A telescope in Chile will soon dwarf today’s biggest optical telescopes. The Extremely Large Telescope’s 39-metre primary mirror will collect roughly 13 times as much light as a 10-metre-class telescope — and it isn’t even finished yet.
Right now, the title of “world’s largest working telescope” belongs to a 10.4-metre giant in Spain’s Canary Islands. But that crown is about to change hands — twice — over the next few years. This list covers the ten biggest telescopes on Earth today, both operating and under construction, using verified specs from ESO, NASA-linked sources, and the observatories themselves.
Key Highlights / Quick Facts
- The Gran Telescopio Canarias (GTC) in Spain is currently the largest single-aperture optical telescope working today, at 10.4 metres.
- The Extremely Large Telescope (ELT), under construction in Chile, will have a 39-metre mirror — about 13 times more light-gathering power than today’s biggest scopes.
- ELT’s dome alone is 93 metres wide and 80 metres tall, roughly the size of a football stadium.
- The twin Keck I and Keck II telescopes in Hawaii were the first to use a segmented-mirror design, at 10 metres each.
- The Large Binocular Telescope (LBT) in Arizona uses two 8.4m mirrors side by side for a combined 11.8m aperture — the largest non-segmented design on Earth.
- SALT in South Africa is the largest optical telescope in the entire Southern Hemisphere, with a 9.2m effective aperture.
- The Giant Magellan Telescope (GMT) in Chile, targeting first light around 2029, will use seven 8.4m mirrors for a 24.5m aperture.
- ELT construction crossed the 50% completion milestone back in July 2023, and ESO’s official timeline now targets telescope first light in March 2029 and scientific first light in December 2030.
How “Largest Telescope” Is Actually Measured
Here’s where most lists get it wrong. “Largest” isn’t just about the width of the mirror — it depends on whether you’re counting a single solid mirror, a segmented mirror made of dozens of smaller pieces, or an interferometer array where multiple separate telescopes work together as one “virtual” instrument.
For example, the Very Large Telescope Interferometer in Chile can combine four 8.2m telescopes to reach an effective baseline of 130 metres — but you can’t point that “130 metres” at a planet like a single mirror. So this list focuses on genuine single-observatory apertures, the number astronomers actually use when comparing light-gathering power.
One more thing worth flagging upfront: this ranking mixes physical primary-mirror diameter (like GTC’s 10.4m) with effective/combined collecting aperture (like LBT’s 11.8m from two mirrors, or HET’s upgraded 10m effective aperture). These aren’t perfectly interchangeable numbers, but they’re the standard figures each observatory itself publishes, so that’s what we’ve used here rather than forcing every telescope into one measurement type.
Why Bigger Mirrors Actually Matter
A bigger mirror isn’t just about bragging rights. Light-gathering power grows with the square of the diameter, so a jump from 10 metres to 39 metres isn’t four times better — it’s closer to fifteen times better. That’s the difference between barely detecting a distant galaxy and actually studying its structure in detail.
The Top 10 Largest Telescopes in the World
1. Extremely Large Telescope (ELT) — 39 metres (under construction)
Sitting atop Cerro Armazones in Chile’s Atacama Desert, the ELT will hold the record for the largest optical and infrared telescope ever built once it’s finished. Its primary mirror is made of 798 hexagonal segments, and the whole structure is housed inside a dome roughly the size of a football stadium. Construction passed the halfway mark back in July 2023, and according to ESO’s official project timeline, the telescope structure is due for completion in 2027, with telescope first light planned for March 2029 and scientific first light targeted for December 2030.
2. Thirty Meter Telescope (TMT) — 30 metres (planned)
The TMT is designed to combine 492 mirror segments into a single 30-metre aperture, and its planned site is Mauna Kea in Hawaii — though the project has faced years of delays tied to land-use disputes with Native Hawaiian groups. If it goes ahead as planned, it will sit just behind the ELT and GMT in raw size, but its high-altitude Hawaiian location would give it exceptionally stable atmospheric conditions for sharp imaging.
3. Giant Magellan Telescope (GMT) — 24.5 metres (under construction)
Built on Cerro Las Campanas in Chile, the GMT uses a distinctive design of seven 8.4-metre mirrors arranged like a flower, rather than hundreds of tiny segments. That approach makes each individual mirror easier to manufacture and polish. The GMT Consortium’s most recent reports point to first light around 2029, and once running, it’s expected to produce images roughly ten times sharper than the Hubble Space Telescope.
4. Large Binocular Telescope (LBT) — 11.8 metres combined
Located on Mount Graham in Arizona, USA, the LBT is genuinely unique — it uses two identical 8.4-metre mirrors mounted side by side on one structure, working almost like a giant pair of binoculars. That gives it a combined light-collecting area larger than any single non-segmented mirror on Earth. In 2008, LBT contributed to spotting a galaxy cluster roughly 6 billion light-years away, proving its deep-field capability.
5. Gran Telescopio Canarias (GTC) — 10.4 metres
Perched at 2,267 metres altitude on La Palma in Spain’s Canary Islands, GTC currently holds the title of the world’s largest single-aperture optical telescope actually in operation. Its mirror is built from 36 hexagonal segments, each 1.9 metres wide, working together as one surface. It took more than a decade and over 1,000 people from 100+ companies to complete, and it officially saw first light back in 2007.
6. Keck I and Keck II — 10 metres each
Twin telescopes on the summit of Mauna Kea in Hawaii, the Keck Observatory telescopes were the first in the world to successfully use a segmented mirror, a design every giant telescope on this list has since copied in some form. Each mirror is made from 36 hexagonal segments. Keck I opened in 1993 and Keck II in 1996, and together they’ve been central to some of astronomy’s biggest discoveries, including early evidence for the supermassive black hole at the centre of our galaxy.
7. Southern African Large Telescope (SALT) — 9.2 metres effective aperture
Located near Sutherland in South Africa’s semi-desert Karoo region, SALT is the largest optical telescope anywhere in the Southern Hemisphere. Its primary mirror array actually spans 11.1 by 9.8 metres physically, built from 91 hexagonal 1-metre segments, but its usable effective aperture works out to 9.2 metres. SALT is built mainly for spectroscopy — breaking down starlight to study what distant objects are made of — rather than sharp direct imaging.
8. Hobby-Eberly Telescope (HET) — 10 metres effective aperture
Based at McDonald Observatory in Texas, USA, the Hobby-Eberly Telescope shares a similar segmented-mirror, fixed-elevation design philosophy to SALT. Its effective aperture grew to 10 metres after a major 2015 upgrade added extra mirror segments. HET was built specifically to be a cost-efficient spectroscopy powerhouse rather than a general-purpose imaging telescope, which let its designers cut construction costs significantly compared to fully steerable giants like Keck.
9. Subaru Telescope — 8.2 metres
Owned and operated by Japan, the Subaru Telescope sits on Mauna Kea in Hawaii and uses a single monolithic 8.2-metre mirror rather than segments — one of the largest solid, one-piece mirrors ever cast. Subaru is especially known for its wide-field imaging capability, useful for surveying huge patches of sky at once, including work that has helped track near-Earth asteroids.
10. Very Large Telescope (VLT) — 8.2 metres x 4 (interferometer)
Operated by the European Southern Observatory on Cerro Paranal in Chile, the VLT is actually four separate 8.2-metre telescopes that can work individually or be combined through interferometry to simulate a much larger instrument. When linked, the VLT Interferometer can achieve a resolution roughly equivalent to a 130-metre telescope for certain observations, even though no single mirror is anywhere near that size.
Telescope Specifications Table
| Telescope | Aperture | Status | Location |
| Extremely Large Telescope (ELT) | 39 m | Under construction | Cerro Armazones, Chile |
| Thirty Meter Telescope (TMT) | 30 m | Planned | Mauna Kea, Hawaii, USA |
| Giant Magellan Telescope (GMT) | 24.5 m | Under construction | Cerro Las Campanas, Chile |
| Large Binocular Telescope (LBT) | 11.8 m (combined) | Operating | Mount Graham, Arizona, USA |
| Gran Telescopio Canarias (GTC) | 10.4 m | Operating | La Palma, Canary Islands, Spain |
| Keck I & Keck II | 10 m each | Operating | Mauna Kea, Hawaii, USA |
| Southern African Large Telescope (SALT) | 9.2 m effective | Operating | Sutherland, South Africa |
| Hobby-Eberly Telescope (HET) | 10 m (segmented) | Operating | Fort Davis, Texas, USA |
| Subaru Telescope | 8.2 m | Operating | Mauna Kea, Hawaii, USA |
| Very Large Telescope (VLT) | 8.2 m x 4 | Operating | Cerro Paranal, Chile |
Data compiled from ESO, Britannica, Sky & Telescope, and individual observatory reports, current to 2026.
Pros and Cons of Giant Ground Telescopes
| Pros | Cons |
| Far cheaper per metre of aperture than launching a space telescope | Ground-based scopes still fight atmospheric blur, even with adaptive optics |
| Segmented-mirror designs let engineers build far larger apertures than a single-cast mirror allows | Giant projects like ELT and TMT face decade-long construction timelines and billion-dollar budgets |
| Can be serviced, upgraded, and fitted with new instruments on-site | Remote mountaintop locations mean high transport and maintenance costs |
| Interferometry (like VLT) can simulate much larger effective apertures | Combined-array systems are far more complex to operate and calibrate |
| High-altitude desert sites offer extremely clear, dry, stable skies | Some sites, like TMT’s, face land-rights disputes that delay construction for years |
Comparison Table: Operating vs Under-Construction Telescopes
| Category | Largest Example | Aperture | Expected Impact |
| Currently Operating | Gran Telescopio Canarias | 10.4 m | World’s largest working single-aperture scope today |
| Under Construction | Extremely Large Telescope | 39 m | ~13x more light-gathering power than today’s biggest scopes |
| Combined/Binocular Design | Large Binocular Telescope | 11.8 m combined | Largest non-segmented light-collecting surface |
| Interferometer Array | Very Large Telescope Interferometer | ~130 m effective baseline | Resolution rivaling a much larger single mirror for specific targets |
Step-by-Step: How a Giant Segmented Mirror Is Built
- Cast individual hexagonal segments — Each mirror piece, often 1 to 1.9 metres wide, is cast separately from special low-expansion glass ceramic.
- Grind and polish to nanometre precision — Segments are shaped so precisely that surface errors are smaller than a fraction of the wavelength of light.
- Coat with a reflective layer — A thin aluminum or silver coating is applied in a vacuum chamber to maximize reflectivity.
- Mount segments on active supports — Each segment sits on actuators that constantly make tiny adjustments to keep the whole mirror surface perfectly aligned.
- Install adaptive optics systems — Deformable secondary or tertiary mirrors correct for atmospheric turbulence in real time, sharpening the final image.
- First light and calibration — The completed telescope is pointed at a bright, well-known star or galaxy to test focus and alignment before science operations begin.
2026 Trends and News in Telescope Construction
The biggest story in ground-based astronomy right now is the ELT’s construction pace. The project passed its 50% completion milestone back in July 2023, and ESO’s current official timeline has the telescope structure and dome finishing in 2027, with telescope first light planned for March 2029 and scientific first light expected in December 2030 — a timeline that has shifted somewhat from earlier, more optimistic projections due to the sheer complexity of the build.
Meanwhile, the Thirty Meter Telescope’s Hawaii site remains contested, and its timeline continues to depend on resolving long-standing community and land-use concerns before construction can resume at full pace. The Giant Magellan Telescope, by contrast, has kept a steadier build schedule in Chile, with its seven-mirror design and first-light target still pointing to around 2029.
There’s also fresh movement on the instrument side — agreements for ELT’s next-generation instruments, including MOSAIC, were finalized in late 2025, and testing continues on the telescope’s deformable mirror system, a key piece of technology for correcting atmospheric distortion once the ELT finally opens its eye on the sky.
References
- European Southern Observatory (ESO) — Extremely Large Telescope Progress Reports — https://www.eso.org/public/news/eso2310/
- Space.com — Extremely Large Telescope Facts — https://www.space.com/40746-extremely-large-telescope.html
- Britannica — Gran Telescopio Canarias — https://www.britannica.com/topic/Gran-Telescopio-Canarias
- Gran Telescopio CANARIAS Official Site — https://www.gtc.iac.es/gtc/gtc.php
- Sky & Telescope — The New Largest Telescope in the World — https://skyandtelescope.org/astronomy-news/the-new-largest-telescope-in-the-world/
- W. M. Keck Observatory — https://www.keckobservatory.org/
- Southern African Large Telescope (SALT) — https://www.salt.ac.za/
- Go Astronomy — 10 Largest Optical Telescopes in the World — https://www.go-astronomy.com/10-largest-telescopes.htm
- RankRed — Largest Telescopes in the World — https://www.rankred.com/largest-telescopes-in-the-world/
- Friends of NASA — ELT Construction Update — https://www.friendsofnasa.org/2026/07/extremely-large-telescope-construction.html
- ESO — Giant Magellan Telescope Reports — https://giantmagellan.org/
- Space.com — World’s Largest Telescope Comes Together — https://www.space.com/the-universe/a-giant-rising-in-the-desert-worlds-largest-telescope-comes-together-photo
- ESO — ELT Official Project Timeline — https://elt.eso.org/about/timeline/
- ESO — Telescope First Light Now Planned for March 2029 — https://www.eso.org/public/announcements/ann25001/
- ESO — Facts About the ELT — https://elt.eso.org/about/facts/
FAQs
The Gran Telescopio Canarias (GTC) in Spain’s Canary Islands is currently the largest single-aperture optical telescope in operation, with a 10.4-metre mirror.
The Extremely Large Telescope (ELT), under construction in Chile, will hold that title with a 39-metre primary mirror. ESO’s official timeline points to telescope first light in March 2029 and scientific first light in December 2030.
The VLT consists of four separate 8.2-metre telescopes. They can be combined using interferometry to simulate a much larger effective aperture for specific observations, but no single VLT mirror is anywhere near the size of GTC or Keck.
According to ESO, the ELT’s 39-metre mirror will collect roughly 13 times as much light as a 10-metre-class telescope, letting it detect much fainter and more distant objects than anything currently operating.
The majority sit atop high-altitude, dry mountain sites — Mauna Kea in Hawaii, La Palma in Spain’s Canary Islands, and Chile’s Atacama Desert — chosen specifically for their clear, stable, low-turbulence skies.
Not always. Larger apertures mean more light-gathering power and sharper resolution, but the telescope’s design, adaptive optics quality, and instrument suite also heavily determine what kind of science it can actually do.



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