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Great Orion Nebula

  • 17 sessions
  • 1,901 images
  • 26.26 hours

Details

The Great Orion Nebula (Messier 42, M42) is one of the brightest and most famous nebulae in the night sky, visible even to the naked eye as a fuzzy patch in Orion’s Sword below the constellation’s three Belt stars. It lies about 1,344–1,500 light-years from Earth, is roughly 24–25 light-years across, and has an apparent magnitude of +4.0, making it a stellar nursery packed with young stars, protoplanetary disks, clouds of gas and dust, and intense star formation activity.

Physical Features
  • • The nebula radiates in striking hues due to ionized hydrogen (red), oxygen (green), and sulfur (orange)—these emissions result from the energetic activity of newly formed stars.
  • • The heart of the Orion Nebula glows with the Trapezium Cluster, a group of four (actually six+) young, massive, hot stars arranged in a trapezoidal pattern and responsible for carving out a cavity in the nebula with powerful ultraviolet radiation.
  • • Surrounded by clouds and filaments, the nebula hosts about 2,000–3,000 solar masses of material, supporting ongoing stellar birth and evolution.

Observational Highlights
  • • Located in Orion’s Sword (below Orion’s Belt), the nebula spans approximately 1 degree of sky—around two full moons.
  • • Through binoculars or small telescopes, the Orion Nebula displays complex structure: bright knots, dark lanes (such as the “Fish’s Mouth” feature), the intensely bright Trapezium Cluster, and intricate patterns of glowing gas.
  • • Astrophotography captures its vivid colors and fine details—one of the best targets for both beginners and experienced imagers under dark skies.

Astronomical Significance
  • • The Orion Nebula is part of the greater Orion Molecular Cloud Complex, a star-forming region that includes the Horsehead Nebula, Barnard’s Loop, M43, and M78.
  • • Astronomers have observed protoplanetary disks, brown dwarfs, and turbulent motions within the nebula, making it a central object for understanding how stars and planetary systems form from collapsing clouds of interstellar material.
  • • The nebula’s ionized gas has temperatures reaching 10,000 K at its core, and the active ultraviolet radiation from the Trapezium cluster continuously shapes and disperses surrounding material.

Cultural and Historic Impact
  • • Ancient cultures, notably the Maya, likened the Orion Nebula to a cosmic fire of creation—a testament to its prominence and mystery in the sky.
  • • The nebula has drawn the attention of scientists since the 19th century, and Hubble Space Telescope observations have mapped thousands of stars and revealed new wonders within its intricate clouds.

In summary, the Great Orion Nebula is a prototypical stellar nursery, offering a stunning view of star formation and dynamic interstellar processes, and remains one of the most beloved astronomical subjects for both visual observers and astrophotographers.

Sessions

Date L R G B Ha Oiii Sii Ha-oiii Sii-oiii Uvir
2025-10-04 0.28 0.1 0.1 0.09 0.37 0.4 0.4
2025-10-05 1.03 1.08
2025-10-06 0.6 1.57
2025-10-07 0.28
2025-10-14 0.48 0.15 0.13 0.13 1.0
2025-10-20 0.08 0.09 0.11 0.11 0.67
2025-10-21 1.37
2025-10-22 1.45
2025-10-29 0.58 0.6 0.6 0.43 0.4 0.33
2025-10-30 0.3 0.23 0.33 0.38 1.33 1.2 1.0
2025-10-31 0.4 0.12 0.73 1.53 1.6 0.48
2025-11-03 0.33 0.4 0.03
2025-11-11 0.37 0.43
2025-11-13 0.03
Total 1.14 0.34 0.34 0.33 3.21 5.94 5.04 3.99 4.03 1.87

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