We recently shared the story of Blender’s role in the adult animated series Il Baracchino, and now, a fascinating new article by Ph.D. student MohammadHossein Jamshidi showcases how he applied Geometry Nodes in his cosmology research.

Cosmology is the study of the universe and its fundamental nature. MohammadHossein Jamshidi, from Shahid Beheshti University in Iran, has also worked as an animation engineer in the game industry since 2012. His initial inspiration to apply Blender to scientific work came from the creative projects of Seanterelle, which led him to experiment with using Geometry Nodes for cosmological computations.

In the article, he shares several ideas and techniques for using Blender in his research, and he believes that these approaches could be applied to other areas of science as well. All the files featured are freely available on this GitHub repository.

A restarted black hole in J1007+3540 reveals how episodic jet activity and cluster pressure sculpt giant radio galaxies. Astronomers have captured one of the clearest views yet of a black hole returning to life, in a vast radio galaxy where activity stretches nearly one million light-years across

That the universe is expanding has been known for almost a hundred years now, but how fast? The exact rate of that expansion remains hotly debated, even challenging the standard model of cosmology. A research team at the Technical University of Munich (TUM), the Ludwig Maximilians University (LMU) and the Max Planck Institutes, MPA and MPE, has now imaged and modeled an exceptionally rare supernova that could provide a new, independent way to measure how fast the universe is expanding. The studies are published on the arXiv preprint server.

The supernova is a rare superluminous stellar explosion, 10 billion light-years away, and far brighter than typical supernovae. It is also special in another way: the single supernova appears five times in the night sky, like cosmic fireworks, due to a phenomenon known as gravitational lensing.

Two foreground galaxies bend the supernova’s light as it travels toward Earth, forcing it to take different paths. Because these paths have slightly different lengths, the light arrives at different times. By measuring the time delays between the multiple copies of the supernova, researchers can determine the universe’s present-day expansion rate, known as the Hubble constant.

An international team of astronomers has performed multi-wavelength observations of the nearby Araish galaxy to investigate the origin of its radio emission. As a result, they detected an extended radio jet of this galaxy. The finding was reported February 11 on the arXiv pre-print server.

Observations show that powerful radio jets are commonly observed in elliptical galaxies or massive quasars. However, their presence in spiral galaxies is relatively rare. These systems, known as spiral double radio-source associated with galactic nuclei (DRAGNs), are therefore unique galaxies where classical disk morphology coexists with large-scale radio jets.

What if the Milky Way’s central “black hole” isn’t a black hole at all? A new model proposes that an ultra-dense dark matter core could mimic its gravitational pull.