Context:
Astronomers have discovered a rare class of stars, called helium-covered hot stars.
Astronomers Discover a Hot Helium Star
- After the research, scientists finally discovered a missing population of stars that confirms a key prediction of how Binary Star evolved.
Binary Star
- A system of two stars in which one star revolves around the other or both revolve around a common centre.
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Also Read: Formation Of Stars
What Is a Helium Star?
- It is a class O or B star (blue), which has extraordinarily strong helium lines, and weaker than normal Hydrogen lines, indicating strong stellar winds.
Class O or B Star
- Class O: It includes bluish-white stars with surface temperatures typically 25,000–50,000 K.
- Lines of ionized helium appear in the spectra.
- Class B: These stars typically range from 10,000 K to 25,000 K and are also bluish-white but show neutral helium lines
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- Extreme Helium Stars are scarce stars that are almost completely devoid of hydrogen.
- Temperature: Helium-rich stars are the hottest star category, almost 10 times as hot as the Sun.
- Their immense heat means that despite being exceptionally rare, they make an outsize contribution to the universe’s stock of heavier elements.
- Hypothetical Star: A Helium star is also a term for a hypothetical star that could occur if two helium white dwarfs subsequently start nuclear fusion of helium, with a lifetime of a few hundred million years.
- This may only happen if these two binary masses share the same type of envelope phase. It is believed this is the origin of the extreme helium stars.
Also Read: Black Hole Mass Gap
News Source: ILF Science and The Hindu
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