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The Star that shouldn't exist and the Vanishing at TYC 8241 2652

February 21, 2017
by
John Michael Godier
YouTube video player
The Star that shouldn't exist and the Vanishing at TYC 8241 2652

TL;DR

Two stars defy explanation - one is composed almost entirely of hydrogen and helium, defying the standard model of star formation, while the other star's surrounding gas and dust disappeared in a short period of time, contrary to typical astronomical processes.

Transcript

As of right now Tabby's star rightfully holds the title of the galaxy's strangest star, but there are two others that defy explanation and even years after their discovery they remain mysteries. One of them should not exist at all. And the other is missing something really important. Located in the constellation Leo, there exists a star known as SD... Read More

Key Insights

  • 🌟 SDSS J102915 + 172927 challenges the standard model of star formation due to its lack of heavier elements and low levels of lithium.
  • 😚 TYC 8241 2652 defies typical timescales for planetary disc condensation by losing its gas and dust in just a few years.
  • 🤩 These mysterious stars highlight gaps in our understanding of astrophysics and emphasize the need for further exploration and study.
  • 🤩 Discoveries like these suggest that our current theories on star formation and astronomical phenomena may require revisions.
  • 🤩 These enigmatic stars showcase the complexity and unpredictability of the universe, leaving scientists with more questions than answers.
  • 🤩 The mysteries surrounding these stars provide opportunities for future research and the potential for groundbreaking discoveries.
  • 🤩 Further investigation and the discovery of more stars with similar characteristics may help unravel the secrets behind these peculiar phenomena.

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Questions & Answers

Q: Why does SDSS J102915 + 172927 defy the standard model of star formation?

This star, composed almost entirely of hydrogen and helium, lacks the heavier elements needed for core formation, contradicting our understanding of how stars condense.

Q: Why does SDSS J102915 + 172927 have significantly less lithium than expected?

Given its age, this star should have similar composition to the early universe, but it possesses 50 times less lithium, suggesting our theories on lithium production may be flawed.

Q: How did the gas and dust surrounding TYC 8241 2652 disappear so quickly?

Astronomers have no satisfying theory to explain this phenomenon, as natural processes typically occur over millions of years, not a few years as observed in this case.

Q: Is it possible that someone or something harvested the material around TYC 8241 2652?

Although unlikely, the sudden disappearance of the material leaves the question open, even though we may never have a definitive answer.

Summary & Key Takeaways

  • SDSS J102915 + 172927, an extremely old star with the lowest observed amount of heavier elements, challenges the standard model of star formation.

  • This star also has significantly less lithium than expected, raising questions about our understanding of the early universe.

  • TYC 8241 2652, a young star, had its surrounding gas and dust vanish within a few years, defying conventional timescales for planetary disc condensation.


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