In geometry, the exsphere of a face of a regular polyhedron is the sphere outside the polyhedron which touches the face and the planes defined by extending the adjacent faces outwards. It is tangent to the face externally and tangent to the adjacent faces internally.
It is the 3-dimensional equivalent of the excircle.
The sphere is more generally well-defined for any face which is a regular polygon and delimited by faces with the same dihedral angles at the shared edges. Faces of semi-regular polyhedra often have different types of faces, which define exspheres of different size with each type of face.
The exsphere touches the face of the regular polyedron at the center of the incircle of that face. If the exsphere radius is denoted rex, the radius of this incircle rin and the dihedral angle between the face and the extension of the adjacent face δ, the center of the exsphere is located from the viewpoint at the middle of one edge of the face by bisecting the dihedral angle. Therefore
δ is the 180-degree complement of the internal face-to-face angle.
Applied to the geometry of the Tetrahedron of edge length a, we have an incircle radius rin = a/(2√3) (derived by dividing twice the face area (a2√3)/4 through the perimeter 3a), a dihedral angle δ = π - arccos(1/3), and in consequence rex = a/√6.
The radius of the exspheres of the 6 faces of the Cube is the same as the radius of the inscribed sphere, since δ and its complement are the same, 90 degrees.
The dihedral angle applicable to the Icosahedron is derived by considering the coordinates of two triangles with a common edge, for example one face with vertices at
the other at
where g is the golden ratio. Subtracting vertex coordinates defines edge vectors,
of the first face and
of the other. Cross products of the edges of the first face and second face yield (not normalized) face normal vectors
of the first and
of the second face, using g2=1+g. The dot product between these two face normals yields the cosine of the dihedral angle,
For an icosahedron of edge length a, the incircle radius of the triangular faces is rin = a/(2√3), and finally the radius of the 20 exspheres
A centripetal force is a force that makes a body follow a curved path. Its direction is always orthogonal to the motion of the body and towards the fixed point of the instantaneous center of curvature of the path. Isaac Newton described it as "a force by which bodies are drawn or impelled, or in any way tend, towards a point as to a centre". In Newtonian mechanics, gravity provides the centripetal force causing astronomical orbits.
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