Question...? Are you a Swiftie? We are too! Our Neil Gehrels Swift Observatory telescope and several other X-ray telescopes observed one of the most extreme rotating neutron stars or pulsars – ever detected in 2016. Swift Observatory helps detect gamma-ray bursts – large gamma radiation pulses which form when a massive star collapses, creating a black hole – using optical, ultraviolet, and X-ray light. This composite image shows the remains of a supernova, around 9,000 light-years from Earth, in three bands of X-ray light detected by @NASAChandraXRay, with low energy X-rays in red, medium in green, and the highest in blue. Image description: Blank space as black as #Midnight is dotted with tiny white stars across the image. A swirling labyrinth of colors of blue, green, yellow, purple, and red makes up the center of the photo surrounding the neutron star in bright blue. Credit: NASA/CXC/University of Amsterdam/N.Rea et al; Optical: DSS #Supernova #Star #NeutronStar #Galaxy #Space #Xray #Universe #NASA