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"Ozone Discovery on Jupiter's Moon"

International team of scientists, including from India, discovered ozone on Jupiter’s moon, Callisto.

"Ozone Discovery on Jupiter's Moon"

GS PAPER 3

(SCIENCE AND TECHNOLOGY)



Discovery of Ozone on Callisto:

  • International team of scientists, including from India, discovered ozone on Jupiter’s moon, Callisto.
  • Published in March 2024 in the journal Icarus.
  • Study focused on chemical evolution of 'SO2 astrochemical ice' under UV irradiation.
  • UV absorption spectra analysis identified distinct ozone signature.

Importance of Ozone:

  • Ozone shields Earth from harmful UV radiation.
  • UV-B and UV-C components damage DNA, increase cancer risk.
  • Ozone layer absorbs UV-B and UV-C radiation.
  • Essential for maintaining habitable conditions on Earth.

Callisto's Unique Environment:

  • Callisto: Jupiter's Second-largest moon.
  • Composition: water ice, rocky materials, sulphur dioxide, organic compounds.
  • Heavily cratered surface, indicating long history of impacts.
  • Stable surface, relatively inactive geologically.
  • Potential for subsurface ocean or habitats beneath icy crust.

Recreating Conditions on Earth:

  • Led by R. Ramachandran, scientists investigated chemical evolution of sulphur dioxide ice under irradiation.
  • Experiments conducted at NSRRC in Taiwan to mimic solar radiation.
  • Used vacuum ultraviolet photons to simulate sunlight.
  • Lithium fluoride substrate used to model Callisto's surface.
  • Controlled temperature conditions during experiments.

Detection of Ozone and Potential Habitability:

  • Ultraviolet absorption spectrum revealed ozone formation after irradiation.
  • Ozone presence suggests oxygen presence, crucial for life's complex molecules.
  • Raises questions about Callisto's habitability and potential for life.
  • Discovery extends to other icy moons in the Solar System.
  • Comparison with Hubble Space Telescope data confirmed ozone presence.

Insights and Future Research:

  • Unidentified band in absorption spectrum hints at common molecular source on icy moons.
  • Provides insights into geological and atmospheric processes.
  • Helps understand formation mechanisms of Jupiter and its moons.
  • Active research area with potential for further discoveries.

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