Coronal Mass Ejection

17 Nov 2025

Coronal Mass Ejection

Astronomers have detected the first-ever CME from another star (red dwarf named StKM 1-1262, located 133 light years away) , proving such events are not unique to our Sun.

About the Breakthrough Observation

  • Intensity: The eruption was 10,00 times more energetic than any solar CME recorded on the Sun.
  • Duration: The entire explosion lasted just one minute, indicating extremely violent magnetic reconnection.
  • Planetary Risk: Such intense CMEs could strip atmospheres from nearby exoplanets, eliminating chances of life.

How the Discovery Was Made

  • Detection Method: The event was identified using data from LOFAR (Low Frequency Array), a European network of low-frequency radio telescopes.
    • LOFAR is typically used to study extreme cosmic events such as black holes, which emit stable radio signals.

Aditya-L1 Mission

  • India’s first dedicated solar observatory, stationed at Lagrange Point L1, studies the Sun’s corona, flares, and CMEs to improve early warnings of geomagnetic storms.

  • Hidden Signals: Researchers developed a secondary data system to store weaker background signals from stars.
  • Breakthrough Analysis: In 2022, scientists reviewing this stored data discovered the massive CME event on StKM 1-1262.

Significance for Astronomy and Space Weather

  • New Era in Stellar Space Weather: 
    • The detection inaugurates a new phase of studying space weather in star systems beyond our own.
    • This provides first direct evidence of how violent stellar activity can be outside the solar system.
  • Stellar Magnetic Activity: CMEs give insight into star magnetic fields, flares, and extreme energetic processes in the universe.
  • Exoplanet Habitability: Extremely violent CMEs can strip atmospheres off Earth-like planets, increase radiation levels and destabilise climates
    • Important for evaluating life-supporting conditions around red dwarfs, which make up 75% of stars in the universe.
  • Better Solar Weather Modelling: Studying extreme stellar CMEs helps refine models of solar storms affecting Earth.

What are Coronal Mass Ejections (CMEs)?

  • Definition: CMEs are large expulsions of plasma and magnetic fields from the Sun’s corona into space.
  • Composition: They contain billions of tons of charged particles (electrons, protons, ions) carried by strong magnetic fields.
  • Cause: Triggered by magnetic energy buildup and sudden release in the Sun’s corona.
  • Relation with Solar Flares: Solar flares and CMEs often occur together, but CMEs are much larger and slower, with long-lasting geomagnetic effects.

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CMEs vs Solar Flares

Feature Solar Flare CME
Nature Burst of electromagnetic energy Ejection of plasma + magnetic fields
Speed Immediate impact (light-speed propagation) Slower Impact; takes 1–3 days to reach Earth
Duration Minutes to hours Hours to days
Impact Radio blackouts, signal disruptions Major geomagnetic storms, power outages
Occurrence Often precede CMEs Not all flares cause CMEs

Impact on Earth & Technology

  • Satellites & GPS: CMEs can damage satellite electronics, cause GPS inaccuracy, and disrupt communications.
  • Power Grids: Strong geomagnetic storms can induce currents that overload transformers, as in the 1989 Quebec blackout.
  • Aviation: Aircraft flying polar routes may face blackouts in HF communication, forcing flight diversions.
  • Space Missions: Astronauts on the ISS face increased radiation exposure, requiring protection protocols.
  • Auroras: CMEs create spectacular auroras, seen unusually far south (e.g., Tennessee, USA) during the Nov 12, 2024 storm.

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UDAAN PRELIMS WALLAH
Comprehensive coverage with a concise format
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Designed as per recent trends of Prelims questions
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