XMM-Newton’s View of Supernova 1987A
And in the X-ray spectrum, SN 1987A is quite spectacular. It outshines all the nearby X-ray sources, and it’s now 10 times brighter than it was when XMM-Newton first observed it back in 2000. The X-rays we see are generated when the expanding supernova shock wave interacts with the surrounding material.
The data gathered by XMM-Newton will help scientists understand how a supernova remnant forms, and eventually reveal the neutron star spinning at the centre.
Original Source: ESA News Release
Recent Posts
China Creates a High-Resolution Atlas of the Moon
Multiple space agencies are looking to send crewed missions to the Moon's southern polar region…
Dinkinesh's Moonlet is Only 2-3 Million Years Old
Last November, NASA's Lucy mission conducted a flyby of the asteroid Dinkinish, one of the…
The Universe Could Be Filled With Ultralight Black Holes That Can't Die
Steven Hawking famously calculated that black holes should evaporate, converting into particles and energy over…
Starlink on Mars? NASA Is Paying SpaceX to Look Into the Idea
NASA has given the go-ahead for SpaceX to work out a plan to adapt its…
Did You Hear Webb Found Life on an Exoplanet? Not so Fast…
The JWST is astronomers' best tool for probing exoplanet atmospheres. Its capable instruments can dissect…
Vera Rubin’s Primary Mirror Gets its First Reflective Coating
First light for the Vera Rubin Observatory (VRO) is quickly approaching and the telescope is…