List of space telescopes
This list of space telescopes is grouped by major frequency ranges: gamma ray, X-ray, ultraviolet, visible, infrared, microwave and radio. Telescopes that work in multiple frequency bands are included in all of the appropriate sections. Space telescopes that collect particles, such as cosmic ray nuclei and/or electrons, as well as instruments that aim to detect gravitational waves, are also listed. Missions with specific targets within the Solar System, are excluded; see List of Solar System probes and List of heliophysics missions for these, and List of Earth observation satellites for missions targeting Earth.
Two values are provided for the dimensions of the initial orbit. For telescopes in Earth orbit, the minimum and maximum altitude are given in kilometers. For telescopes in solar orbit, the minimum distance and the maximum distance between the telescope and the center of mass of the Sun are given in astronomical units.
Gamma ray
Gamma-ray telescopes collect and measure individual, high energy gamma rays from astrophysical sources. These are absorbed by the atmosphere, requiring that observations are done by high-altitude balloons or space missions. Gamma rays can be generated by supernovae, neutron stars, pulsars and black holes. Gamma ray bursts, with extremely high energies, have also been detected but have yet to be identified.| Photo | Name | Space agency | Launch date | Terminated | Location | Ref |
| Proton-1 | USSR | Earth orbit | ||||
| Proton-2 | USSR | Earth orbit | ||||
| Proton-4 | USSR | Earth orbit | ||||
| Small Astronomy Satellite 2 | NASA | Earth orbit | ||||
| Cos-B | ESA | Earth orbit | ||||
| High Energy Astronomy Observatory 3 | NASA | Earth orbit | ||||
| Granat | CNRS & IKI | Earth orbit | ||||
| Gamma | USSR, CNES, RSA | Earth orbit | ||||
| Compton Gamma Ray Observatory | NASA | Earth orbit | ||||
| Low Energy Gamma Ray Imager | INTA | Earth orbit | ||||
| High Energy Transient Explorer 2 | NASA | Earth orbit | ||||
| International Gamma Ray Astrophysics Laboratory | ESA | Earth orbit | ||||
| Neil Gehrels Swift Observatory | NASA | — | Earth orbit | |||
| Astrorivelatore Gamma ad Immagini Leggero | ISA | 18 | Earth orbit | |||
| Fermi Gamma-ray Space Telescope | NASA | — | Earth orbit | |||
| Gamma-Ray Burst Polarimeter | JAXA | 21 May 2015 | Heliocentric orbit | |||
| Space Variable Objects Monitor | CNSA & CNES | — | Earth orbit |
X-ray
s measure high-energy photons called X-rays. These can not travel a long distance through the atmosphere, meaning that they can only be observed high in the atmosphere or in space. Several types of astrophysical objects emit X-rays, from galaxy clusters, through black holes in active galactic nuclei to galactic objects such as supernova remnants, stars, and binary stars containing a white dwarf, neutron star or black hole. Some Solar System bodies emit X-rays, the most notable being the Moon, although most of the X-ray brightness of the Moon arises from reflected solar X-rays. A combination of many unresolved X-ray sources is thought to produce the observed X-ray background.| Photo | Name | Space agency | Launch date | Terminated | Location | Ref |
| Uhuru | NASA | Earth orbit | ||||
| Astronomical Netherlands Satellite | SRON | Earth orbit | ||||
| Ariel V | SRC & NASA | Earth orbit | ||||
| Aryabhata | ISRO | Earth orbit | ||||
| Small Astronomy Satellite 3 | NASA | Earth orbit | ||||
| Cos-B | ESA | Earth orbit | ||||
| Cosmic Radiation Satellite | ISAS | Failed launch | ||||
| High Energy Astronomy Observatory 1 | NASA | Earth orbit | ||||
| Einstein Observatory | NASA | Earth orbit | ||||
| Hakucho | ISAS | Earth orbit | ||||
| High Energy Astronomy Observatory 3 | NASA | Earth orbit | ||||
| Tenma | ISAS | Earth orbit | ||||
| Astron | IKI | Earth orbit | ||||
| EXOSAT | ESA | Earth orbit | ||||
| Ginga | ISAS | Earth orbit | ||||
| Granat | CNRS & IKI | Earth orbit | ||||
| ROSAT | NASA & DLR | Re-entry 23 October 2011. Formerly Earth orbit | ||||
| Broad Band X-ray Telescope / Astro 1 | NASA | Earth orbit | ||||
| Advanced Satellite for Cosmology and Astrophysics | ISAS & NASA | Earth orbit | ||||
| Array of Low Energy X-ray Imaging Sensors | LANL | Earth orbit | ||||
| Rossi X-ray Timing Explorer | NASA | Earth orbit | ||||
| BeppoSAX | ASI | Earth orbit | ||||
| A Broadband Imaging X-ray All-sky Survey | DLR | Earth orbit | ||||
| Chandra X-ray Observatory | NASA | — | Earth orbit | |||
| XMM-Newton | ESA | — | Earth orbit | |||
| High Energy Transient Explorer 2 | NASA | Earth orbit | ||||
| International Gamma Ray Astrophysics Laboratory | ESA | Earth orbit | ||||
| Neil Gehrels Swift Observatory | NASA | — | Earth orbit | |||
| Suzaku | JAXA & NASA | Earth orbit | ||||
| Astrorivelatore Gamma ad Immagini Leggero | ISA | 18 | Earth orbit | |||
| Nuclear Spectroscopic Telescope Array | NASA | — | Earth orbit | |||
| AstroSat | ISRO | — | Earth orbit | |||
| Hitomi | JAXA | Earth orbit | ||||
| Mikhailo Lomonosov | Moscow State University | Earth orbit | ||||
| Neutron Star Interior Composition Explorer | NASA | — | International Space Station | |||
| Hard X-ray Modulation Telescope | CNSA & CAS | — | Low Earth orbit | |||
| Spektr-RG | RSRI & MPE | — | Sun-Earth L2 | |||
| Imaging X-ray Polarimetry Explorer | NASA | — | Earth orbit | |||
| Lobster Eye Imager for Astronomy | CAS | — | Low Earth orbit | |||
| X-ray Imaging and Spectroscopy Mission | JAXA & NASA | — | Earth orbit | |||
| X-ray Polarimeter Satellite | ISRO & RRI | — | Earth orbit | |||
| Einstein Probe | CAS & ESA & MPE | — | Earth orbit | |||
| Space Variable Objects Monitor | CNSA & CNES | — | Earth orbit | |||
| BlackCAT | NASA | — | Geocentric orbit |
Ultraviolet
Ultraviolet telescopes make observations at ultraviolet wavelengths, i.e. between approximately 10 and 320 nm. Light at these wavelengths is absorbed by the Earth's atmosphere, so observations at these wavelengths must be performed from the upper atmosphere or from space. Objects emitting ultraviolet radiation include the Sun, other stars and galaxies.| Photo | Name | Space agency | Launch date | Terminated | Observing location | Ref |
| OAO-2 | NASA | Earth orbit | ||||
| Orion 1 and Orion 2 Space Observatories | USSR | ; | ; 1973 | Earth orbit | ||
| Far Ultraviolet Camera/Spectrograph | NASA | Descartes Highlands on lunar surface | ||||
| OAO-3 Copernicus | NASA | Earth orbit | ||||
| Astronomical Netherlands Satellite | SRON | Earth orbit | ||||
| International Ultraviolet Explorer | ESA & NASA & SERC | Earth orbit | ||||
| Astron | IKI | Earth orbit | ||||
| Hubble Space Telescope | NASA & ESA | — | Earth orbit | |||
| Broad Band X-ray Telescope / Astro 1 | NASA | Earth orbit | ||||
| Extreme Ultraviolet Explorer | NASA | Earth orbit | ||||
| Astro 2 | NASA | Earth orbit | ||||
| Far Ultraviolet Spectroscopic Explorer | NASA & CNES & CSA | Earth orbit | ||||
| Cosmic Hot Interstellar Spectrometer | NASA | Earth orbit | ||||
| Galaxy Evolution Explorer | NASA | Earth orbit | . | |||
| Korea Advanced Institute of Science and Technology Satellite 4 | KARI | ? | Earth orbit | |||
| Neil Gehrels Swift Observatory | NASA | — | Earth orbit | |||
| Interface Region Imaging Spectrograph | NASA | — | Earth orbit | |||
| Hisaki | JAXA | 8 December 2023 | Earth orbit | |||
| Venus Spectral Rocket Experiment | NASA | reusable | Suborbital to 300 km | |||
| Lunar-based ultraviolet telescope | CNSA | — | Lunar surface | |||
| AstroSat | ISRO | — | Earth orbit | |||
| Spatial Heterodyne Interferometric Emission Line Dynamics Spectrometer | NASA | 19 Apr 2021 | 19 Apr 2021 | Suborbital to 284.8 km | ||
| Colorado Ultraviolet Transit Experiment | NASA, Colorado University | 27 Sep 2021 | nearly Sun-synchronous orbit with a ~90 minute orbital period | |||
| Carruthers Geocorona Observatory | NASA | L1 Lagrange point | ||||
| SPARCS | NASA | — | Geocentric orbit |
UV ranges listed at Ultraviolet astronomy#Ultraviolet space telescopes.