Particle.news

Download on the App Store

Cambridge Scientists Report Potential Biosignatures on Exoplanet K2-18 b

Detection of dimethyl sulfide and dimethyl disulfide in the atmosphere of the distant 'Hycean' world sparks debate over methodology and implications for extraterrestrial life.

An artist's concept shows what exoplanet K2-18 b could look like based on science data.
An artist's concept shows what exoplanet K2-18 b could look like based on science data.
Image
Image

Overview

  • Cambridge researchers claim a 99.7% confidence level in detecting dimethyl sulfide (DMS) and dimethyl disulfide (DMDS) on K2-18 b, molecules considered potential biosignatures on Earth.
  • K2-18 b, classified as a 'Hycean' world, is located in its star's habitable zone and may host liquid oceans beneath a hydrogen-rich atmosphere.
  • Critics argue that the findings rely on data-processing methods that are sensitive to small adjustments, potentially explaining the signals without requiring DMS or DMDS.
  • While DMS is often associated with biological processes, it can also be produced through non-biological means, such as in comets or under specific chemical conditions.
  • The announcement draws comparisons to the controversial phosphine detection on Venus, emphasizing the need for higher statistical thresholds and rigorous validation in biosignature research.