Chemistry, asked by dpadmaja4352, 9 months ago

Write a 200 word paper on the new developments, describing how these effect the telescopes, and in what environments these work best. Remember to cite any sources you use in your paper.

Answers

Answered by janakash992
2

Explanation:

The Development Of The Telescope And Auxiliary Instrumentation

Evolution of the optical telescope

Galileo is credited with having developed telescopes for astronomical observation in 1609. While the largest of his instruments was only about 120 cm (47 inches) long and had an objective diameter of 5 cm (2 inches), it was equipped with an eyepiece that provided an upright (i.e., erect) image. Galileo used his modest instrument to explore such celestial phenomena as the valleys and mountains of the Moon, the phases of Venus, and the four largest Jovian satellites, which had never been systematically observed before.

The Development Of The Telescope And Auxiliary Instrumentation

Evolution of the optical telescope

Galileo is credited with having developed telescopes for astronomical observation in 1609. While the largest of his instruments was only about 120 cm (47 inches) long and had an objective diameter of 5 cm (2 inches), it was equipped with an eyepiece that provided an upright (i.e., erect) image. Galileo used his modest instrument to explore such celestial phenomena as the valleys and mountains of the Moon, the phases of Venus, and the four largest Jovian satellites, which had never been systematically observed before.

The reflecting telescope was developed in 1668 by Newton, though John Gregory had independently conceived of an alternative reflector design in 1663. Cassegrain introduced another variation of the reflector in 1672. Near the end of the century, others attempted to construct refractors as long as 61 metres, but these instruments were too awkward to be effective.

The most significant contribution to the development of the telescope in the 18th century was that of Sir William Herschel. Herschel, whose interest in telescopes was kindled by a modest 5-cm Gregorian, persuaded the king of England to finance the construction of a reflector with a 12-metre (39-foot) focal length and a 120-cm mirror. Herschel is credited with having used this instrument to lay the observational groundwork for the concept of extragalactic “nebulas”—i.e., galaxies outside the Milky Way system.

Reflectors continued to evolve during the 19th century with the work of William Parsons, 3rd earl of Rosse, and William Lassell. In 1845 Lord Rosse constructed in Ireland a reflector with a 185-cm (73-inch) mirror and a focal length of about 16 metres (52 feet). For 75 years this telescope ranked as the largest in the world and was used to explore thousands of nebulae and star clusters. Lassell built several reflectors, the largest of which was on Malta; this instrument had a 124-cm (49-inch) primary mirror and a focal length of more than 10 metres (33 feet). His telescope had greater reflecting power than Rosse’s, and it enabled him to catalog 600 new nebulae as well as to discover several satellites of the outer planets—Triton (Neptune’s largest moon), Hyperion (Saturn’s 8th moon), and Ariel and Umbriel (two of Uranus’s moons).

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