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A compendium of spherical astronomy with its applications to the determination and reduction of positions of the fixed stars (1906)

Newcomb, Simon, 1835-1909 · New York, The Macmillan company; London, Macmillan and co., ltd. · leaf 169

An illustration from A compendium of spherical astronomy with its applications to the determination and reduction of positions of the fixed stars, 1906, leaf 169
Fig. 15. When used without any other qualifying adjective, parallaxcommonly means the difference in the directions of a heavenlybody as seen from the point of reference, which may be thecentre of the earth or of the sun, and from some point ofobservation on the surface of the earth. … Fig. 16. Parallax in altitude is the difference between the geocentricand apparent altitude of a body. If in Fig. 16, P is the body,Q the point of observation, and 0 the centre of the earth, theparallax in altitude is the angle OPQ. If Q is so situated that the body is in its horizon, say at B,the…

Spherical astronomy · Stars

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