Stars, supernovae, black holes and stellar remnants

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Unique shape of star’s explosion revealed just a day after detection

12 November 2025

Swift observations with the European Southern Observatory’s Very Large Telescope (ESO’s VLT) have revealed the explosive death of a star just as the blast was breaking through the star’s surface. For the first time, astronomers unveiled the shape of the explosion at its earliest, fleeting stage. This brief initial phase wouldn’t have been observable a day later and helps address a whole set of questions about how massive stars go supernova.

https://www.eso.org/public/news/eso2520/


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Credit: ESO/L. Calçada
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The Longest Gamma Ray Burst Ever Detected Is an Intriguing Puzzle
By Evan Gough
December 9, 2025

Introduction:
(Universe Today) Gamma-ray bursts (GRB) are some of the most perplexing phenomena in Nature. Even though astronomers have detected about 15,000 of them, with a new one each day, they're still mysterious. They're the most luminous, energetic explosions in the Universe, and typically last only a few milliseconds, or a few minutes, with a handful of them lasting for a few hours.

GRBs that last longer than about two seconds typically come from supernova explosions where a high-mass star reaches the end of its life and collapses into a black hole. They produce focused, energetic jets that are ultrarelativistic.* The tight focus of the jets means that most GRBs miss the Earth and are never detected, and all GRBs detected so far have been in distant galaxies.

When a GRB on July 2nd, 2025 lasted for seven hours, it highlighted how uncertain astronomers are about their causes.

The July 2nd GRB is named GRB 250702B and at seven hours long, it's the longest one ever detected. It lasted almost twice as long as the next longest-known GRB. In fact, it endured for so long that no single telescope could follow it.
Additional extract:
There are two likely explanations for this GRB, though neither are totally certain. Both involve a black hole eating its stellar companion.
Read more here: https://www.universetoday.com/articles ... ng-puzzle

*In physics, a particle is called ultrarelativistic when its speed is very close to the speed of light.

Source of Definition: https://en.wikipedia.org/wiki/Ultrarelativistic_limit
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Supernova from the dawn of the universe captured by James Webb Space Telescope
https://phys.org/news/2025-12-supernova ... james.html
by University College Dublin
An international team of astronomers has achieved a first in probing the early universe, using the James Webb Space Telescope (JWST), detecting a supernova—the explosive death of a massive star—at an unprecedented cosmic distance.

The explosion, designated SN in GRB 250314A, occurred when the universe was only about 730 million years old, placing it deep in the era of reionization. This remarkable discovery provides a direct look at the final moments of a massive star from a time when the first stars and galaxies were just beginning to form.

The event, which has been reported on in the recently published academic paper JWST reveals a supernova following a gamma-ray burst at z ≃ 7.3, (Astronomy & Astrophysics, 704, December 2025), was initially flagged by a bright burst of high-energy radiation, known as a long-duration Gamma-Ray Burst (GRB), detected by the space-based multi-band astronomical Variable Objects Monitor (SVOM) on March 14, 2025. Follow-up observations with the European Southern Observatory's Very Large Telescope (ESO/VLT) confirmed the extreme distance.
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Re: Stars, supernovae, black holes and stellar remnants

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A Black Hole Flare Launches a Relativistic Wind
By Philip Plait
January 6, 2026
Introduction:
(Bad Astronomy) NGC 3783 is a spectacular face-on spiral galaxy about 125 million light-years from us. In its exact center is a supermassive black hole, some 30 million times heftier than our Sun (about 7 times more massive than Sgr A*, the central black hole in our Milky Way). It’s actively feeding, meaning material like gas is falling into it. As it does, this matter forms an accretion disk that gets very hot, and glows brightly.

These disks are made of ionized gas, material with electrons stripped away from their parent atoms. Moving charged particles make a magnetic field, so the NGC 3783 disk has a powerful field embedded in it.

The magnetic field lines — the loops you can see when, for example, iron filings are spread around a bar magnet — store a vast amount of energy, and aren’t always stable. I like the analogy of a bag full of giant metal springs that have been bent and the ends very gently connected. If one snaps it sproings straight and releases its energy, slapping into other springs and triggering them too, generating a cascade you don’t want to stick your hand in. You get a huge burst of energy.

Same thing here. The magnetic field lines in the accretion disk can snap and release their energy, making a runaway effect, and it can be soul-chillingly powerful blast, outshining the entire galaxy at some wavelengths. In 2024 just such a flare was seen from NGC 3783, a blast of X-rays so powerful it was equal to 10 billion times the Sun’s luminosity! [link to journal paper] :https://www.aanda.org/articles/aa/full_ ... tmosphere

But it did more than that: the data indicate that the explosion also sent out a huge blast of subatomic particles, what we call a wind, accelerated to immense speed. The wind velocity was measured to be a staggering 57,000 kilometers per second, or about one-fifth the speed of light! To get an idea of how much energy was involved in this, only about 10% of the energy went into the X-ray flare, the other 90% went into blasting out this material. So, 90 billion times the energy the Sun produces every second.
Read more here: https://badastronomy.beehiiv.com/p/a-b ... mosphere
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Intricacies of Helix Nebula Revealed With NASA’s Webb

https://science.nasa.gov/missions/webb/ ... asas-webb/
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