
Time-series images made by cameras onboard the Hubble Space Telescope show the evolution of the inner remnant of Supernova 1987A
This well-known supernova remnant in a neighboring galaxy has been studied for more than 10 years, but the recent observations could glean new knowledge of how such stellar debris helps shape the evolution of galaxies.
The new study, led by Kevin France, a research associate at the Center for Astrophysics and Space Astronomy at the University of Colorado in Boulder, targeted the remnants of star SN1987A, which was first discovered in 1987.
Stars like this that have at least eight times the mass of our sun are considered "massive" stars, France said, and they speed toward death very quickly. Unable to support their weight any longer, these stars end their lives by collapsing in spectacular supernova explosions.











