— Ch. 1 · Origins And Early History —
Refracting telescope.
~4 min read · Ch. 1 of 6
In the month of May 1609, Galileo Galilei stood in Venice and heard news of a new invention from the Netherlands. A spectacle maker named Hans Lippershey had tried to patent a device that used lenses to magnify distant objects about three years earlier. The first record of such a telescope appeared around 1608 in Middelburg, but Lippershey failed to secure his patent rights. News traveled quickly across Europe, reaching Galileo while he was visiting the city of Venice. He constructed his own version using available glass and applied it to the study of the night sky. His most powerful instrument measured roughly five feet in length and could magnify objects thirty times. Despite poor lens technology, he used aperture stops to reduce blurriness and distortion. This early design allowed him to view craters on the Moon and observe four large moons orbiting Jupiter.
Evolution Of Lens Designs
Chester More Hall created the first twin color corrected lens in 1730 as an English barrister. John Dollond independently patented a similar achromatic design around 1758 after developing practical methods for mass production. These instruments combined crown glass with flint glass to bring red and blue wavelengths into focus simultaneously. The resulting telescopes were shorter than previous single-element models yet offered clearer images. Pierre-Louis Guinand developed better quality glass blanks exceeding ten centimeters in diameter during the late 1700s. Joseph von Fraunhofer learned this technique at Utzschiner's glassworks and later established his own optical company. By the end of the nineteenth century, refractors reached over one meter in aperture before being replaced by reflectors. Achromatic lenses became popular because they required less maintenance than metal mirrors and produced sharper views. Apochromatic designs emerged using fluorite or extra-low dispersion materials to correct three wavelengths instead of two.