A telescope placed in space to observe astronomical objects without atmospheric interference.A space telescope is an observatory placed beyond Earth's atmosphere to capture astronomical images and spectra without the distortions and absorption caused by air. The atmosphere blocks most ultraviolet and infrared light, and it causes visible light to twinkle and blur. By operating in space, telescopes like Hubble and James Webb achieve diffraction-limited resolution and access wavelengths that never reach the ground. This has enabled discoveries from exoplanet atmospheres to the most distant galaxies, fundamentally changing our view of the cosmos.
The concept was proposed by Lyman Spitzer in 1946, leading to the launch of the Hubble Space Telescope in 1990. Earlier, the Orbiting Astronomical Observatory (1968) and the International Ultraviolet Explorer (1978) pioneered space-based astronomy.
Space telescopes use mirrors and detectors similar to ground-based ones, but they are launched into orbit or at Lagrange points. They maintain precise pointing using reaction wheels and star trackers, and they often include cryogenic cooling to reduce thermal noise for infrared observations. Data is transmitted to Earth via radio links, where it is processed and analyzed. The absence of atmospheric turbulence allows the telescope to reach its theoretical resolution limit.
Space telescopes are used for cosmology, exoplanet characterization, and monitoring space weather. They also serve as testbeds for technologies like adaptive optics and precision pointing systems.
The Hubble Space Telescope has observed the same patch of sky for over 20 years, creating the Hubble Ultra-Deep Field, which contains thousands of galaxies from when the universe was less than a billion years old.




