Loren Booda
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Are there stars primarily composed of helium?
Stars primarily composed of helium do exist, particularly within the class known as "Extreme Helium Stars," which exhibit low or absent hydrogen in their surface spectra. These stars are typically remnants of evolved stars, such as white dwarfs, which leave behind a helium-burning shell. Additionally, models suggest that colliding white dwarfs could lead to a scenario where the total helium content surpasses that of other elements. However, such occurrences are rare and would involve stars significantly smaller than solar mass, taking an extensive period to evolve past the hydrogen stage.
PREREQUISITESAstronomers, astrophysicists, and students of stellar evolution who are interested in the composition and lifecycle of stars, particularly those focusing on helium-rich stellar phenomena.
There is a class designated "Extreme Helium Stars", but this comes from the spectra of the surface only where Hydrogen is low or lacking. Most would be the "remnant" (white dwarf) of an evolved star, leaving behind the outer helium burning shell as a "surface", even though the interior would still be composed mostly of carbon and oxygen.Originally posted by Loren Booda
Are there stars primarily composed of helium?