May 15, 2025

On the left the supernova SN 1987A remnant as seen by the James Webb Space Telescope, and in the other two panels the simulation of the density distribution of the remnant, which include the iron-rich materials, and the current morphology of that remnant

An article to be published in the journal “Astronomy & Astrophysics” reports a study of the supernova SN 1987A that offers evidence that the explosion was decidedly asymmetric and dominated by two bipolar jets. A team of researchers led by astrophysicist Salvatore Orlando of the Italian National Institute of Astrophysics in Palermo has developed a model that takes into account the interaction between matter and magnetic field to study the evolution of SN 1987A. The results successfully reproduce the morphology of the iron-rich ejected materials, which was observed in particular by the James Webb Space Telescope. This shows that those structures are the result of an asymmetric explosion.