International Space Agencies – Missions and Discoveries

Betelgeuse: The Red Giant Star on the Brink of Supernova

Note4Students

From UPSC perspective, the following things are important :

Prelims level: Betelgeuse

Mains level: NA

Betelgeuse

Central Idea: Recent research has shed light on the Betelgeuse’s current stage and its potential fate as it approaches the end of its lifecycle.

Betelgeuse: The Bright Red Star in Orion

  • Easily visible in the constellation Orion, Betelgeuse is a bright red star known as “Thiruvathirai” or “Ardra” in Indian astronomy.
  • It is a massive star that undergoes the carbon-burning stage, leading to its eventual collapse into a supernova.

How is it dying?

  • Massive stars like Betelgeuse exhaust their hydrogen fuel and transition to using helium to create carbon.
  • The energy released during helium fusion is lower than that of hydrogen, requiring the star to burn more helium to maintain stability.
  • Eventually, the helium is depleted, leading to the star’s progression through various burning stages, including carbon and silicon burning.

Pulsation and Betelgeuse’s Death Throes

  • Researchers studying Betelgeuse have observed its pulsation, indicating its stage of evolution.
  • The observed pulsation aligns with theoretical estimates of the late carbon-burning stage, suggesting that Betelgeuse is in its death throes.
  • Astronomers detect the expansion and contraction of Betelgeuse by analyzing its pulsation and corresponding brightness variations.
  • Previous studies disagreed on which pulsation period is fundamental, with one team considering 417 days and another team proposing 2,190 days.
  • Researchers conclude that it is in the final stage of burning carbon, considering the 2,190-day pulse as fundamental.

 

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