SPHERE, in astronomy, a term for merly applied to any one of the concen tric and eccentric revolving transparent shells in which the heavenly bodies were supposed to be fixed, and by which they were carried so as to produce their ap parent motions. The word now signifies the vault of heaven, which to the eye seems the concave side of a hollow sphere, and on which the imaginary cir cles marking the positions of the equator, the ecliptic, etc., are supposed to be drawn. It is that portion of limit less space which the eye is powerful enough to penetrate, and appears a hol low sphere because the capacity of the eye for distant vision is equal in every direction.
In geometry, a solid or volume bounded by a surface, every point of which is equally distant from a point within, called the center. Or it is a volume that may be generated by re volving a semicircle about its diameter as an axis. The distance from any part of the surface to the center is called a radius of the sphere. Every section of a sphere made by a plane is a circle, and all sections made by planes equally dis tant from the center are equal. A cir cle of the sphere whose plane passes through the center is a great circle; all other circles are small circles. All great
circles are equal, and their radii are equal to the radii of the sphere. The surface of a sphere is equal to the product of the diameter by the circum ference of a great circle; or it is equiva lent to the area of four great circles. Denoting the radius of the sphere by r, and its diameter by d, we have the fol lowing formula for the surface: sr= 3 .14159 . .
The volume of a sphere is equal to the product of its surface by one-third of its radius. It is also equivalent to two thirds of the volume of its circumscrib ing cylinder. The following formula gives the value of the volume of any sphere, whose radius is r and diameter is d: v =71 pl.'. Spheres are to one an other as the cubes of their diameters.
In logic, the extension of a general conception; the individuals and species comprised in any general conception. The doctrine of the sphere is the appli cation of geometrical principles to geog raphy and astronomy. An oblique sphere, or spherical projection, is the projection made on the plane of the horizon of any place not on the equator or at the poles.