Space and PhysicsAstronomy

What Comes After JWST? More Extraordinary Telescopes Are On Their Way

The breathtaking images from the JWST are just the beginning; a range of giant telescopes and niche designs are on their way.


Stephen Luntz

Freelance Writer

clockJul 29 2022, 08:01 UTC
The Extremely Large Telescope now under construction and to become the largest optical telescope in history when it opens.
Artist's impression of the Extremely Large Telescope now under construction and set to become the largest optical telescope in history when it opens. Swinburne Astronomy Productions/ESO - ESO, CC BY 4.0

The first images from the JWST have dazzled the world, but someone is always looking for the next challenge. An even larger space telescope will require a significant upgrade on humanity's current launch capacity. Instead, a new generation of giant Earth-based telescopes are on their way, along with smaller space telescopes optimized for specific purposes. Some of the monster instruments under construction are expected to begin operations in just a few years and their immense scale is hard to grasp.


Sometimes Size Does Matter

Over the next three centuries after Galileo's first astronomical telescope apertures grew more than 100-fold, allowing them to collect more than 10,000 times as much light as the original. Then progress stalled. 

From 1949 to 1976 the largest telescopic mirror belonged to the 5.1 meter-wide (200 inches) Hale Telescope, known as the “Glass Giant of Palomar”. After the partial failure of the larger BTA-6 telescope, many astronomers ruefully concluded the limit for telescopes operating in the optical wavelengths had been reached. To see deeper into the universe we would have to put telescopes above the atmosphere.

The capacity to use active optics to operate smaller mirror segments as a single mirror, seen in the JWST's 18 hexagonal segments, restarted the race. The current record-holder, the Gran Telescopio Canarias, has a collecting area of 74 square meters, more than four times that of Hale (the combined size of the Large Binocular Telescope's mirrors are somewhat greater). That, however, is small compared to what is to come.

In the next decade, three giant instruments are expected to experience first light: the Giant Magellan Telescope (GMT), the Thirty Meter Telescope (TMT), and the Extremely Large Telescope (ELT). These will have respectively collecting areas of 368, 655, and 978 square meters – in the largest case almost 30 times greater than Hale.


By contrast, the JWST has a collecting area of 25.4 m2. Being in space is an immense advantage, of course, but not an infinite one. The ELT in particular is expected to exceed even the JWST's capabilities for many tasks, such as the direct spotting of Earth-sized planets around nearby stars.

Delays are not just for space telescopes; controversy over the location of the TMT telescope atop Mauna Kea in Hawai'i has led to construction being suspended. The GMT and ELT could strike problems of their own. Nevertheless, they are expected to see first light between 2027 and 2029, although in the GMT's case this will be with only four of its eventual seven mirrors, each of which takes several years to make.

Before then we can expect the Vera Rubin telescope – slightly smaller than the largest existing telescopes, but whose enormous field of view will allow it to photograph the entire sky at its location every few nights. First light is anticipated for next year, with full survey operations in 2024.

Comparison of the sizes of existing and planned telescope mirrors, and a tennis and basketball court for scale. Note that at this size the primary lenses on Gallileo's telescopes would be small to see.
Comparison of the sizes of existing and planned optical/infrared telescope mirrors, and tennis and basketball courts for scale. Note that at this size the primary lenses on Gallileo's telescopes would be too small to see. Image Credit: Cmglee; data on holes in mirrors provided by an anonymous user from IP - Own work. CC BY-SA 3.0

Don't Forget About Radio, Too

Telescopes that operate at radio wavelengths need to be much larger than those that collect light our own eyes can see, although fortunately they don't need the same precisely smoothed mirrors. The largest single-dish radio telescope in the world today is the Five-hundred-meter-Aperture Spherical radio Telescope (FAST). Radio-telescope arrays, such as the Very Large Array combine multiple dishes to have even larger collecting areas.

Here too, instruments are on their way that will far exceed anything currently in existence. The Square Kilometer Array (SKA) will be made up of hundreds of radio dishes in Australia and South Africa whose combined collection area is in the name.

The Australian core will consist of 100-meter-wide dishes at Murchison in Western Australia. South Africa's counterpart will be in the Meerkat National Park. Predecessor telescopes have already been built at both sites. The sites have been chosen for their “radio quiet”. With these telescopes operating at frequencies that include those used by FM radio, it's important not to drown out signals from billions of light-years away. Additional stations will be dotted across Africa and Australia, making the arrays able to operate for some purposes as if they were a single continent-sized dish.


The SKA will test general relativity with currently impossible precision, explore the universe before the first stars, map a billion galaxies, and advance the search for dark matter. They will also investigate a number of recently discovered radio sources we can't explain and provide us with our best chance of detecting signs of alien civilizations.

How the Australian node of the SKA at Murchison is likely to look. The instruments at the South African node are smaller
How the Australian node of the SKA at Murchison is likely to look. The instruments at the South African node are smaller. Image credit: SKA

Filling In the Niches

Big telescopes are expensive – the giants under construction all have budgets of billions of dollars; some may eventually exceed the JWST's $10 billion cost. Once built, demands on their time far exceed what is available. An alternative approach is to build smaller, cheaper telescopes carefully honed to do quite specific tasks. 

An extreme example of this is the TOLIMAN telescope, which has just one job: to find out if Alpha Centauri A or B have habitable planets. As comfortably the closest stars that resemble the Sun, planets orbiting this pair would be prime targets for the search for life, but none have yet been confirmed. The telescope's designer told IFLScience there was a possibility the instrument would prove useful for a handful of other nearby binary systems, but in reality, it was being launched to study “just two stars”. It will, however, cost thousands of times less than the JWST.


The Huntsman telescope, now in the tuning phase, is cheaper still. It combines 10 Canon telephoto lenses and it is expected to discover planets on distant orbits that TESS, NASA's planet hunter, has missed and answer questions about the formation of galaxies and individual stars.

The Nancy Grace Roman telescope is far more expensive and ambitious than these, but still significantly smaller, and hopefully cheaper, than the JWST. However, its wide field of view will allow it to explore large areas of the skies in infrared much more quickly than the JWST, particularly useful for exploring dark energy and conducting an exoplanet census

Right now, the JWST is exploring space like nothing else humanity has ever built, but soon these multitude of telescopes, with all their different functions, will contribute to our understanding of the cosmos like never before, and we can't wait. 

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