Extreme Helium Star is a rare type of low-mass supergiant star that is mostly made up of helium and heavier elements and has almost no hydrogen.
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Source: Youtube
Scientists have found an interesting twist in the universe in the star A980, which is in a small group of stars called Extreme Helium (EHe) stars. This star has a lot of germanium, a metal that has never been seen in this type of star before.
Element Name |
Germanium |
Symbol |
Ge |
Atomic Number |
32 |
Group in Periodic Table |
Group 14 (IVa), between silicon and tin |
Appearance |
Silvery-gray metalloid |
Type |
Metalloid (intermediate between metals and nonmetals) |
Crystal Structure |
Diamondlike crystalline structure |
Similar To |
Chemically and physically similar to silicon |
Stability |
Stable in air and water |
Reactivity |
Unaffected by alkalis and most acids, except nitric acid |
Source: PIB
Practice Question: Q. With reference to Extreme Helium Stars (EHe stars), consider the following statements: They are extremely rare stars with very low hydrogen content. They are believed to be formed by the merger of two white dwarfs. These stars are rich in helium and carbon. Which of the statements given above is/are correct? A) 1 and 2 only B) 2 and 3 only C) 1 and 3 only D) 1, 2 and 3 Answer: D) 1, 2 and 3 Explanation: Statement 1: Correct. EHe stars are very rare and almost devoid of hydrogen, which is unusual since hydrogen is the most abundant element in most stars. Statement 2: Correct. The most accepted theory is that they form through the merger of a helium white dwarf with a carbon-oxygen white dwarf. Statement 3: Correct. These stars are composed mainly of helium and show a significant amount of carbon in their atmospheres. |
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