Orions Arm even has a story about how such process might look like: https://www.orionsarm.com/eg-article/46709da5de6be
You basically let material stream into a black hole, it forms an acreation disk which gets very hot and dense even before the material actually falls into the black hole. The temperatture and pressure is high enough to trigger nucleosynthetic fusion reactions that generate heavy elements from lighter stuff, like the abundant hydrogen and helium. And a lot of "process heat" that can be used as energy source for other purposes. :)
Joking aside, it could be a Kardashev Type II (or higher) civilization. https://en.wikipedia.org/wiki/Kardashev_scale
They could have used a dense Dyson sphere to “suck” the energy of the star, but if that was the case we would be able to detect its infrared radiation. https://en.wikipedia.org/wiki/Dyson_sphere
Anyway, I prefer the giant star eating dragon alternative ;-)
It was multi-wave analysis not just visible light, IR spread can differentiate this.
It’s been missing since 2015. Probability of something being large enough to cover the star and stay on a path completely obscuring it for 10 years is shall we say, not likely.
It didn’t rage against the dying of the light, it just switched off.
Stellar cores are relatively small, and the infalling matter is essentially in freefall at high g, gets to a significant fraction of c in about 0.1 seconds.
The visible disk of a red supergiant — of the kind that can supernova or surprise us by failing — is on the order of multiple AU radius, so speed of light limits there are in the tens of minutes.
Imagine seeing that up fairly close - a massive star just shrivel into a black hole and wink out.
https://open.clemson.edu/cgi/viewcontent.cgi?article=1006&co...
bell-cot•7h ago
Is there an astrophysicist in the house?
metalman•6h ago
madaxe_again•5h ago
MoonGhost•5h ago
magicalhippo•2h ago
But yeah, just a layman so hopefully someone knowledgeable chimes in.
[1]: https://doi.org/10.1093/mnras/staa863
[2]: https://doi.org/10.3847/1538-4357/acda94
[3]: https://arxiv.org/abs/2503.23856