XMM-Newton Latest News


For older news stories regarding XMM-Newton please visit the News Archive

Quasar 18-Mar-2019:
'Teacup' Quasar Causes Galactic Storms
SDSS J143029.88+133912.0, nicknamed the 'Teacup' because of its shape, is a quasar powered by a supermassive black hole. New data from NASA's Chandra X-ray Observatory and ESA's XMM-Newton mission provide detailed information about the history of the eruptions of energy and particles produced by the black hole.
Further details on Sci-News pages.

NGC 300 25-Feb-2019:
Past and future generations of stars in NGC 300
This swirling palette of colours portrays the life cycle of stars in a spiral galaxy known as NGC 300. The different colours are derived from optical observations performed by MPG/ESO's Wide Field Imager (WFI) telescope at La Silla, Chile; infrared observations made with NASA's Spitzer space telescope; and data collected in X-rays by ESA's XMM-Newton space observatory.
Further details on ESA's Space in Images portal.

Measuring the Expansion of the Universe 28-Jan-2019:
Active galaxies point to new physics of cosmic expansion
Investigating the history of our cosmos with a large sample of distant ‘active’ galaxies observed by ESA’s XMM-Newton, a team of astronomers found there might be more to the early expansion of the Universe than predicted by the standard model of cosmology.
Further details on ESA's Space Science portal.

Supernova 10-Jan-2019:
Team of telescopes finds X-ray engine inside mysterious supernova
ESA’s high-energy space telescopes Integral and XMM-Newton have helped to find a source of powerful X-rays at the centre of an unprecedentedly bright and rapidly evolving stellar explosion that suddenly appeared in the sky earlier this year.
Further details on ESA's Space Science portal.

Black hole devours a star 09-Jan-2019:
XMM-Newton captures final cries of star shredded by black hole
Astronomers using ESA's XMM-Newton space observatory have studied a black hole devouring a star and discovered an exceptionally bright and stable signal that allowed them to determine the black hole's spin rate.
Further details on ESA's Space Science portal.