The first birth of a magnetar, caught live
In 2024, a distant supernova called SN 2024afav started doing something no one had seen before. Its light was chirping.
Not a steady blaze, but a rhythmic brightening and fading that sped up as the weeks passed, like a top slowly winding down [4]. Graduate student Joseph Farah at Las Cumbres Observatory brought the data to UC Berkeley astrophysicist Dan Kasen, who had published a theory about this exact signal sixteen years earlier and never had confirmation. His 2010 paper, cowritten with Lars Bildsten, proposed that the universe's most brilliant supernovae stay bright long after they should fade because the dying core collapses into a magnetar: a neutron star about ten miles across, spinning more than a thousand times per second, with a magnetic field a hundred to a thousand times stronger than a typical pulsar. Spinning at that rate, it pumps energy into the surrounding explosion like a battery, keeping it blazing. SN 2024afav's chirp matched the theory exactly, and the precise timing required Einstein's general relativity to decode, making this the first time general relativity has been used to explain how a supernova actually works. The results were published in Nature [4].





