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A Hot Star Built a Sulfur Factory

Original: "Discovery of sulfur oxides in the ejecta of a B[e] supergiant"
arXiv:2607.02191v1 · 2026-07-02 · CC BY 4.0 · ⏱ 2 min · Stellar
For the first time, molecules of sulfur oxides have been found around a massive star, created by its own ultraviolet radiation.
Abstract

Scientists have for the first time found sulfur molecules (like sulfur dioxide) around a rare massive star, even though it was thought its radiation destroys any chemistry. It's like discovering an oasis in the desert, where life bustles against all odds. The finding hints that similar stars may have influenced the sulfur composition on ancient Earth. What other secrets do these cosmic giants hold?

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A hot supergiant, dozens of times more massive than the Sun, blazes so intensely that its ultraviolet light can tear apart nearly any molecule. Such stars live fast and die young, ending their lives as a supernova — a cataclysm scrutinized by Fritz Zwicky. Conventional wisdom held that complex molecules couldn't survive near such behemoths, save for the toughest ones like CO (carbon monoxide). But when astronomers aimed the ALMA radio telescope array at the exceptionally rare star HD 87643, the view was different. Using spectroscopy — a technique pioneered in the 19th century by Johann Balmer to decode starlight — they uncovered a host of sulfur molecules: SO, SO₂, and more.

The star's light acts not like a wrecking ball, but like a master chef: it 'carves up' some compounds and 'prepares' others, driving nearly all the sulfur into SO₂.

Most unexpected was the behavior of sulfur isotopes — atoms with slightly different masses. Under normal conditions, in the universe, the light isotope ³²S is 127 times more abundant than the heavy ³³S. Here, the ratio was only 15. Scientists explain this by the star's ultraviolet light selectively destroying molecules containing the lighter isotope — much like a strong flame chars delicate foods faster on a skillet. This gives rise to non-equilibrium photochemistry, similar to what once simmered in the young Earth's atmosphere and left traces in ancient minerals. As Margaret Burbidge established, massive stars forge heavy elements, including sulfur, by burning hydrogen and helium in their cores, then scatter them across the galaxy.

The isotope shift at the star matches what is seen in Archean rocks on Earth. Now astronomers can observe this process in real time in space.

The discovery shows that chemistry around massive stars is far richer than assumed. Their surroundings can serve as natural reactors where molecules important for prebiotic evolution are born. Further observations will help clarify exactly how complex substances accumulated in the early history of the cosmos.

🎯 The SO₂ molecule is familiar to everyone from the smell of a burnt match. Around the star, there's so much of it that a cloud roughly a thousand times larger than our Solar System would smell like volcanic gases and burning sulfur combined.

🎬 A veritable 'sulfur factory' at the star HD 87643 brings to mind the sulfur-based alien life from Star Trek.

OH + SO \rightarrow H + SO_2
An OH molecule and sulfur monoxide SO combine to yield sulfur dioxide SO₂ and a hydrogen atom.
Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
spectroscopy supernova carbon hydrogen entropy galaxy helium big bang
Laws
Friedmann equationsHubble's lawsecond law of thermodynamicsDoppler effectBekenstein-Hawking entropyCoulomb's law
Original: arXiv:2607.02191v1 · CC BY 4.0 · bridge42worlds