Alex McColgan
speaker
27,837 appearances
101 recordings
1 series
first heard Nov 2024
last heard 5d ago
Alex McColgan’s voice in public audio — every appearance, attributed to the second.
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recordings per month · last 12 monthsRecordings per month over the last 12 months — 65 in all, peaking in Aug 2026 with 11.
Appearances
A collection of a few dozen neighbouring galaxies near to our own.
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Our local group belongs to a larger collection called the Laniakea supercluster, which contains some 100,000 galaxies and measures five hundred million light years across.
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As you might have guessed, all these galaxies are strung along the cosmic web like beads on strings perched along the edge of great voids.
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But even though we've been mapping this cosmic web for decades, most of what we can see is the beads, the distribution of galaxy clusters along the web, not the strings that hold them together or the filaments themselves.
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Or is it?
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Whilst most of the visible matter in the universe is tied up in galaxies,
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Not all of it is.
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The dark matter in the cosmic web has a pretty strong pull itself.
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There, bound up as vast diffuse gas in those long strings or filaments, is where large scale cosmological simulations have predicted we might not only find dark matter, but our missing visible matter too.
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This low density, diffuse gas is known as the warm hot intergalactic medium.
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But simulations are one thing, detecting these diffuse filaments is another.
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And this is where historically, we've not had much luck.
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Although that started to change about 20 years ago.
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In 2005, NASA's Chandra X-ray Observatory imaged two huge intergalactic clouds of diffuse gas.
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We'd seen clouds like this around our own galaxy and in others local to us, but not between distant galaxies.
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Could it be gas on the cosmic web?
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This was some of the first evidence that the cosmic web was hiding our missing mass.
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but the light was too faint to completely isolate it, so scientists couldn't quite be sure
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Then in twenty twelve a combination of eighteen Hubble images was used to infer the presence of a filament funneling matter into the galaxy cluster Max J0717.
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Scientists found it by studying the distortion of light from background galaxies due to the gravity of the filament's dark matter.
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Showing 1421–1440 of 27,837 · page 72 of 1392
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