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Summary of the development of the telescope

  • Early 13th century: Italian monks and scholars experimented with glass lenses to magnify text.

  • 1608: Hans Lippershey, a Dutch eyeglass maker, created the first refracting telescope using two lenses.

  • 1609: Galileo Galilei improved the design, making telescopes with up to 30x magnification for astronomical observations.

  • 1611: Johannes Kepler suggested using two convex lenses, enhancing image quality in refracting telescopes.

  • 1668: Isaac Newton invented the reflecting telescope, using mirrors instead of lenses to avoid chromatic aberration.

  • 18th century: Reflectors grew larger, with William Herschel building a 40-foot-long telescope by 1789.

  • 19th century: Achromatic lenses, developed by Chester Moor Hall and John Dollond, reduced colour distortion in refractors.

  • 1840s: Photography paired with telescopes, enabling permanent records of celestial objects.

  • 1897: The Yerkes Observatory’s 40-inch refractor became the largest working refracting telescope.

  • 1917: The 100-inch Hooker Telescope at Mount Wilson marked a leap in reflector size and power.

  • 1930s: Radio telescopes emerged, with Karl Jansky detecting cosmic radio waves.

  • 1940s-50s: Larger reflectors like the 200-inch Hale Telescope at Palomar improved light-gathering capability.

  • 1960s: Adaptive optics began correcting atmospheric distortion in real-time.

  • 1990: The Hubble Space Telescope launched, offering unprecedented views from space.

  • 2000s: Segmented mirrors, as in the Keck Observatory’s 10-meter telescopes, pushed size limits.

  • 2010s: The James Webb Space Telescope (launched 2021) used infrared to peer deeper into the universe.

  • Today: Giant projects like the Extremely Large Telescope (39-meter mirror) aim to explore exoplanets and dark energy.


 Definitions:


  • Refractor: A telescope that uses lenses to bend and focus light to form an image.

  • Convex lens: A lens thicker in the middle than at the edges, curving outward to converge light rays.

  • Chromatic aberration: A distortion where a lens fails to focus all colours of light at the same point, causing colour fringes.

  • Achromatic lens: A lens designed to minimize chromatic aberration by combining two types of glass with different dispersion properties.

  • Radio telescope: An instrument that collects and analyses radio waves from space to study celestial objects.

  • Atmospheric distortion: Blurring or twinkling of images caused by Earth’s atmosphere bending and scattering light.

  • Segmented mirror: A large telescope mirror made of smaller, hexagonal pieces fitted together to act as a single surface.

  • Exoplanet: A planet orbiting a star outside our solar system.

  • Dark energy: A mysterious force driving the accelerated expansion of the universe, making up most of its energy content.

 
 
 

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