A telescope is a device used to observe distant objects. Originally, telescopes were optical instruments using lenses and mirrors to observe visible light. Today, the term "telescope" encompasses a broader range of instruments that can detect various forms of electromagnetic radiation beyond the visible spectrum. Some telescopes even utilize detectors beyond those used for electromagnetic radiation.
In 1932, a significant advancement in telescope technology occurred with the introduction of aluminized mirrors. This innovation addressed the problem of fast tarnishing in reflecting telescopes, which had previously relied on silver-coated glass mirrors.
The year 1937 marked a pivotal moment in astronomical observation with the commencement of operations for the first purpose-built radio telescope. This event expanded the horizons of astronomy beyond the visible spectrum.
In 1952, Hans Wolter proposed three innovative methods for constructing telescopes using ring-shaped "glancing" mirrors made from heavy metals. These designs revolutionized X-ray astronomy by enabling the reflection and focusing of X-rays.
By 2005, astronomical interferometers, using multiple dishes to create a 'virtual' telescope, reached a milestone. Using space-based very-long-baseline interferometry (VLBI), such as the Japanese HALCA and VSOP satellites, arrays achieved virtual apertures several times larger than Earth, significantly increasing resolution for observing distant objects.
June 2008 saw the launch of the Fermi Gamma-ray Space Telescope, a significant development in our ability to observe the universe in gamma rays. The Earth's atmosphere is opaque to gamma rays, necessitating space-based telescopes like Fermi.
A groundbreaking discovery in 2012 revealed that the index of refraction for photons starts to increase again at energies exceeding 700 keV. This finding opened up new possibilities for developing gamma-ray telescopes capable of focusing these high-energy photons.
The launch of the NuSTAR X-ray Telescope in 2012 marked a significant step in X-ray astronomy. The telescope, employing Wolter telescope design optics on a deployable mast, allowed scientists to study high-energy photons up to 79 keV.
On December 25, 2021, NASA launched the James Webb Space Telescope, a groundbreaking observatory designed to detect infrared light. The launch took place in Kourou, French Guiana, marking a new era in space exploration and infrared astronomy.