List of space telescopes

Last updated

The Hubble Space Telescope Hubble 01.jpg
The Hubble Space Telescope
Comparison between many space telescopes by diameter Space telescopes comparison.jpg
Comparison between many space telescopes by diameter
Overview of active and future telescopes (as of January 2021) Space observatories.png
Overview of active and future telescopes (as of January 2021)

This list of space telescopes (astronomical space observatories) 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 (e.g., the Sun and its planets), are excluded; see List of Solar System probes for these, and List of Earth observation satellites for missions targeting Earth.

Contents

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 (periapsis) and the maximum distance (apoapsis) between the telescope and the center of mass of the Sun are given in astronomical units (AU).

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. [1]

PhotoNameSpace agencyLaunch dateTerminatedLocationRef(s)
Proton1-2.gif Proton-1 USSR 16 Jul 196511 Oct 1965Earth orbit (183-589 km) [2]
Proton1-2.gif Proton-2 USSR 2 Nov 19656 Feb 1966Earth orbit (191-637 km) [2]
Proton1-2.gif Proton-4 USSR 16 Nov 196824 Jul 1969Earth orbit (248-477 km) [3]
SAS 2.gif Small Astronomy Satellite 2 (SAS-B) NASA 15 Nov 19728 Jun 1973Earth orbit (443–632 km) [4] [5]
Cos-B.jpg Cos-B ESA 9 Aug 197525 Apr 1982Earth orbit (339.6–99,876 km) [6] [7] [8]
HEAO-C in clean room.jpg High Energy Astronomy Observatory 3 NASA 20 Sep 197929 May 1981Earth orbit (486.4–504.9 km) [9] [10] [11]
Granat.gif Granat CNRS & IKI 1 Dec 198925 May 1999Earth orbit (2,000–200,000 km) [12] [13] [14]
Mir-27.jpg Gamma USSR, CNES, RSA 11 Jul 19901992Earth orbit (375 km) [15]
Cartoon CGRO.jpg Compton Gamma Ray Observatory (CGRO) NASA 5 Apr 19914 Jun 2000Earth orbit (362–457 km) [16] [17] [18]
Low Energy Gamma Ray Imager (LEGRI) INTA 19 May 1997Feb 2002Earth orbit (600 km) [19] [20]
HETE-2 launch preparations.jpg High Energy Transient Explorer 2 (HETE 2) NASA 9 Oct 2000Mar 2008Earth orbit (590–650 km) [21] [22] [23]
INTEGRAL spacecraft model.png International Gamma Ray Astrophysics Laboratory (INTEGRAL) ESA 17 Oct 2002Earth orbit (639–153,000 km) [24] [25]
Swift Observatory spacecraft model.png Neil Gehrels Swift Observatory NASA 20 Nov 2004Earth orbit (585–604 km) [26] [27]
AGILE satellite model 1.jpg Astrorivelatore Gamma ad Immagini Leggero (AGILE) ISA 23 Apr 200718 Jan 2024Earth orbit (524–553 km) [28] [29]
Diagram of the GLAST instrument.jpg Fermi Gamma-ray Space Telescope NASA 11 Jun 2008Earth orbit (555 km) [30]
IKAROS IAC 2010.jpg Gamma-Ray Burst Polarimeter (IKAROS) JAXA 21 May 201021 May 2015Heliocentric orbit [31] [32]

X-ray

X-ray telescopes 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 (cataclysmic variable stars), neutron star or black hole (X-ray binaries). 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.

PhotoNameSpace agencyLaunch dateTerminatedLocationRef(s)
X-Ray Explorer Satellite.jpg Uhuru (Small Astronomy Satellite 1, SAS-A) NASA 12 Dec 1970Mar 1973Earth orbit (531–572 km) [33] [34] [35]
ANS backup flightarticle.jpg Astronomical Netherlands Satellite (ANS) SRON 30 Aug 1974Jun 1976Earth orbit (266–1176 km) [36] [37]
Ariel-5.jpg Ariel V SRC & NASA 15 Oct 197414 Mar 1980Earth orbit (520 km) [38] [39]
Aryabhata Satellite.jpg Aryabhata ISRO 19 Apr 197523 Apr 1975Earth orbit (563–619 km) [40]
SAS-3 layout.gif Small Astronomy Satellite 3 (SAS-C) NASA 7 May 1975Apr 1979Earth orbit (509–516 km) [41] [42] [43]
Cos-B.jpg Cos-B ESA 9 Aug 197525 Apr 1982Earth orbit (339.6–99,876 km) [6] [7] [8]
Cosmic Radiation Satellite (CORSA) ISAS 4 Feb 19764 Feb 1976Failed launch [44] [45]
HEAO-1 Assembling the High Energy Astronomy Observatory 7884320.jpg High Energy Astronomy Observatory 1 (HEAO 1) NASA 12 Aug 19779 Jan 1979Earth orbit (445 km) [46] [47] [48]
HEAO-2 High Energy Astronomy Observatory 0102090.jpg Einstein Observatory (HEAO 2) NASA 13 Nov 197826 Apr 1981Earth orbit (465–476 km) [49] [50]
Corsa-b hakucho.gif Hakucho (CORSA-b) ISAS 21 Feb 197916 Apr 1985Earth orbit (421–433 km) [51] [52] [53]
HEAO-C in clean room.jpg High Energy Astronomy Observatory 3 (HEAO 3) NASA 20 Sep 197929 May 1981Earth orbit (486.4–504.9 km) [9] [10] [11]
Astro-b tenma.gif Tenma (Astro-B) ISAS 20 Feb 198319 Jan 1989Earth orbit (489–503 km) [54] [55] [56]
Astron.gif Astron IKI 23 Mar 1983Jun 1989Earth orbit (2,000–200,000 km) [57] [58] [59]
Exosat.jpg EXOSAT ESA 26 May 19838 Apr 1986Earth orbit (347–191,709 km) [60] [61] [62]
Astro-c ginga.png Ginga (Astro-C) ISAS 5 Feb 19871 Nov 1991Earth orbit (517–708 km) [63] [64] [65]
Granat.gif Granat CNRS & IKI 1 Dec 198925 May 1999Earth orbit (2,000–200,000 km) [12] [13] [14]
ROSAT NASA & DLR 1 Jun 199012 Feb 1999Re-entry 23 October 2011. [66]
Formerly Earth orbit (580 km)
[67] [68] [69]
Astro-1 payload.png Broad Band X-ray Telescope / Astro 1 NASA 2 Dec 199011 Dec 1990Earth orbit (500 km) [70] [71]
ASCA.jpg Advanced Satellite for Cosmology and Astrophysics (ASCA, Astro-D) ISAS & NASA 20 Feb 19932 Mar 2001Earth orbit (523.6–615.3 km) [72] [73]
ALEXIS.png Array of Low Energy X-ray Imaging Sensors (Alexis) LANL 25 Apr 19932005Earth orbit (749–844 km) [74] [75] [76]
Rxte.jpg Rossi X-ray Timing Explorer (RXTE) NASA 30 Dec 19953 Jan 2012Earth orbit (409 km) [77] [78] [79]
BeppoSAX.jpg BeppoSAX ASI 30 Apr 199630 Apr 2002Earth orbit (575–594 km) [80] [81] [82]
Abrixas.png A Broadband Imaging X-ray All-sky Survey (ABRIXAS) DLR 28 Apr 19991 Jul 1999Earth orbit (549–598 km) [83] [84] [85]
Chandra artist illustration.jpg Chandra X-ray Observatory NASA 23 Jul 1999Earth orbit (9,942–140,000 km) [86] [87]
XMM-Newton spacecraft model.png XMM-Newton ESA 10 Dec 1999Earth orbit (7,365–114,000 km) [88] [89]
HETE-2 launch preparations.jpg High Energy Transient Explorer 2 (HETE 2) NASA 9 Oct 2000Mar 2008Earth orbit (590–650 km) [21] [22] [90]
INTEGRAL spacecraft model.png International Gamma Ray Astrophysics Laboratory (INTEGRAL) ESA 17 Oct 2002Earth orbit (639–153,000 km) [24] [25]
Swift Observatory spacecraft model.png Neil Gehrels Swift Observatory NASA 20 Nov 2004Earth orbit (585–604 km) [26] [27]
Astro-E2.jpg Suzaku (Astro-E2) JAXA & NASA 10 Jul 20052 Sep 2015Earth orbit (550 km) [91] [92]
AGILE satellite model 1.jpg Astrorivelatore Gamma ad Immagini Leggero (AGILE) ISA 23 Apr 200718 Jan 2024Earth orbit (524–553 km) [28] [29]
NuSTAR spacecraft model.png Nuclear Spectroscopic Telescope Array (NuSTAR) NASA 13 Jun 2012Earth orbit (603.5 km) [93] [94]
Astrosat-1 in deployed configuration.png AstroSat ISRO 28 Sep 2015Earth orbit (600–650 km) [95] [96] [97]
Astro-H schema (en).png Hitomi (Astro-H) JAXA 17 Feb 201628 Apr 2016Earth orbit (575 km) [98] [99] [100]
Maquete satellite MVL-300 (Mikhailo Lomonosov) DSC 0071.JPG Mikhailo Lomonosov Moscow State University 28 Apr 201630 Jun 2018Earth orbit (478–493 km) [101] [102]
NICER on the ISS.jpg Neutron Star Interior Composition Explorer (NICER) NASA 7 Jun 2017 International Space Station [103]
HXMT rendering.jpg Hard X-ray Modulation Telescope (HXMT) CNSA & CAS 14 Jun 2017Low Earth orbit (545–554.1 km) [104]
Spektr-RG russian X-ray space telescope P1110968.jpg Spektr-RG RSRI & MPE Jul 13, 2019Sun-Earth L2 [105]
Imaging X-ray Polarimetry Explorer.jpg Imaging X-ray Polarimetry Explorer (IXPE) NASA 9 Dec 2021Earth orbit (540 km) [106] [107]
Lobster Eye Imager for Astronomy (LEIA) CSA 27 Jul 2022 Low Earth orbit [108] [109]
XRISM in a nutshell (cropped).png X-ray Imaging and Spectroscopy Mission (XRISM) JAXA & NASA 7 Sep 2023Earth orbit (550 km) [110] [111]
X-ray Polarimeter satellite (XPoSat).jpg X-ray Polarimeter Satellite (XPoSat) ISRO & RRI 1 Jan 2024Earth orbit (638–653 km) [112] [113]
Einstein Probe illustration.png Einstein Probe CAS & ESA & MPE 9 Jan 2024Earth orbit (581–593 km) [114]

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. [115] Objects emitting ultraviolet radiation include the Sun, other stars and galaxies. [116]

PhotoNameSpace agencyLaunch dateTerminatedObserving locationRef(s)
Orbiting Astronomical Observatory 2.jpg OAO-2 (Stargazer) NASA 7 Dec 1968Jan 1973Earth orbit (749–758 km) [117] [118]
Orion 1 and Orion 2 Space Observatories USSR 19 Apr 1971 (Orion 1); (Orion 2) 18 Dec 19731971; 1973Earth orbit (Orion 1: 200–222 km; Orion 2: 188–247 km) [119] [120]
Far Ultraviolet Camera Spectrograph.jpg Far Ultraviolet Camera/Spectrograph (UVC) NASA 16 Apr 197223 Apr 1972Descartes Highlands on lunar surface [121]
OAO-3 in the clean room.jpg OAO-3 Copernicus NASA 21 Aug 1972Feb 1981Earth orbit (713–724 km) [117]
ANS backup flightarticle.jpg Astronomical Netherlands Satellite (ANS) SRON 30 Aug 1974Jun 1976Earth orbit (266–1176 km) [36] [37]
International Ultraviolet Explorer.gif International Ultraviolet Explorer (IUE) ESA & NASA & SERC 26 Jan 197830 Sep 1996Earth orbit (32,050–52,254 km) [122] [123]
Astron.gif Astron IKI 23 Mar 1983Jun 1989Earth orbit (2,000–200,000 km) [57] [58] [59]
HST-SM4.jpeg Hubble Space Telescope NASA & ESA 24 Apr 1990Earth orbit (586–610 km) [124]
Astro-1 payload.png Broad Band X-ray Telescope / Astro 1 NASA 2 Dec 199011 Dec 1990Earth orbit (500 km) [70] [71]
EUVE.jpg Extreme Ultraviolet Explorer (EUVE) NASA 7 Jun 199231 Jan 2001Earth orbit (515–527 km) [125] [126]
Astro2 sts67 big.jpg Astro 2 NASA 2 Mar 199318 Mar 1993Earth orbit (349–363 km) [127] [128]
FUSE prelaunch crop.jpg Far Ultraviolet Spectroscopic Explorer (FUSE) NASA & CNES & CSA 24 Jun 199912 Jul 2007Earth orbit (752–767 km) [129] [130]
CHIPSAT 2.jpg Cosmic Hot Interstellar Spectrometer (CHIPS) NASA 13 Jan 200311 Apr 2008Earth orbit (578–594 km) [131] [132]
Galex.jpg Galaxy Evolution Explorer (GALEX) NASA 28 Apr 200328 Jun 2013Earth orbit (691–697 km). [133] [134] [135]
Korea Advanced Institute of Science and Technology Satellite 4 (Kaistsat 4) KARI 27 Sep 20032007?Earth orbit (675–695 km) [136] [137]
Swift Observatory spacecraft model.png Neil Gehrels Swift Observatory (Swift) NASA 20 Nov 2004Earth orbit (585–604 km) [26] [27]
IRIS (Explorer).jpg Interface Region Imaging Spectrograph (IRIS) NASA 27 Jun 2013Earth orbit (387–415 km) [138] [139]
Hisaki-sprint-a-artistconcept2013.png Hisaki (SPRINT-A) JAXA 14 Sep 20138 December 2023Earth orbit (957–1151 km) [140] [141]
Venus Spectral Rocket Experiment NASA 26 Nov 2013reusableSuborbital to 300 km [142]
Lunar-based ultraviolet telescope (LUT) CNSA 1 Dec 2013Lunar surface [143]
Astrosat-1 in deployed configuration.png AstroSat ISRO 28 Sep 2015Earth orbit (600–650 km) [96] [95] [97]
Spatial Heterodyne Interferometric Emission Line Dynamics Spectrometer (SHIELDS) NASA 19 Apr 202119 Apr 2021Suborbital to 284.8 km [144]

UV ranges listed at Ultraviolet astronomy#Ultraviolet space telescopes.

Visible light

The oldest form of astronomy, optical or visible-light astronomy, observes wavelengths of light from approximately 400 to 700 nm. [145] Positioning an optical telescope in space eliminates the distortions and limitations that hamper that ground-based optical telescopes (see Astronomical seeing), providing higher resolution images. Optical telescopes are used to look at planets, stars, galaxies, planetary nebulae and protoplanetary disks, amongst many other things. [146]

PhotoNameSpace agencyLaunch dateTerminatedLocationRef(s)
Hipparcos-testing-estec.jpg Hipparcos ESA 8 Aug 1989Mar 1993Earth orbit (223–35,632 km) [147] [148] [149]
HST-SM4.jpeg Hubble Space Telescope NASA & ESA 24 Apr 1990Earth orbit (586.47–610.44 km) [124]
MOST CSA 30 Jun 2003Mar 2019Earth orbit (819–832 km) [150] [151]
Swift Observatory spacecraft model.png Neil Gehrels Swift Observatory NASA 20 Nov 2004Earth orbit (585–604 km) [26] [27]
COROT integration.jpg COROT CNES & ESA 27 Dec 20062013Earth orbit (872–884 km) [152] [153]
Kepler Space Telescope spacecraft model 2.png Kepler NASA 6 Mar 200930 Oct 2018Earth-trailing heliocentric orbit [154] [155] [156]
V Sieradzka Konferencja Kosmiczna Satelita Lem - model 2014 MZW 100 8550.jpg BRITE constellationAustria, Canada, Poland25 Feb 2013 - 19 Aug 2014Earth orbit [157]
Near Earth Object Surveillance Satellite (NEOSSat) CSA, DRDC 25 Feb 2013 Sun-synchronous Earth orbit (776–792 km) [158] [159]
Gaia spacecraft.jpeg Gaia (astrometry) ESA 19 Dec 2013 Sun-Earth L2 Lagrange point [160]
Astrosat-1 in deployed configuration.png AstroSat ISRO 28 Sep 2015Earth orbit (600–650 km) [95] [96] [97]
Transiting Exoplanet Survey Satellite artist concept (transparent background).png Transiting Exoplanet Survey Satellite (TESS) NASA 18 Apr 2018High Earth Orbit [161]
CHEOPS ESA 18 Dec 2019 Sun-synchronous orbit [162]
ILO-X ILOA 15 Feb 2024Lunar surface [163]

Infrared and submillimetre

Infrared light is of lower energy than visible light, hence is emitted by sources that are either cooler, or moving away from the observer (in present context: Earth) at high speed. As such, the following can be viewed in the infrared: cool stars (including brown dwarves), nebulae, and redshifted galaxies. [164]

PhotoNameSpace agencyLaunch dateTerminatedLocationRef(s)
IRAS in orbit.jpg IRAS NASA 25 Jan 198321 Nov 1983Earth orbit (889–903 km) [165] [166]
STS072-734-011.jpg Infrared Telescope in Space ISAS & NASDA 18 Mar 199525 Apr 1995Earth orbit (486 km) [167] [168]
Schema-telescope-ISO.png Infrared Space Observatory (ISO) ESA 17 Nov 199516 May 1998Earth orbit (1000–70500 km) [169] [170] [171]
Midcourse Space Experiment.png Midcourse Space Experiment (MSX) USN 24 Apr 199626 Feb 1997Earth orbit (900 km) [172]
Swas 1.jpg Submillimeter Wave Astronomy Satellite (SWAS) NASA 6 Dec 1998Last used in 2005Earth orbit (638–651 km) [173] [174]
Wide Field Infrared Explorer module.jpg Wide Field Infrared Explorer (WIRE) NASA 5 Mar 1999no observationsRe-entered May 10, 2011 [175] [176]
Spitzer space telescope.jpg Spitzer Space Telescope NASA 25 Aug 200330 Jan 2020 [177] Solar orbit (0.98–1.02 AU) [178] [179]
Scale model of the Akari (ASTRO-F, 2006-005A) exhibited at Noshiro City Children's Center.jpg Akari (Astro-F) JAXA 21 Feb 200624 Nov 2011 [180] Earth orbit (586.47–610.44 km) [181] [182]
Maquette Herschel salon du Bourget 2013 DSC 0217.JPG Herschel Space Observatory ESA & NASA 14 May 2009 [183] 29 Apr 2013 [184] Sun-Earth L2 Lagrange point [185] [186] [187]
WISE artist concept (PIA17254, crop).jpg Wide-field Infrared Survey Explorer (WISE) NASA 14 Dec 2009(hibernation Feb 2011 – Aug 2013) Earth orbit (500 km) [188] [189] [190]
CHEOPS spacecraft.jpg CHEOPS ESA 18 Dec 2019 Sun-synchronous orbit [162]
James Webb Space Telescope.jpg James Webb Space Telescope (JWST) NASA/ESA/CSA 25 Dec 2021 SunEarth L2 Lagrange point [191]
Euclid spacecraft ESA24912474.jpg Euclid ESA 1 Jul 2023Sun–Earth L2 Lagrange point [192] [193]

Microwave

Microwave space telescopes have primarily been used to measure cosmological parameters from the Cosmic Microwave Background. They also measure synchrotron radiation, free-free emission and spinning dust from our Galaxy, as well as extragalactic compact sources and galaxy clusters through the Sunyaev-Zel'dovich effect. [194]

PhotoNameSpace agencyLaunch dateTerminatedLocationRef(s)
Cobe vision1.jpg Cosmic Background Explorer (COBE) NASA 18 Nov 198923 Dec 1993Earth orbit (900 km) [195] [196]
Odin Swedish Space Corporation 20 Feb 2001Earth orbit (622 km) [197] [198]
WMAP2.jpg WMAP NASA 30 Jun 2001Oct 2010 Sun-Earth L2 Lagrange point [199]
Model of the Planck Satellite.jpg Planck ESA 14 May 2009Oct 2013 Sun-Earth L2 Lagrange point (mission)
Heliocentric (Derelict)
[186] [200] [201]

Radio

As the atmosphere is transparent for radio waves, radio telescopes in space are most useful for Very Long Baseline Interferometry: doing simultaneous observations of a source with both a satellite and a ground-based telescope and by correlating their signals to simulate a radio telescope the size of the separation between the two telescopes. Typical targets for observations include supernova remnants, masers, gravitational lenses, and starburst galaxies.[ citation needed ]

PhotoNameSpace agencyLaunch dateTerminatedLocationRef(s)
Haruka HALCA VSOP MUSES-B.jpg Highly Advanced Laboratory for Communications and Astronomy (HALCA, VSOP or MUSES-B) ISAS 12 Feb 199730 Nov 2005Earth orbit (560–21,400 km) [202] [203] [204]
RIAN archive 930415 Russian Spektr R space-born radio telescope.jpg Spektr-R (RadioAstron) ASC LPI 18 Jul 201111 Jan 2019Earth orbit (10,000–390,000 km) [205] [206] [207]

Particle detection

Spacecraft and space-based modules that do particle detection, looking for cosmic rays and electrons. These can be emitted by the sun (Solar Energetic Particles), our galaxy (Galactic cosmic rays) and extragalactic sources (Extragalactic cosmic rays). There are also Ultra-high-energy cosmic rays from active galactic nuclei, those can be detected by ground-based detectors via their particle showers.

PhotoNameSpace agencyLaunch dateTerminatedLocationRef(s)
Proton1-2.gif Proton-1 USSR 16 Jul 196511 Oct 1965Earth orbit (589–183 km) [2]
Proton1-2.gif Proton-2 USSR 2 Nov 19656 Feb 1966Earth orbit (637–191 km) [2]
HEAO-C in clean room.jpg High Energy Astronomy Observatory 3 (HEAO 3) NASA 20 Sep 197929 May 1981Earth orbit (486.4–504.9 km) [9] [10] [11]
SAMPEX.jpg SAMPEX NASA / DE3 Jul 199230 Jun 2004Earth orbit (512–687 km) [208]
AMS01Geneva.jpg Alpha Magnetic Spectrometer 01 (AMS-01) NASA 2 Jun 199812 Jun 1998Earth orbit (296 km) [209]
PAMELAonResurs-DK.jpg Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) ISA, INFN, RSA, DLR & SNSB 15 May 20067 Feb 2016Earth orbit (350–610 km) [210] [211]
IBEX spacecraft.jpg IBEX NASA 19 Oct 2008Earth orbit (86,000–259,000 km) [212]
Alpha Magnetic Spectrometer - 02.jpg Alpha Magnetic Spectrometer 02 (AMS-02) NASA 16 May 2011Earth orbit (353 km) on ISS [213]
Dark Matter Particle Explorer (DAMPE) CNSA & CAS 17 Dec 2015Earth orbit (500 km) [214]

Gravitational waves

A type of telescope that detects gravitational waves; ripples in space-time generated by colliding neutron stars or black holes.

PhotoNameSpace agencyLaunch dateTerminatedLocationRef(s)
A17 lunar surface gravimeter.jpg Lunar Surface Gravimeter NASA 7 Dec 197214 Dec 1972Taurus–Littrow [215]

To be launched

PhotoNameSpace agencyPlanned launch dateLocationRef(s)
SVOM.JPG SVOM CNSA/CNES 24 June 2024Low Earth orbit [216]
China CSST Xuntian.jpg Xuntian CNSA/CAS 2024Low Earth orbit [217] [218]
SPHEREx March2022 Update.jpg SPHEREx NASA 2025Earth orbit [219]
PLATO spacecraft.jpg PLATO ESA 2026Geosynchronous orbit [220]
Ultrasat model1.jpg ULTRASAT Israel Space Agency 2026Sun–Earth L2 Lagrange point [221]
ROMANNewModelV8RomanStill00049.png Nancy Grace Roman Space Telescope (Wide Field Infrared Survey Telescope; WFIRST) NASA/DOE 2027Sun–Earth L2 Lagrange point [222]
ARIEL ESA 2029Sun–Earth L2 Lagrange point [223]
Advanced Telescope for High Energy Astrophysics (Athena) ESA/NASA/JAXA 2035Sun–Earth L2 Lagrange point [224]
LISA-waves.jpg Laser Interferometer Space Antenna (LISA) ESA 2037 Heliocentric orbit [225]

See also

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