What is Hypergiant Star?

Hypergier Stars are the most massive and holy stars. The star hypergient includes about 100-150 solar masses worth the material, approaching Eddington's limit, the theoretical upper threshold of star matter, which the star starts to throw a huge amount of material due to its great radiation. However, there are some hypergiant stars with approximately 100 solar masses, which are expected to have once weighed 200-250 solar masses, which challenges the current theory of stars formation. Hypergiers can be thousands to 40 million times more light than our sun. As silicon connects the core, a process that lasts only a few weeks, the star cannot extract any energy from the nuclear fusion (fusion of iron requiring an even greater temperature) and supernova occurs when the star collapses and Tslepice "reflects" out. Somewhat prosaic: when a hypergiant star goes nova, sometimes called "Hypern".

HypergiantDy have a diameter between about 100 and 2100 times higher than the Sun diameter. You canis Mairis, a red hypergiant star, is the largest known star between 1800 and 2100 solar averages of width. Like the main sequential stars, hypergiers come in all spectral flavors: there are blue hypergiers, red hypergiers and yellow hypergiers. On the other hand, the Milky Way galaxy is the LBV 1806-20, one of the light blue variables, the most largest star, at 2 to 40 million times brighter than the Sun. The absolute size of this star is close to the extent of some smaller galaxies.

Star Hypergiant is short -term, existing only a few million years before they get to Nova. As a result, relatively rare and theory of hypergiers are limited by rare data. Hypergiers are one of the most precious classes of well -known stars, yellow hypergiers, of which there are only about seven in our galaxy.