Three-dimensional prototypes of astronomical objects can be highly complicated. They can vary from black holes, so light doesn’t escape the sheer size of the universe and everything within. However, not every object has attained the attention required to develop a perfect model. Still, we can officially enlist another super complex model to our charts. Astronomers at the University of Arizona have created a model of VY Canis Majoris. It is a red hypergiant that is perhaps the biggest star in the Milky Way. The astronomers will utilize that model to anticipate how it will perish.
How red hypergiants die has been a matter of some debate recently. Data exhibits a substantial lack of supernovae correlated to the numbers that would be required if red hypergiants themselves were to explode in that manner…
Here comes the UA team. They selected VY Canis Majoris as an outstanding stand-in for the category of red hypergiants they were enthusiastic about learning more about. The star itself is enormous, ranging from 10,000 AU to 15,000 AU in size, implying that it would reach 10,000 to 15,000 times farther out than the Earth is presently from the sun. This makes VY Canis Majoris, which inhabits the southern constellation Canis Major, exciting to observers.
The UA researchers utilized time on ALMA to obtain radio signals of the material that is fired into space as part of these explosions.
Processing all that obtained data can be tricky, and they are still working on a few. However, they had enough to demonstrate their findings to the American Astronomical Society in mid-June. After retaining even more data, they’ll be prepared to describe an even nicer model of what one of the biggest stars in the galaxy looks like.
