
NASA/Goddard Area Flight Heart
This week we’re specializing in what’s presently a darkish patch within the sky, however received’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 following few months.
In fact, the star isn’t truly new – it has been round for billions of years. What’s new is that it will likely be seen to the bare eye, briefly, whereas present process an explosive occasion referred to as a nova.
The item in query, referred to as T Coronae Borealis – or the a lot catchier “blaze star” – is definitely a binary star system made up of…