telescope completed by him, and far exceeding in all respects any yet attempted, has an object fpeculum of forty feet focal length. The reflecting telescope, which is most in use y at prefent, is compofed of two concave mirrors of different radii. The larger concave AR (fig. 113) forms the focal image 1 m, which serves as an object for the fmall mirror K c: a fecond image im is formed by the mirror, the rays paffing through the amplifying lens L, which is placed in a hole or perforation in the center of the great mirror AR. This image is erect, and is viewed much enlarged through the eye-glafs or lens P. In good reflecting telescopes the object speculum z is not of a spherical form. Reflecting microscopes are fometimes made; A the method of conftructing which, as alfo of other inftruments, may be deduced from what has been faid concerning reflecting telescopes. END OF THE FIRST VOLUME. IN D E X то THE FIRST VOLUME ABERRATION, 254. Acceleration, 27. Achromatic telescope, 351. A Air, its colour, 297. want of transparency, 345. Alps, their colour, 297. Analogy, 2, 4. Analysis and fynthesis, 100, Animalculæ, 12, Aperture, 350. Aphelium, 122. Apogee, 122. Appearances, mutual, of the planets, 113-115, Archimedes, 319. Attraction, 7, 8, 25. wherein it differs from impulfe, 33: Axis and wheel, 60. B Balance, 59. Black, 61. Bradley, Dr. 249. 254. Buffon, his burning machine, 319. Camera C Camera obfcura, 346. Centripetal force, 94 & feq. 197 & feq. Clocks, 88 & feq. Clouds, why of fuch various colours, 297. a deception arif- Cobefion, 44 & feq. Cold, 16. Colour, wherein it consists, 271, 272. 292 & feq. Comets, 159-162. 167. their motion explained, 208. Creator, 50. III. Earth, proofs of its fpherical figure, 108-110. of its an- Eccentricity, 121. Eclipfe, 139, 145–158. Ecliptic, 123. 181. Effect and caufe, 4. 6. Elafticity, 41. Ellipfis, its defcription, 97. 122. Elongation, 105. 113-118. Equator, 181. measure of a degree at, 236. Equilibrium, |