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  1. The first record of a telescope comes from the Netherlands in 1608. It is in a patent filed by Middelburg spectacle-maker Hans Lippershey with the States General of the Netherlands on 2 October 1608 for his instrument " for seeing things far away as if they were nearby.

  2. Historia. Pierwsze znane praktyczne teleskopy zostały skonstruowane przy użyciu szklanych soczewek w Holandii na początku XVII wieku przez Hansa Lipperheya, a wkrótce potem przez Galileusza we Włoszech. Znalazły one zastosowanie w działaniach militarnych i w astronomii.

  3. en.wikipedia.org › wiki › TelescopeTelescope - Wikipedia

    The reflecting telescope, which uses mirrors to collect and focus light, was invented within a few decades of the first refracting telescope. In the 20th century, many new types of telescopes were invented, including radio telescopes in the 1930s and infrared telescopes in the 1960s.

  4. The following timeline lists the significant events in the invention and development of the telescope. BC. 2560 BC to 1 BC. c.2560 BC–c.860 BC — Egyptian artisans polish rock crystal, semi-precious stones, and latterly glass to produce facsimile eyes for statuary and mummy cases. The intent appears to be to produce an optical illusion. [1][2][3]

  5. 2005 – First light at SALT, the largest optical telescope in the Southern Hemisphere, with a hexagonal primary mirror of 11.1 by 9.8 meters. 2007 – First light at Gran Telescopio de Canarias (GTC), in Spain, the largest optical telescope in the world with an effective diameter of 10.4 meters.

  6. An optical telescope is a telescope that gathers and focuses light mainly from the visible part of the electromagnetic spectrum, to create a magnified image for direct visual inspection, to make a photograph, or to collect data through electronic image sensors. There are three primary types of optical telescope:

  7. 12 paź 2024 · telescope, device used to form magnified images of distant objects. The telescope is undoubtedly the most important investigative tool in astronomy. It provides a means of collecting and analyzing radiation from celestial objects, even those in the far reaches of the universe.

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