Alex McColgan
speaker
28,875 appearances
103 recordings
1 series
first heard Nov 2024
last heard 2d ago
Alex McColgan’s voice in public audio — every appearance, attributed to the second.
Trend
recordings per month · last 12 monthsRecordings per month over the last 12 months — 67 in all, peaking in Aug 2026 with 11.
Appearances
Even as we burn through our dwindling fossil fuel reserves and climate chaos intensifies all around us, every year our energy requirements rise by an estimated 1-2%.
The
need for a clean, efficient and inexhaustible energy source has never been so acute.
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For many decades, this has been the promise of nuclear fusion.
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Unlike nuclear fission, which splits rare and unstable isotopes to generate power, fusion technology aims to replicate the processes that happen inside our sun, fusing hydrogen into helium, and releasing a huge amount of energy in the process.
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Yet since fusion was first talked about as a serious contender for energy generation in the 1950s, it has become a cliché that is perpetually 30 years away from becoming reality.
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So why then does it seem that fusion is always just out of reach?
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And do the new private enterprises that have recently entered the field really offer any hope of shaking things up?
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To begin to answer these questions, there is no better place to start than the place that inspired fusion science in the first place, our sun.
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As strange as it sounds now, at the turn of the last century, we didn't know what powered the sun.
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The source of the heat and light that sustains all of life on Earth was a mystery.
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The leading theory was that the Sun's energy came from gravitational contraction.
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Simply put, the idea proposed that as a star gradually radiates energy to space, it cools, and so collapses further under its own gravity, which in turn causes gravitational potential energy to be converted into heat in the star's core.
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Today, we know that is a genuine process.
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Not only is it involved in the formation of stars, it's also the reason that the gas giant Jupiter radiates more energy to space than it receives from the Sun.
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In fact, the planet is shrinking by about 2cm every year under its own gravity.
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And as the resultant internal heat works its way from deep in Jupiter's interior and out into space, it drives the intense storms that dance
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across the planet's surface.
But when it comes to powering a star, one scientist
realized that contraction didn't stand up.
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Showing 1721–1740 of 28,875 · page 87 of 1444
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