These two stellar siblings don't seem to like each other very much. But it's OK, they make up in the end.
These two stellar siblings don't seem to like each other very much. But it's OK, they make up in the end.
White dwarfs may technically be the remnants of dead stars, but could they provide a steady, long-term energy source to alien life?
Nothing lights up the cosmos like a supernova. But why does a star explode to begin with?
Measuring the influence of dark energy on the universe is a tricky business, but refining our understanding of Type Ia supernovae may uncover the true nature of this mysterious force.
Trace metals consistent with rocky, possibly watery bodies have been discovered in stars far beyond our solar system.
HM Cancri has been confirmed as a binary system of two white dwarfs orbiting one other so close, they complete one orbit every 5.4 minutes. With a year this short, it's little wonder HM Cancri is a record breaker!
Explosions that scientists have long used to measure the universe are finally explained as merging, dying stars.