Life Detected on Distant Exoplanet K2-18b

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Life Detected on Distant Exoplanet K2-18b

Scientists detect signature of life on a distant planet, study suggests

Context: A team of astronomers has detected what may be the most promising signs of extraterrestrial life on the exoplanet K2-18b, located 124 light-years away. However, the researchers remain cautious and have not declared a definitive discovery of life beyond Earth. 

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  • The discovery was led by Dr. Nikku Madhusudhan, an Indian-origin astrophysicist and professor at the University of Cambridge.
  • Data was collected using NASA’s James Webb Space Telescope (JWST), revealing potential biosignatures in the planet’s atmosphere.

What is K2-18b?

  • K2-18b is an exoplanet—a planet that orbits a star outside our solar system.
  • It orbits the cool red dwarf star K2-18, situated in the Leo constellation.
  • Lies within the habitable zone of its star, where liquid water could potentially exist.
  • Approximately 2.6 times the size of Earth and 8.6 times its mass.
  • Classified as a sub-Neptune—a type of planet not found in our solar system but believed to have hydrogen-rich atmospheres and possibly liquid water oceans.

Key Findings

  • Using JWST’s Near-Infrared Imager and Slitless Spectrograph (NIRISS) and Near-Infrared Spectrograph (NIRSpec) instruments, the team detected:
    • Methane (CH₄) and Carbon Dioxide (CO₂).
    • Absence of Ammonia (NH₃) — supporting the Hycean planet hypothesis.
  • Most notably, a possible signal of Dimethyl Sulfide (DMS) — a molecule on Earth produced only by living organisms, especially marine phytoplankton. NASA emphasised the DMS detection is not yet confirmed and requires further observation.
  • The presence of these sulfur-based molecules is consistent with predictions for a Hycean world, a new class of planet theorised to have warm oceans under a hydrogen-rich atmosphere.

Challenges in Interpretation

  • Although these molecules have been detected, the possibility remains that they could be produced by non-biological processes. The team is still unsure about the exact source.
  • Nikku Madhusudhan, lead author of the study, emphasised that more data is needed to confirm these findings, and follow-up observations over 16 to 24 hours are expected to provide further clarity.

Further Observations and the Road Ahead

  • While the detection has reached a three-sigma significance (meaning there’s a 0.3% chance the result occurred by chance), astronomers typically require five-sigma significance (a 0.00006% chance of error) to confirm a scientific discovery.
  • The team will conduct follow-up JWST observations within the next 1–2 years to confirm DMS.
  • The European Space Agency’s Ariel mission, launching in 2029, will further investigate exoplanetary atmospheres including K2-18b.

Dr. Nikku Madhusudhan

  • An Indian-British astrophysicist and Professor at the University of Cambridge’s Institute of Astronomy.
  • Academic background:  
    • B.Tech from IIT-BHU
    • MS & PhD in Physics from MIT
  • Formerly affiliated with Yale, Princeton, and MIT.
  • Awards include:
    • 2019 MERAC Prize (European Astronomical Society)
    • 2016 Young Scientist Medal (International Union for Pure and Applied Physics)
  • Pioneered the concept of Hycean worlds in 2021.

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