Researchers have applied a physics-informed neural network to the problem of accretion disks, successfully reproducing key features like spiral density waves while solving problems faced by numerical models.

The binary Kuiper Belt object 2016 BP81 appears to belong to a small and newly identified group of objects that differs from other water-type Kuiper Belt objects, hinting at a different formation environment.

Using magnetohydrodynamics simulations, researchers predicted the spectral signals of chromospheric magnetic reconnection, which is thought to be responsible for phenomena like ultraviolet bursts and jets.

Large moons orbiting habitable-zone planets around M-dwarf stars appear to be unstable; if large moons enhance the habitability of their planets, this result has implications of the potential number of habitable planets in the galaxy.

Using three-dimensional covariant magnetohydrodynamics simulations to track the accretion of magnetized gas onto black holes, researchers have probed how black hole jets extract spin energy.

Simulations show that the accretion disks that form in nova and Type Ia supernova progenitor systems are partially or totally destroyed by an explosion, which will impact subsequent explosions.