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Blood Moon

  • 08 Sep 2025
  • 3 min read

Why in News?

On 8th September 2025, skywatchers across Asia, Australia, and parts of Africa witnessed a spectacular Blood Moon—a total lunar eclipse where Earth’s shadow turned the Moon deep red. 

  • It was the year’s second total lunar eclipse after March 2025, lasting over five hours with 82 minutes of totality, and building anticipation for the August 2026 solar eclipse. 
  • Unlike a solar eclipse, lunar eclipses are safe to view with the naked eye.

Lunar Eclipse

Key Points

  • Lunar Eclipse: A lunar eclipse occurs when the Sun, Earth, and Moon align in a straight line, with Earth positioned in the middle. This blocks sunlight from directly reaching the Moon.
    • Total Lunar Eclipse: When the Moon passes through the Earth’s inner, darkest shadow (umbra), it appears deeply shaded or red.
    • Partial Eclipse: When only part of the Moon passes through the umbra.
    • Penumbral Eclipse: When the Moon enters only the outer shadow (penumbra), the dimming is subtle and often hard to notice.

Types of Lunar Eclipse

  • “Blood Moon” Effect: The “Blood Moon” effect happens because Earth’s atmosphere filters sunlight before it reaches the Moon. When light passes through our atmosphere:
    • Blue light scatters easily (this is why our sky looks blue).
    • Red light bends around Earth and reaches the Moon, causing it to glow red or coppery during a total eclipse.
    • A bright red Moon suggests clearer air with fewer pollutants.
      • A deeper red Moon signals more dust, ash, or pollution in the air, reflecting the condition of Earth’s atmosphere.
  • Correlation: The phenomenon behind the Blood Moon is the same process that colours the sky and sunsets: Rayleigh scattering, first explained by physicist John William Strutt, 3rd Baron Rayleigh.
    • Daytime Sky: Short-wavelength blue light scatters in all directions, making the sky appear blue.
    • Sunrise & Sunset: Sunlight passes through thicker layers of atmosphere, scattering away blue light. What remains are long wavelengths — red, orange, and yellow.
      • During a lunar eclipse, the Moon is essentially bathed in all the world’s sunsets at once, projected through Earth’s atmosphere.
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