🧠 A brain floating in space — and it’s real
NASA’s James Webb Space Telescope just released the sharpest images ever taken of nebula PMR 1, nicknamed the “Exposed Cranium” — because it looks almost exactly like a human brain inside a transparent skull.
PMR 1 is a planetary nebula — an expanding shell of ionized gas and dust expelled by a star in the final stages of its life, as the nuclear fuel in its core runs out.
Webb captured it in both near- and mid-infrared light. The images reveal a distinctive dark lane running vertically through the center, dividing the nebula into two lobes — just like left and right brain hemispheres. That eerie split is likely carved by twin polar jets blasting outward from the dying star at its core.
The central star is several times more massive than our Sun and is just a few thousand years from its ultimate fate — either a spectacular supernova or a quiet collapse into a white dwarf. Scientists aren’t sure yet which way it will go.
The nebula was first spotted by the Spitzer telescope back in 2013, but Webb’s more advanced instruments now reveal features that were previously invisible, making its brain-like structure stand out with unprecedented clarity.
The universe has a sense of aesthetics.
🔗 Source: https://science.nasa.gov/missions/webb/nasas-webb-examines-cranium-nebula/
#space #JWST #astronomy #nebula #science
NASA’s James Webb Space Telescope just released the sharpest images ever taken of nebula PMR 1, nicknamed the “Exposed Cranium” — because it looks almost exactly like a human brain inside a transparent skull.
PMR 1 is a planetary nebula — an expanding shell of ionized gas and dust expelled by a star in the final stages of its life, as the nuclear fuel in its core runs out.
Webb captured it in both near- and mid-infrared light. The images reveal a distinctive dark lane running vertically through the center, dividing the nebula into two lobes — just like left and right brain hemispheres. That eerie split is likely carved by twin polar jets blasting outward from the dying star at its core.
The central star is several times more massive than our Sun and is just a few thousand years from its ultimate fate — either a spectacular supernova or a quiet collapse into a white dwarf. Scientists aren’t sure yet which way it will go.
The nebula was first spotted by the Spitzer telescope back in 2013, but Webb’s more advanced instruments now reveal features that were previously invisible, making its brain-like structure stand out with unprecedented clarity.
The universe has a sense of aesthetics.
🔗 Source: https://science.nasa.gov/missions/webb/nasas-webb-examines-cranium-nebula/
#space #JWST #astronomy #nebula #science
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🌌 The Ingredients for Planets Were Spreading Through Space Just 500 Million Years After the Big Bang
The newborn universe started simple.
After the Big Bang, almost everything was hydrogen and helium. Carbon, oxygen, silicon and nearly every other element needed to build planets — and eventually us — had to be manufactured later inside stars.
Astronomers expected that process to take time.
JWST has now shown that it happened remarkably fast.
Researchers analyzed nearly 30 hours of Webb observations of three galaxies seen as they existed roughly 500–700 million years after the Big Bang.
They found unmistakable chemical fingerprints of carbon, oxygen and silicon in gas associated with the galaxies.
But the really interesting part was where that gas was going.
The absorption signatures were blueshifted by roughly 50–250 km/s, indicating that metal-enriched material was moving outward from the galaxies — consistent with powerful galactic winds carrying newly forged elements into surrounding space.
That means an entire cosmic recycling system was already operating while the universe was only about 3% of its present age.
Stars formed.
They forged heavier elements.
Stellar winds and explosions returned those elements to their galaxies.
And galaxies began spraying them outward, chemically transforming the surrounding universe.
Remarkably, the chemical fingerprints look similar to those seen around galaxies billions of years later.
The result may also help solve another mystery.
Astronomers have spent decades searching for Population III stars — the hypothetical first generation of stars, made almost entirely from pristine hydrogen and helium.
None has ever been conclusively found.
If early galaxies contaminated their surroundings with heavier elements this quickly, the window in which truly pristine stars could form may simply have been much shorter than expected.
Important caveat: the result comes from only three unusually bright early galaxies. We don’t yet know whether such rapid enrichment was universal across the young cosmos.
Still, the implication is striking.
Only half a billion years after the Big Bang, the universe had already started distributing the carbon in our bodies, the oxygen in our water and the silicon beneath our feet.
Cosmic chemistry apparently wasted very little time.
#JWST #Space #Astronomy #Cosmology #BigBang #EarlyUniverse #Science
https://www.nature.com/articles/s41550-026-02988-2
The newborn universe started simple.
After the Big Bang, almost everything was hydrogen and helium. Carbon, oxygen, silicon and nearly every other element needed to build planets — and eventually us — had to be manufactured later inside stars.
Astronomers expected that process to take time.
JWST has now shown that it happened remarkably fast.
Researchers analyzed nearly 30 hours of Webb observations of three galaxies seen as they existed roughly 500–700 million years after the Big Bang.
They found unmistakable chemical fingerprints of carbon, oxygen and silicon in gas associated with the galaxies.
But the really interesting part was where that gas was going.
The absorption signatures were blueshifted by roughly 50–250 km/s, indicating that metal-enriched material was moving outward from the galaxies — consistent with powerful galactic winds carrying newly forged elements into surrounding space.
That means an entire cosmic recycling system was already operating while the universe was only about 3% of its present age.
Stars formed.
They forged heavier elements.
Stellar winds and explosions returned those elements to their galaxies.
And galaxies began spraying them outward, chemically transforming the surrounding universe.
Remarkably, the chemical fingerprints look similar to those seen around galaxies billions of years later.
The result may also help solve another mystery.
Astronomers have spent decades searching for Population III stars — the hypothetical first generation of stars, made almost entirely from pristine hydrogen and helium.
None has ever been conclusively found.
If early galaxies contaminated their surroundings with heavier elements this quickly, the window in which truly pristine stars could form may simply have been much shorter than expected.
Important caveat: the result comes from only three unusually bright early galaxies. We don’t yet know whether such rapid enrichment was universal across the young cosmos.
Still, the implication is striking.
Only half a billion years after the Big Bang, the universe had already started distributing the carbon in our bodies, the oxygen in our water and the silicon beneath our feet.
Cosmic chemistry apparently wasted very little time.
#JWST #Space #Astronomy #Cosmology #BigBang #EarlyUniverse #Science
https://www.nature.com/articles/s41550-026-02988-2
Nature
Early metal-enriched baryon cycling before the midpoint of cosmic reionization
Nature Astronomy - Deep JWST spectra of three galaxies seen within the Universe’s first 700 million years allow the detection of blueshifted, chemically enriched gas, providing evidence that...
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