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Evolution of the Orion Nebula (M42)

Evolution of the Orion Nebula (M42)
Radiation and wind from a nebula's stars push surrounding gas away, creating cavities within the nebula's cloud. In the Orion Nebula, several hot, young central stars, called the Trapezium, have carved out the core of the nebula. This cavernous core has broken through the part of the cloud that faces Earth, enabling Hubble and other telescopes to observe within.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    05h 35m 17.0s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -5° 23' 27.99"
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Orion Nebula, M42, NGC 1976
  • Release Date
    January 11, 2006
  • Science Release
    Hubble Panoramic View of Orion Nebula Reveals Thousands of Stars
  • Credits
    NASA, ESA, and A. Feild (STScI)

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Details

Last Updated
Mar 14, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov