is more difficult to recognise owing to the fact that the sun and stars are not seen together.
As other motions of the celestial bodies have to be dealt with, the general motion just described may be conveniently referred to as the daily motion or daily rotation of the celestial sphere.
9. A further study of the daily motion would lead to the recognition of certain important circles of the celestial sphere.
Each star describes in its daily motion a circle, the size of which depends on its distance from the poles. Fig. 2 shews the paths described by a number of stars near the pole, recorded photographically, during part of a night. The pole-star describes so small a circle that its motion can only with difficulty be detected with the naked eye, stars a little farther off the pole describe larger circles, and so on, until we come to stars half-way between the two poles, which describe the largest circle which can be drawn on the celestial sphere. The circle on which these stars lie and which is described by any one of them daily is called the equator. By looking at a diagram such as fig. 3, or, better still, by looking at an actual globe, it can easily be seen that half the equator (e q w) lies above and half (the dotted part, w r e) below the horizon, and that in consequence a star, such as s, lying on the equator, is in its daily motion as long a time above the horizon as below. If a star, such as s, lies on the north side of the equator, i.e. on the side on which the north pole p lies, more than half of its daily path lies above the horizon and less than half (as shewn by the dotted line) lies below; and if a star is near enough to the north pole (more precisely, if it is nearer to the north pole than the nearest point, k, of the horizon), as σ, it never sets, but remains continually above the horizon. Such a star is called a (northern) circumpolar star. On the other hand, less than half of the daily path of a star on the south side of the equator, as s', is above the horizon, and a star, such as σ', the distance of which from the north pole is greater than the distance of the farthest point, h, of the horizon, or which is nearer than h to the south pole, remains continually below the horizon.
10. A slight familiarity with the stars is enough to shew any one that the same stars are not always visible at the
