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Space telescopes

See further.
Beyond the atmosphere.

Hubble, James Webb and space observatories: complementary instruments for exploring galaxies, stars and planets.

Why observe from space?

The atmosphere blurs some images and absorbs much infrared radiation, X-rays and gamma rays. Above it, each mission opens a different window on the Universe.

Three ways to travel

Around Earth

An Earth orbit, low or highly elongated depending on the mission.

Near the L2 point

A region of the Sun–Earth system about 1.5 million kilometres from Earth. Observatories follow an orbit around L2.

Around the Sun

Some missions follow heliocentric orbits, sometimes gradually drifting away from Earth.

Hubble photographed from the shuttle Atlantis after servicing in 2009.
Photograph · NASA · Source · Public domain
NASA / ESALaunch 1990

Hubble

Ultraviolet, visible and near-infrared.

A versatile observatory upgraded through crewed servicing missions.

Observing location
Low Earth orbit.
History, instruments and discoveries

The instruments

Its instruments include WFC3, ACS, COS and STIS.

Scientific contribution

Deep images revealed distant galaxies; its measurements refined our understanding of cosmic expansion.

Official sources

Artist’s impression of the Chandra space telescope.
Artist’s impression · NASA/CXC · Source · Public domain
NASALaunch 1999

Chandra

X-rays.

A detailed view of extremely hot regions of the Universe.

Observing location
Highly elliptical Earth orbit.
History, instruments and discoveries

The instruments

ACIS and HRC detectors, with spectroscopy gratings.

Scientific contribution

Its images and spectra reveal supernova remnants, black holes and gas in galaxy clusters.

Official sources

Artist’s impression of the XMM-Newton space telescope.
Artist’s impression · ESA/XMM-Newton · Source · CC BY-SA 3.0 IGO
ESALaunch 1999

XMM-Newton

X-rays, complemented by ultraviolet and visible light.

Three X-ray telescopes collect light from the hot Universe.

Observing location
Elliptical Earth orbit.
History, instruments and discoveries

The instruments

EPIC cameras, RGS spectrometers and the OM optical monitor.

Scientific contribution

Spectra probe hot gas and matter around black holes.

Official sources

Artist’s impression of the Spitzer space telescope.
Artist’s impression · NASA · Source · Public domain
NASALaunch 2003

Spitzer

Infrared.

An observatory cooled to detect infrared light from celestial objects.

Observing location
During its mission: Earth-trailing solar orbit.
History, instruments and discoveries

The instruments

IRAC, IRS and MIPS; only two IRAC channels operated during the warm mission.

Scientific contribution

Its data explored forming stars, dusty galaxies and exoplanets.

Official sources

Artist’s impression of the Fermi space telescope.
Artist’s impression · NASA’s Goddard Space Flight Center/CI Lab · Source · Public domain
NASA / DOE / international partnersLaunch 2008

Fermi

Gamma rays.

An observatory of the most energetic cosmic light.

Observing location
Earth orbit.
History, instruments and discoveries

The instruments

Large Area Telescope (LAT) and Gamma-ray Burst Monitor (GBM).

Scientific contribution

It explores pulsars, jets from active galaxies and gamma-ray bursts.

Official sources

Artist’s impression of the Herschel space telescope.
Artist’s impression · NASA · Source · Public domain
ESALaunch 2009

Herschel

Far-infrared and submillimetre.

Its 3.5-metre mirror observed the cold Universe, often hidden by dust.

Observing location
During its mission: orbit around Sun–Earth L2.
History, instruments and discoveries

The instruments

PACS, SPIRE and HIFI.

Scientific contribution

It studied star formation and reservoirs of gas and dust in galaxies.

Official sources

Artist’s impression of the Planck space telescope.
Artist’s impression · ESA/NASA/JPL-Caltech · Source · Public domain
ESALaunch 2009

Planck

Microwaves through very far-infrared.

An observatory designed to measure tiny variations in the cosmic microwave background.

Observing location
During its mission: orbit around Sun–Earth L2.
History, instruments and discoveries

The instruments

LFI and HFI instruments.

Scientific contribution

Its maps refined parameters describing the age, composition and evolution of the Universe.

Official sources

Artist’s impression of the Kepler space telescope.
Artist’s impression · NASA · Source · Public domain
NASALaunch 2009

Kepler / K2

Visible light.

It searched for tiny dips in starlight caused by planets crossing their stars.

Observing location
During its mission: orbit around the Sun.
History, instruments and discoveries

The instruments

A photometer coupled to a Schmidt-type telescope.

Scientific contribution

Kepler showed that planetary systems are widespread in our Galaxy.

Official sources

Artist’s impression of the Gaia space telescope.
Artist’s impression · ESA/ATG medialab; background image: ESO/S. Brunier · Source · CC BY 4.0
ESALaunch 2013

Gaia

Visible light, extending into near-infrared.

An astrometry mission measuring stellar positions, distances and motions.

Observing location
During observations: orbit around Sun–Earth L2.
History, instruments and discoveries

The instruments

Astrometric field, BP/RP photometers and RVS spectrometer.

Scientific contribution

Its catalogues reconstruct the Milky Way in three dimensions and reveal its dynamical history.

Official sources

TESS in a cleanroom before launch.
Photograph · Orbital ATK / NASA · Source · Public domain
NASA / MITLaunch 2018

TESS

Red visible light and near-infrared.

A sky survey seeking planets that cross nearby, bright stars.

Observing location
Highly elliptical Earth orbit in resonance with the Moon.
History, instruments and discoveries

The instruments

Four wide-field cameras.

Scientific contribution

Its discoveries provide targets for measuring planetary masses and studying atmospheres.

Official sources

James Webb’s primary mirror in a cleanroom before launch.
Photograph · NASA/Chris Gunn · Source · Public domain
NASA / ESA / CSALaunch 2021

James Webb

Near- and mid-infrared.

A segmented mirror and large sunshield enable infrared exploration.

Observing location
Orbit around the Sun, near Sun–Earth L2.
History, instruments and discoveries

The instruments

NIRCam, NIRSpec, MIRI and NIRISS.

Scientific contribution

It studies early galaxies, star formation and the composition of exoplanet atmospheres.

Official sources

Artist’s impression of the Euclid space telescope.
Artist’s impression · ESA. Acknowledgement: Work performed by ATG under contract for ESA. · Source · CC BY-SA 3.0 IGO
ESA / Euclid Consortium / NASALaunch 2023

Euclid

Visible and near-infrared.

A galaxy survey designed to understand cosmic structure and expansion.

Observing location
Orbit around Sun–Earth L2.
History, instruments and discoveries

The instruments

VIS camera and NISP spectrometer-photometer.

Scientific contribution

Galaxy shapes and distributions test the effects of dark matter and dark energy.

Official sources

Selected historical and modern missions. Locations describe their observing orbits, not real-time tracking. The filter uses a main band; several missions cover multiple bands.

Images resized for the web. Credits, sources and licences appear below each image.