphere that lie on a straight line through the sphere's center (i.e., the diameter) are called [[antipodal point|''antipodal points'']]{{snd}}on the sphere, the distance between them is exactly half the length of the circumference.{{NoteTag |group="Notes" |It does not matter which direction is chosen, the distance is the sphere's radius × ''π''.}} Any other (i.e., not antipodal) pair of distinct points on a sphere
*lie on a unique great circle,
*segment it into one minor (i.e., shorter) and one major (i.e., longer) [[Arc (geometry)|arc]], and
*have the minor arc's length be the ''shortest distance'' between them on the sphere.{{NoteTag |group="Notes" |The distance between two non-distinct points (i.e., a point and itself) on the sphere is zero.}}

Spherical geometry is a form of [[elliptic geometry]], which together with [[hyperbolic geometry]] makes up [[non-Euclidean geometry]].

===Differential geometry===
The sphere is a [[smooth surface]] with constant [[Gaussian curvature]] at each point equal to {{math|1/''r''<sup>2</sup>}}.<ref name=MathWorld_Sphere /> As per Gauss's [[Theorema Egregium]], this curvature is independent of the sphere's embedding in 3-dimensional space. Also following from Gauss, a sphere cannot be mapped to a plane while maintaining both areas and angles. Therefore, any [[map projection]] introduces some form of distortion.

A sphere of radius {{mvar|r}} has [[area element]] <math>dA = r^2 \sin \theta\, d\theta\, d\varphi</math>. This can be found from the [[volume element]] in [[spherical coordinates]] with {{mvar|r}} held constant.<ref name=MathWorld_Sphere />

A sphere of any radius centered at zero is an [[integral surface]] of the following [[differential form]]:
:<math> x \, dx + y \, dy + z \, dz = 0.</math>
This equation reflects that the position vector and [[tangent plane (geometry)|tangent plane]] at a point are always [[Orthogonality|orthogonal]] to each other. Furthermore, the outward-facing [[normal vector]] is equal to the position vector scaled by {{mvar|1/r}}.

In [[Riemannian geometry]], the [[filling area conjecture]] states that the hemisphere is the optimal (least area) isometric filling of the [[Riemannian circle]].

===Topology===
Remarkably, it is possible to turn an ordinary sphere inside out in a [[three-dimensional space]] with possible self-intersections but without creating any creases, in a process called [[sphere eversion]].

The antipodal quotient of the sphere is the surface called the [[real projective plane]], which can also be thought of as the [[Northern Hemisphere]] with antipodal points of the equator identified.

==Curves on a sphere {{anchor|Curves}}==
[[File:Ellipso-eb-ku.svg|upright=1.2|thumb|Plane section of a sphere: one circle]]
[[File:Kugel-zylinder-kk.svg|thumb|Coaxial intersection of a sphere and a cylinder: two circles]]

===Circles===
{{Main|Circle of a sphere}}
Circles on the sphere are, like circles in the plane, made up of all points a certain distance from a fixed point on the sphere. The intersection of a sphere and a plane is a circle, a point, or empty.<ref>{{MathWorld |id=SphericSection |title=Spheric section}}</ref> Great circles are the intersection of the sphere with a plane passing through the center of a sphere: others are called small circles.

More complicated surfaces may intersect a sphere in circles, too: the intersection of a sphere with a [[surface of revolution]] whose axis contains the center of the sphere (are ''coaxial'') consists of circles and/or points if not empty. For example, the diagram to the right shows the intersection of a sphere and a cylinder, which consists of two circles. If the cylinder radius were that of the sphere, the intersection would be a single circle. If the cylinder radius were larger than that of the sphere, the intersection would be empty.

===Loxodrome===
{{Main|Rhumb line}}
[[File:Loxodrome.png|thumb|upright=0.5|Loxodrome]]

In [[navigation]], a ''loxodrome'' or ''rhumb line'' is a path whose [[bearing (navigation)|bearing]], the angle between its tangent and due North, is constant. Loxodromes project to straight lines under the [[Mercator projection]]. Two special cases are the [[meridian (geography)|meridians]] which are aligned directly North–South and [[circle of latitude|parallels]] which are aligned directly East–West. For any other bearing, a loxodrome spirals infinitely around each pole. For the Earth modeled as a sphere, or for a general sphere given a [[spherical coordinate system]], such a loxodrome is a kind of [[spherical spiral]].<ref>{{cite web | url=https://mathworld.wolfram.com/Loxodrome.html | title=Loxodrome }}</ref>

===Clelia curves===
{{Main|Clélie}}
[[File:Kugel-spirale-1-2.svg|thumb|upright=0.8|Clelia spiral with {{math|1=''c'' = 8}}]]

Another kind of spherical spiral is the Clelia curve, for which the [[longitude]] (or azimuth) <math>\varphi</math> and the [[colatitude]] (or polar angle) <math>\theta</math> are in a linear relationship, {{tmath|1=\varphi = c\theta}}. Clelia curves project to straight lines under the [[equirectangular projection]]. [[Viviani's curve]] ({{tmath|1=c=1}}) is a special case. Clelia curves approximate the [[ground track]] of satellites in [[polar orbit]].

===Spherical conics===
{{Main|Spherical conic}}
The analog of a [[conic section]] on the sphere is a [[spherical conic]], a [[quartic function|quartic]] curve which can be defined in several equivalent ways.
*The intersection of a sphere with a quadratic cone whose vertex is the sphere center
*The intersection of a sphere with an [[cylinder#cylindrical surfaces|elliptic or hyperbolic cylinder]] whose axis passes through the sphere center
*The locus of points whose sum or difference of [[great-circle distance]]s from a pair of [[focus (geometry)|foci]] is a constant

Many theorems relating to planar conic sections also extend to spherical conics.

===Intersection of a sphere with a more general surface===
[[File:Is-spherecyl5-s.svg|thumb|upright=0.8|General intersection sphere-cylinder]]

If a sphere is intersected by another surface, there may be more complicated spherical curves.
;Example: sphere–cylinder
{{Main|Sphere–cylinder intersection}}
The intersection of the sphere with equation <math>\; x^2+y^2+z^2=r^2\;</math> and the cylinder with equation <math> \;(y-y_0)^2+z^2=a^2, \; y_0\ne 0\; </math> is not just one or two circles. It is the solution of the non-linear system of equations
:<math>x^2+y^2+z^2-r^2=0</math>
:<math>(y-y_0)^2+z^2-a^2=0\ .</math>
(see [[implicit curve]] and the diagram)

==Generalizations==
===Ellipsoids===
An [[ellipsoid]] is a sphere that has been stretched or compressed in one or more directions. More exactly, it is the image of a sphere under an [[affine transformation]]. An ellipsoid bears the same relationship to the sphere that an [[ellipse]] does to a circle.

===Dimensionality===
{{Main|n-sphere}}
Spheres can be generalized to spaces of any number of [[dimension]]s. For any [[natural number]] {{mvar|n}}, an ''{{mvar|n}}-sphere,'' often denoted {{math|''S''{{px2}}<sup>''n''</sup>}}, is the set of points in ({{math|''n'' + 1}})-dimensional Euclidean space that are at a fixed distance {{mvar|r}} from a central point of that space, where {{mvar|r}} is, as before, a positive real number. In particular:
*{{math|''S''{{px2}}<sup>0</sup>}}: a 0-sphere consists of two discrete points, {{math|−''r''}} and {{math|''r''}}
*{{math|''S''{{px2}}<sup>1</sup>}}: a 1-sphere is a [[circle]] of radius ''r''
*{{math|''S''{{px2}}<sup>2</sup>}}: a 2-sphere is an ordinary sphere
*{{math|''S''{{px2}}<sup>3</sup>}}: a [[3-sphere]] is a sphere in 4-dimensional Euclidean space.

Spheres for {{math|''n'' > 2}} are sometimes called [[hypersphere]]s.

The {{mvar|n}}-sphere of unit radius centered at the origin is denoted {{math|''S''{{px2}}<sup>''n''</sup>}} and is often referred to as "the" {{mvar|n}}-sphere. The ordinary sphere is a 2-sphere, because it is a 2-dimensional surface which is embedded in 3-dimensional space.

In [[topology]], the {{mvar|n}}-sphere is an example of a [[compact space|compact]] [[topological manifold]] without [[Boundary (topology)|boundary]]. A topological sphere need not be [[Manifold#Differentiable manifolds|smooth]]; if it is smooth, it need not be [[diffeomorphic]] to the Euclidean sphere (an [[exotic sphere]]).

The sphere is the inverse image of a one-point set under the continuous function {{math|{{norm|''x''}}}}, so it is closed; {{math|''S<sup>n</sup>''}} is also bounded, so it is compact by the [[Heine–Borel theorem]].

===Metric spaces===
{{Main|Metric space}}
More generally, in a [[metric space]] {{math|(''E'',''d'')}}, the sphere of center {{mvar|x}} and radius {{math|''r'' > 0}} is the set of points {{mvar|y}} such that {{math|1=''d''(''x'',''y'') = ''r''}}.

If the center is a distinguished point that is considered to be the origin of {{mvar|E}}, as in a [[norm (mathematics)|normed]] space, it is not mentioned in the definition and notation. The same applies for the radius if it is taken to equal one, as in the case of a [[unit sphere]].

Unlike a [[ball (mathematics)|ball]], even a large sphere may be an empty set. For example, in {{math|'''Z'''<sup>''n''</sup>}} with [[Euclidean metric]], a sphere of radius {{math|''r''}} is nonempty only if {{math|''r''<sup>2</sup>}} can be written as sum of {{math|''n''}} squares of [[integer]]s.

An [[octahedron]] is a sphere in [[taxicab geometry]], and a [[cube]] is a sphere in geometry using the [[Chebyshev distance]].

==History==
The geometry of the sphere was studied by the Greeks. ''[[Euclid's Elements]]'' defines the sphere in book XI, discusses various properties of the sphere in book XII, and shows how to inscribe the five regular polyhedra within a sphere in book XIII. Euclid does not include the area and volume of a sphere, only a theorem that the volume of a sphere varies as the third power of its diameter, probably due to [[Eudoxus of Cnidus]]. The volume and area formulas were first determined in [[Archimedes]]'s ''[[On the Sphere and Cylinder]]'' by the [[method of exhaustion]]. [[Zenodorus (mathematician)|Zenodorus]] was the first to state that, for a given surface area, the sphere is the solid of maximum volume.<ref name="EB">{{Cite EB1911|wstitle=Sphere |volume=25 |pages=647–648 }}</ref>

Archimedes wrote about the problem of dividing a sphere into segments whose volumes are in a given ratio, but did not solve it. A solution by means of the parabola and hyperbola was given by [[Dionysodorus]].<ref>{{Cite web |last=Fried |first=Michael N. |date=2019-02-25 |title=conic sections |url=https://oxfordre.com/view/10.1093/acrefore/9780199381135.001.0001/acrefore-9780199381135-e-8161 |access-date=2022-11-04 |website=Oxford Research Encyclopedia of Classics |language=en |doi=10.1093/acrefore/9780199381135.013.8161|isbn=978-0-19-938113-5 |quote=More significantly, Vitruvius (On Architecture, Vitr. 9.8) associated conical sundials with Dionysodorus (early 2nd century bce), and Dionysodorus, according to Eutocius of Ascalon (c. 480–540 ce), used conic sections to complete a solution for Archimedes’ problem of cutting a sphere by a plane so that the ratio of the resulting volumes would be the same as a given ratio.}}</ref> A similar problem{{snd}}to construct a segment equal in volume to a given segment, and in surface to another segment{{snd}}was solved later by [[al-Quhi]].<ref name="EB" />

==Gallery==
<gallery mode="packed" heights="200" style="text-align:left">
File:Einstein gyro gravity probe b.jpg|An image of one of the most accurate human-made spheres, as it [[refraction|refracts]] the image of [[Albert Einstein|Einstein]] in the background. This sphere was a [[fused quartz]] [[gyroscope]] for the [[Gravity Probe B]] experiment, and differs in shape from a perfect sphere by no more than 40 atoms (less than 10{{Spaces}}nm) of thickness. It was announced on 1 July 2008 that [[Australia]]n scientists had created even more nearly perfect spheres, accurate to 0.3{{Spaces}}nm, as part of an international hunt [[Alternative approaches to redefining the kilogram#Alternative approaches to redefining the kilogram|to find a new global standard kilogram]].<ref>[https://www.newscientist.com/article/dn14229-roundest-objects-in-the-world-created.html New Scientist | Technology | Roundest objects in the world created].</ref>
File:King of spades- spheres.jpg|Deck of playing cards illustrating engineering instruments, England, 1702. [[King of spades]]: Spheres
</gallery>

==Regions==
{{see also|Ball (mathematics)#Regions}}
{{div col||colwidth=20em}}
*Hemisphere
*[[Spherical cap]]
*[[Spherical lune]]
*[[Spherical polygon]]
*[[Spherical sector]]
*[[Spherical segment]]
*[[Spherical wedge]]
*[[Spherical zone]]
{{div col end}}

==See also==
{{div col||colwidth=20em}}
*[[3-sphere]]
*[[Affine sphere]]
*[[Alexander horned sphere]]
*[[Celestial spheres]]
*[[Curvature]]
*[[Directional statistics]]
*[[Dyson sphere]]
*[[Gauss map]]
*[[Hand with Reflecting Sphere]], [[M.C. Escher]] self-portrait drawing illustrating reflection and the optical properties of a mirror sphere
*[[Hoberman sphere]]
*[[Homology sphere]]
*[[Homotopy groups of spheres]]
*[[Homotopy sphere]]
*[[Lenart Sphere]]
*[[Napkin ring problem]]
*[[Orb (optics)]]
*[[Pseudosphere]]
*[[Riemann sphere]]
*[[Solid angle]]
*[[Sphere packing]]
*[[Spherical coordinates]]
*[[Spherical cow]]
*Spherical helix, [[tangent indicatrix]] of a curve of constant precession
*[[Spherical polyhedron]]
*[[Sphericity]]
*[[Tennis ball theorem]]
*[[Volume-equivalent radius]]
*[[Zoll surface|Zoll sphere]]
{{div col end}}

==Notes and references==
===Notes===
{{NoteFoot}}

===References===
{{Reflist}}

===Further reading===
{{Wikisource1911Enc|Sphere}}
{{Sister project links}}
*{{citation|first=Abraham Adrian|last=Albert|title=Solid Analytic Geometry|year=2016|orig-year=1949|publisher=Dover|isbn=978-0-486-81026-3}}.
*{{cite book|first=William |last=Dunham |pages=[https://archive.org/details/mathematicaluniv00dunh/page/n34 28], 226 |title=The Mathematical Universe: An Alphabetical Journey Through the Great Proofs, Problems and Personalities |url=https://archive.org/details/mathematicaluniv00dunh |url-access=limited |publisher= Wiley|location=New York |isbn=978-0-471-17661-9 |year=1997 |bibcode=1994muaa.book.....D }}
*{{citation | first1 = Erwin | last1 = Kreyszig | year = 1972 | isbn = 978-0-471-50728-4 | title = Advanced Engineering Mathematics | edition = 3rd | publisher = [[John Wiley & Sons|Wiley]] | location = New York | url-access = registration | url = https://archive.org/details/advancedengineer00krey }}.
*{{citation|first=H.|last=Steinhaus|title=Mathematical Snapshots|year=1969|publisher=Oxford University Press|edition=Third American}}.
*{{citation|first=Frederick S.|last=Woods|title=Higher Geometry / An Introduction to Advanced Methods in Analytic Geometry|year=1961|orig-year=1922|publisher=Dover}}.
*{{Cite web|title=The Geometry of the Sphere |url=https://www.math.csi.cuny.edu/~ikofman/Polking/sphere.html#basic|access-date=2022-01-21|website=www.math.csi.cuny.edu|author=John C. Polking|date=1999-04-15}}

==External links==
*[[b:Mathematica/Uniform Spherical Distribution|Mathematica/Uniform Spherical Distribution]]
*[http://mathschallenge.net/index.php?section=faq&ref=geometry/surface_sphere Surface area of sphere proof]
{{Compact topological surfaces}}
{{Authority control}}

[[Category:Differential geometry]]
[[Category:Differential topology]]
[[Category:Elementary geometry]]
[[Category:Elementary shapes]]
[[Category:Homogeneous spaces]]
[[Category:Spheres| ]]
[[Category:Surfaces]]
[[Category:Topology]]