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
The Sun is increasing its intensity on schedule, continuing its approach to solar maximum. In…
Does another undetected planet languish in our Solar System's distant reaches? Does it follow a…
It's that time again. NIAC (NASA Innovative Advanced Concepts) has announced six concepts that will…
On Friday, May 3rd, the sixth mission in the Chinese Lunar Exploration Program (Chang'e-6) launched…
Earth is the only life-supporting planet we know of, so it's tempting to use it…
Multiple space agencies are looking to send crewed missions to the Moon's southern polar region…