Blast in Space: A terrible explosion has been recorded in space. This explosion took place in another galaxy located near our galaxy. The explosion was so strong that the temperature there reached 30 lakh degrees. Scientists studied this blast with the help of telescope.
Our galaxy ‘Milky Way’ has a small galaxy, which is named Large Magalanic Cloud (LMC). This galaxy keeps circling our ‘Milky-Way’ like a satellite. This explosion has been seen in a star of this galaxy. This explosion is considered to be the hottest explosion ever since the study started on space.
The star in which this explosion has been seen, scientists named him LMCN 1968-12A. The explosion has been seen many times before in this star. Actually, LMC is a dwarf galaxy, where there is a shortage of metals. In such a situation, small stars here draw gas from their companions big stars. LMCN 1968-12A also does the same. & Nbsp; This is the reason that it keeps exploding. Last year too, a big explosion was recorded in the same star. Although the explosion of this time is said to be the most fierce.
Explosion due to increased heat and pressure
When such stars gradually keep taking gas from neighboring fellow stars, then a disc starts forming, due to which heat and pressure in the star starts increasing. When this temperature crosses a certain range, hydrogen fusion begins and then a thermonuclear explosion. This explosion can be seen from a few weeks to months. Please tell that even after such explosions, this star is not destroyed.
56 years ago, this star
This star was discovered in the year 1968. This is why it was named LMCN 1968-12A. The explosion has been recorded in this star continuously since 1990. Chile -based Magelan Bade Telescope and Gemini South Telescope have been continuously studying on this star and its galaxy. In the explosion that scientists saw this time, it was found that during the explosion, silicon was present in the star with tremendous intensity. Other metals were missing. That is why this explosion was more severe and warm.
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