Toward the middle of the seventeenth century the reflecting telescope had been so much improved as nearly to crowd out its refracting rival, but, just as its success seemed to be assured, Dollond, working along lines partially followed up by Hall, found a combination of lenses by which the chromatic aberration of the refractor could be very perfectly corrected. While Dollond's invention was of immense value, it remained that flint object glasses larger than two and one-half inches in diameter could not, for some years, be manufactured, but about the opening of the nineteenth century, Guinand, a Swiss, discovered a process of making masses of optical flint glass sufficiently large as to admit of the construction from them of excellent lenses of sizes gradually increasing as time and experimenting went on. The making of three-inch objectives, achromatic and of short focus, wrought a revolution in telescopes and renewed the demand for refractors, though prices, as compared with those of the present day, were very great. But improvement was succeeded by improvement. Larger and still larger objectives were made, yet progress was not so rapid as not to justify Grant, in 1852, in declaring to be a "munificent gift" the presentation, about 1838, to Greenwhich Observatory, of a six and seven-tenths object glass alone, and so it was esteemed by Mr. Airy, the astronomer royal. Improvement is still the order of the day, and, as a result of keen competition, very excellent telescopes of small aperture can be purchased at reasonable prices. Great telescopes are enormously expensive, and will probably be so until they are superseded by some simple invention which shall be as superior to them as they are to the "mighty" instruments which, from time to time, caused such sensations in the days of Galilei, Cassini, Huyghens, Bradley, Dollond, and those who came after them.