Connect with us

Published

on

Nuclear fusion holds huge promise as a source of clean, abundant energy that could power the world. Now, fusion researchers at a national laboratory in the US have achieved something physicists have been working towards for decades, a process known as “ignition”.

This step involves getting more energy out from fusion reactions than is put in by a laser.

But just how close are we to producing energy from fusion that can power people’s homes? While the ignition is only a proof of principle and the first step in a very long process, other developments are also in the works and together they could spark renewed enthusiasm for making fusion a practical reality.

First, it’s important to recognise that the latest result is indeed a real milestone.

The researchers at the National Ignition Facility (NIF) in California fired the world’s biggest laser at a capsule filled with hydrogen fuel, causing it to implode and starting fusion reactions that mimic what happens in the Sun.

The fusion energy released by the implosion was more than that put in by the laser, a massive achievement given that, just a few years ago, the NIF laser could only get out about a thousandth of the energy it put in.

However, around 10,000 times more energy had to be put into the laser than it produced in light energy.

It can only be run once a day. And every target is so exquisitely designed that each one costs thousands of dollars.

To produce a reactor for a working power station, you would need a laser that produced light energy at much greater efficiency (a few tens of percent) and shot targets successfully at ten times per second, with each target costing a few pence or so.

In addition, each laser shot would need to produce many times – perhaps 100 times – more energy out than was put in.

Very little research has actually been done on fusion “reactors”, where neutrons from the reactions would help drive a steam turbine to produce electricity. But there are other reasons for hope.

Firstly, while NIF has taken more than a decade to achieve ignition, during the same period, scientists have independently developed new lasers.

These use electronic devices called diodes to transfer energy to the laser and are very, very efficient, converting a good fraction of the electricity from the grid into laser light.

Prototype versions of such lasers have been proven to work at the rates of 10 times per second, which would be required for them to be useful in fusion.

These lasers are not yet of the size needed for fusion, but the technology is proven, and the UK leads in this type of research.

Also, the approach to fusion used by the scientists at NIF has some well-known, inherent inefficiencies, and there are several other ideas that could be much more effective.

Nobody is absolutely certain that these other ideas would work, as they have their own unique problems, and have never been tried at scale.

To do so would require hundreds of millions of dollars of investment for each of them with no guarantee of success (otherwise it would not be research).

However, there is now a wind of change blowing: the private sector.

Various funds with a very long-term outlook have started to invest in new start-up firms that are touting fusion as a commercially viable source of energy.

Given that it was private industry that has revolutionised the electric car market (and the rocket industry), maybe that sector could also give fusion the “kick” it requires.

Private firms can work a lot faster than governments, and pivot quickly to adopt new ideas when required.

Estimates of the total private funding in the sector now stand in excess of $2 billion (roughly Rs. 16,500 crore), peanuts compared with the $2 trillion (roughly Rs. 165 lakh crore) in revenue produced by the oil and gas industry each year.

There is still a lot of room in the marketplace for the high-risk, high-pay-off players.

The latest results show that the basic science works: the laws of physics do not prevent us from achieving the goal of unlimited clean energy from fusion.

The problems are technical and economic. While fusion may be too far off to solve matters on the timescale of a decade or two, the latest advance will at least bolster enthusiasm about solving one of humanity’s grand challenges.


Affiliate links may be automatically generated – see our ethics statement for details.

Continue Reading

Science

James Webb Telescope Detects Potential Gas Giant Exoplanet Just 4 Light-Years Away

Published

on

By

James Webb Telescope Detects Potential Gas Giant Exoplanet Just 4 Light-Years Away

New observational evidence from the James Webb Space Telescope (JWST), which has yet to launch, may change that. JWST astronomers have found tantalising hints of an orbiting gas giant around Alpha Centauri A, the closest Sun-like star to us. Located just four light-years away in the Alpha Centauri triple-star system, the potential planet sits within the star’s habitable zone — the region where liquid water could exist — but its gas giant nature makes it inhospitable to life. Even so, its location and distinctiveness make the detection among the most captivating detections in exoplanetary exploration prior.

JWST Unveils Possible Closest Sun-Like Star Exoplanet, Awaiting Confirmation

According to a NASA report, this was done with the JWST Mid-Infrared Instrument (MIRI) using a coronagraphic mask to block out stellar glare. This method caught sight of an object which is almost 10,000 times fainter than Alpha Centauri A and at a separation of around two astronomical units. If upheld, it would be the nearest exoplanet to a similar being ever pictured and, moreover, the first healthy globe discovered in direct significance.

Researchers noted that while Alpha Centauri already hosts two confirmed planets around the red dwarf Proxima Centauri, no planet has yet been confirmed around Alpha Centauri A. Follow-up JWST observations did not capture the planet again, possibly because it was too close to the star during the imaging. Computer simulations support this possibility.

The team wants to look for more evidence using both JWST and the yet-to-be-launched Nancy Grace Roman Space Telescope, due in May 2027. Confirmation would represent a watershed moment in planetary system science, where astronomers are looking into embryonic solar systems around other stars.

Researchers said the potential planet’s existence in such a dynamic binary star system could challenge current models of planetary formation and survival. Two papers detailing the findings have been accepted for publication in The Astrophysical Journal Letters.

Continue Reading

Science

Earliest Known Black Hole Found Just 500 Million Years After the Big Bang

Published

on

By

Earliest Known Black Hole Found Just 500 Million Years After the Big Bang

Astronomers have discovered the most distant black hole yet, an ancient quasar more than 13 billion light years from our own Earth, incredibly close to the limit of where scientists even expect supermassive black holes to form. The cosmic behemoth of a galaxy, known as CAPERS-LRD-z9, provides a wide-window echo back in time to one of the furthest peeks into our early universe yet, only shortly after the Big Bang, when our cosmos was a fraction (3%) of its current age. Now, researchers led by those in The University of Texas at Austin’s Cosmic Frontier team have found what are likely very powerful gas outflows and also evidence that some of the very first black holes were born much, much heavier than previously believed.

Early Black Hole Found in ‘Little Red Dot’ Galaxy Challenges Growth Models

According to a study published in The Astrophysical Journal this week, researchers led by those at The University of Texas at Austin’s Cosmic Frontier team are announcing they have made the most sensitive measurements to date less than a billion years after the Big Bang, and these neonatal black holes were producing gas outflows fast enough — and over a long enough period — to halt stars forming in surrounding galaxies.

More recently discovered, the Little Red Dots galaxy appears to be just the sort of ominous-sounding crimson that would shoot a vibrant deep red due to intense radiation taking place among giant black holes and gas clouds.

A little galaxy of mass in all that more than enough of less, those hundreds of millions of suns among which all those stars are caught. This, in turn, birthed the supermassive galactic monsters — either quickly overcooked giants or premature sizes.

JWST high-z key science theme & imaging science exposure for mapping the process of supermassive black hole formation, growth, and evolution at high spatial detail.

Continue Reading

Science

Greenland’s Melting Glaciers Feed Ocean Life, Study Finds

Published

on

By

Greenland's Melting Glaciers Feed Ocean Life, Study Finds

The process of Greenland’s ice sheet melting is not only raising sea levels, it is also feeding life in the ocean. As the most productive for marine life, phytoplankton harvesting energy from this nutrient-filled climate change is altering how this biological pump works in these warming ares. In a new study, scientists employed cutting-edge computer models to simulate the intricate movements of ice melt and seawater with ocean currents and marine biology behaviour finnesing adding more detail to an understanding of these unseen forces between Earth’s shifting polar zones.

Glacial Melt Fuels a Surge in Ocean Life

According to precious study, each summer Jakobshavn Glacier releases more than 300,000 gallons of freshwater per second into the sea. This less-dense meltwater shoots upward through heavier, salty seawater, dragging deep-sea nutrients—like iron and nitrate—toward the sunlit surface. These nutrients are essential for phytoplankton, which are the foundation of the ocean food chain.

In recent decades, NASA satellite data recorded a 57% surge in Arctic phytoplankton, and scientists now have a clearer picture of why. The nutrient boost is especially crucial in late summer, when spring blooms have already depleted surface waters. Without direct access to such remote regions, researchers had long struggled to test the nutrient-plume hypothesis—until now.

NASA’s Digital Ocean Brings Clarity Beneath the Ice

To simulate the chaotic waters of Greenland’s fjords, researchers used the ECCO-Darwin model, developed by NASA’s Jet Propulsion Laboratory and MIT. Fueled by billions of ocean measurements—temperature, salinity, pressure—this model replicates how biology, chemistry, and physics interact. Using NASA’s supercomputers at Ames Research Center, the team calculated a 15–40% increase in phytoplankton growth from glacial nutrients.

Yet more change looms: as melting accelerates, seawater may lose its ability to absorb CO₂ even as plankton pull more of it in. “Like a Swiss Army knife,” said researcher Michael Wood, “this model helps us explore ecosystems far beyond Greenland.”

Continue Reading

Trending