“A team of scientists have discovered an eclipsing binary located in the Cassiopeia constellation, designated CSS J0031068+313347. This remarkable astronomical object is composed of two stars locked in a close orbit, orbiting each other every 1.7 days. By studying the data collected from this binary system, the team has determined that the two stars are both white dwarfs and that they have a combined mass of 0.6 times the mass of the Sun. This discovery is the first of its kind and is an important step forward for our understanding of stellar evolution.”

The team of scientists have recently made an incredible discovery of an eclipsing binary located in the Cassiopeia constellation. CSS J0031068+313347 is the first of its kind, consisting of two white dwarf stars orbiting each other with a period of 1.7 days. This groundbreaking find is an important step forward in our understanding of stellar evolution. With further research, we may learn more about the formation and fate of such binary systems.

Read Full Article Here

source: Phys.org