Supernovae help astronomers measure how the Universe expands over time
Astronomers have leaned on Type Ia supernovae for decades because these stellar explosions act like mile markers across the cosmos. You simply measure how bright one appears, and then compare that with how bright it ought to be. After that, you can estimate how far away it is. Additionally, when you stack enough of those measurements together, a picture of how the Universe has expanded over time begins to emerge. That picture, though, is never as clean as it sounds. The light from a supernova reaches Earth carrying more than one message at once. Part of it reflects the explosion itself. Part of it is shaped by the star that blew apart, including its age and chemical makeup. Another part has been dimmed or reddened by dust in and around the galaxy where the blast happened. And part of it has been stretched by the expansion of the Universe. A new analysis from Konstantin Karchev and Roberto Trotta of SISSA, working with Raúl Jiménez of the University of Barcelona, tries to sort out those overlapping …









