Black holes are notoriously greedy to devour anything near them. And it’s not going to be a quick and orderly death – because the strength of the force is proportional to the distance, and the part of the celestial body facing the black hole is gravitated much more than the side facing the far away. In this way, the celestial body is elongated like spaghetti – hence the name spaghetti, although it is scientifically known as the tidal disruption event (TDE). < / P > < p > stars are objects that can encounter this fate, and these events are regularly detected as bright flashes, and then disappear in a few months or so. The problem is that it’s often hard for astronomers to figure out what happens in the process – the energy released when matter falls into a black hole can cause dust and debris to fly out, blocking the view. But in this new event, named at2019qiz, astronomers managed to see the process from its early stages. < / P > < p > “because we discovered its early days, we can actually see the curtain of dust and debris being pulled up, because black holes emit a powerful outflow of matter at a speed of 10000 km / s,” said Kate Alexander, author of the study. “This unique” behind the scenes peek “provides us with the first opportunity to accurately determine the source of the obscured matter and track in real time how it engulfs the black hole.” < / P > < p > using the very large telescope (VLT) and new technology telescope (NTT) of the European Southern Observatory (ESO), astronomers observed the star with ultraviolet light, optical light, X-ray and radio waves in six months. For the first time, the observation results show that the flare of light is directly related to the material flowing on the star. It also shows that stars have roughly the same mass as the sun, while black holes have more than a million suns. The release and download schedule of Microsoft Flight Simulation varies from region to region

By ibmwl