White Dwarf "Close" to Exploding as Supernova

Illustration of the white dwarf and its companion HD49798. If it was possible to look at the system up-close, it would look something like this.   Credits: Francesco Mereghetti, background image: NASA, ESA and T.M. Brown (STScI)

ESA’s XMM-Newton orbiting X-ray telescope has uncovered the first close-up of a white dwarf star that could explode into a type Ia supernova within a few million years. That's relatively soon in cosmic time frames, and although this white dwarf that is orbiting its companion star HD 49798, is far enough away to pose no danger to Earth, it is close enough to become an extraordinarily spectacular celestial sight. Calculations suggest that it will blaze initially with the intensity of the full Moon and be so bright that it will be seen in the daytime sky with the naked eye. But don't worry, it will be awhile!
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