Every Space Telescope, One Live Hub
The complete, continuously-updated directory of every operational space telescope, from Hubble in low Earth orbit to JWST and the brand-new Nancy Grace Roman Space Telescope at Sun-Earth L2. Live positions, current science targets, mission history and instrument details for every active observatory, plus the retired legends that reshaped astronomy.
Jump to live trackers ↓ Compare all telescopesThe Three Great Observatories, Live
Live positions, altitudes and current science targets for Orbital Radar's flagship space-telescope trackers, updated every ten seconds and free of charge.
Six More Space Telescopes Currently in Orbit
Beyond the three Great Observatories, NASA operates a fleet of highly specialised space telescopes. Every one has a live position tracker on Orbital Radar built on the same real-time tracking engine as our ISS Tracker.
NICER, the X-ray Telescope on the ISS
Not every space telescope is a free-flyer. NICER is bolted to the ExPRESS Logistics Carrier 2 on the International Space Station, so its live position is the ISS's position, but its science story is entirely its own.
NICER, the Neutron star Interior Composition Explorer
Europe's Neighbours at L2, Euclid & Gaia
JWST and (soon) Roman are not alone at Sun-Earth L2. ESA's Euclid surveys the dark universe from a nearby halo orbit, and Gaia mapped the galaxy from L2 for over a decade before its 2025 retirement. Both journeys are tracked on our Deep Space Tracker.
Every Space Telescope, Compared
A quick-reference comparison of every active NASA-led space telescope plus the two ESA missions at L2. Mirror sizes, orbit types, current status and the year each began science.
| Telescope | Wavelength | Mirror | Orbit | Launched | Status | Tracker |
|---|---|---|---|---|---|---|
| Hubble | Optical / UV | 2.4 m | LEO 480 km | Apr 1990 | ● Active | Live |
| JWST | Infrared | 6.5 m segmented | Sun-Earth L2 | Dec 2021 | ● Active | Live |
| Roman | Wide-field IR | 2.4 m | Sun-Earth L2 (cruise) | Aug 2026 | ◐ Cruise | Live |
| Chandra | X-ray | 1.2 m equivalent | HEO 14k×134k km | Jul 1999 | ● Active | Live |
| TESS | Optical | 4×10 cm | Lunar-resonant | Apr 2018 | ● Active | Live |
| SPHEREx | Near-IR | 20 cm | Sun-sync LEO | Mar 2025 | ● Active | Live |
| Swift | γ / X / UV | 30 cm UVOT | LEO ~335 km | Nov 2004 | ● Active | Live |
| NuSTAR | Hard X-ray | Focusing optics | LEO ~550 km | Jun 2012 | ● Active | Live |
| IXPE | X-ray polarimetry | 3× focusing | Equatorial LEO | Dec 2021 | ● Active | Live |
| NICER | Soft X-ray | 56 detectors | Mounted on ISS | Jun 2017 | ● Active | Via ISS |
| Euclid | Optical / NIR | 1.2 m | Sun-Earth L2 | Jul 2023 | ● Active | Deep Space |
| Gaia | Optical astrometry | 1.45×0.5 m ×2 | Sun-Earth L2 | Dec 2013 | ○ Retired 2025 | Deep Space |
| Kepler | Optical | 0.95 m | Heliocentric | Mar 2009 | ○ Retired 2018 | Retired |
| Spitzer | Mid-IR | 0.85 m | Heliocentric | Aug 2003 | ○ Retired 2020 | Retired |
Space Telescopes by Orbit Type
Where an observatory lives determines what it can see, how long it lasts and how you can find it in the sky. See our Types of Orbits primer for the physics.
Retired Legends of Space Astronomy
Every space telescope has a service life measured in fuel, coolant or component drift. These missions are done, but the data still shapes today's astronomy.
Why We Put Telescopes in Space
Every space telescope exists to solve one problem: Earth's atmosphere. Water vapour, carbon dioxide and ozone absorb most of the infrared, ultraviolet and X-ray light arriving from the universe, and turbulence in the air blurs whatever visible light does make it through. Get above the atmosphere and every waveband opens up.
The world's first space telescope was OAO-2, launched in 1968. Since then more than seventy space telescopes have flown. In September 2026 nine major NASA-led observatories are operating simultaneously, the largest fleet of astrophysics missions in history.
The Great Observatories
NASA's Great Observatories programme flew four flagship telescopes designed to cover the electromagnetic spectrum together: Hubble (visible / UV), the Compton Gamma-Ray Observatory (gamma-ray, deorbited 2000), Chandra (X-ray) and Spitzer (infrared). Three of the four have retired or been deorbited, but Hubble and Chandra are still returning science more than 25 years after launch.
JWST is often called the successor to Hubble but it is really the successor to Spitzer, an infrared observatory of unprecedented sensitivity, parked at Sun-Earth L2 to keep it cold. Roman is the successor to Hubble in a stricter sense: same 2.4-metre mirror class, wide-field imaging where Hubble did pinpoint work.
Why L2 Is the Prime Real Estate
Two telescopes currently orbit the Sun-Earth L2 point 1.5 million kilometres beyond Earth on the anti-Sun side, JWST and ESA's Euclid; Gaia worked there too until its 2025 retirement. Roman will make it three by early December 2026. L2 lets a telescope keep the Sun, Earth and Moon all on the same side of the sky, which means a single sunshield can point away from every warm source at once. That is essential for infrared telescopes that must run at a few tens of kelvin.
How to Read a Space Telescope's Orbit
Different missions live in dramatically different orbits. Hubble is in a shallow low Earth orbit so the Space Shuttle could service it. Chandra was placed in a highly elliptical orbit that carries it a third of the way to the Moon so it can spend most of its time above the Van Allen radiation belts. TESS uses a P/2 lunar-resonant orbit no other spacecraft has ever flown. Each choice trades servicing access, science return and stability. Our Types of Orbits primer walks through why.