Elias 2-24 b: Discovery of the Youngest Known Exoplanet

Elias 2-24 b: Discovery of the Youngest Known Exoplanet

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Key takeaways

  • Astronomers have confirmed Elias 2-24 b as the youngest known exoplanet, with an age estimated at less than 1 million years old.
  • Located 450 light-years from Earth in the Ophiuchus region, it orbits its host star at an extreme distance of 55 Astronomical Units (AU).
  • The planet has a mass similar to Jupiter and is actively gathering gas and dust within a dark gap in its circumstellar disk.
  • This discovery breaks the age record set by planets near PDS 70 and WISPIT 2, which are over 5 million years old.

Why in News

  • Astronomers used archival data from the W. M. Keck Observatory funded by NASA to confirm Elias 2-24 b as the youngest known planet ever detected, aged less than 1 million years old.

What is Elias 2-24 b

  • It is a newly forming gas-giant exoplanet with a mass close to Jupiter, caught in the earliest stages of planetary birth while still embedded inside a disk of gas, dust, and rock.

Origin of Elias 2-24 b

  • This exoplanet formed around the young star Elias 2-24, located approximately 450 light-years from Earth within the Ophiuchus star-forming region.

Key Features

  • The planet has an estimated age of less than 1 million years old, easily breaking the previous age record held by planets around PDS 70 and WISPIT 2, which are over 5 million years old.
  • It orbits its parent star at an extreme distance of 55 Astronomical Units (AU), which equals roughly 55 times the distance between Earth and the Sun.
  • The planet sits directly inside a dark ringed gap in its surrounding disk, actively accumulating gas and dust to build its outer atmosphere.
  • Researchers identified the planet using high-contrast coronagraphy to block starlight, revealing infrared signatures in archival images taken between 2018 and 2020.

Significance of the Discovery

  • The rapid formation of a planet at 55 AU in under 1 million years challenges current planet formation models, suggesting faster mechanisms like gravitational instability or pebble drift.
  • This discovery offers scientists a direct window into how gas giants grow, migrate, and clear out space during the early evolution of solar systems.