
NASA/Goddard Area Flight Heart
This week we’re specializing in what’s at the moment a darkish patch within the sky, however gained’t be for for much longer. That’s as a result of a “new” star is predicted to look within the night time sky over the subsequent few months.
After all, the star isn’t truly new – it has been round for billions of years. What’s new is that it is going to be seen to the bare eye, briefly, whereas present process an explosive occasion referred to as a nova.
The article in query, referred to as T Coronae Borealis – or the a lot catchier “blaze star” – is definitely a binary star system made up of…