Exploring the Universe: The Power of the X-ray Multi Mirror Satellite

The X-ray Multi Mirror (XMM) satellite is the most powerful X-ray telescope in orbit, operating in a 48-hour elliptical orbit to avoid Earth's X-ray interference. It captures detailed images by penetrating dust clouds, revealing new insights into supernovae and black holes. The X-ray cameras, built at Leicester University, provide color-coded images based on temperature. XMM has detected supernova remnants in the Large Magellanic Cloud and is uncovering information about black holes in distant galaxies. The telescope will continue its mission for a decade, with plans for a new generation X-ray telescope underway.

What discoveries have been made regarding supernova remnants using the XMM telescope?

What are the future plans for X-ray telescopes following the XMM?