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Orion Nebula

Orion Nebula

NASA's Hubble Space Telescope captured an unprecedented look at the Orion Nebula, a turbulent stellar nursery that is one of astronomy's most photogenic celestial regions. Newborn stars reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that are reminiscent of the Grand Canyon. The crisp image reveals a tapestry of star formation, from the dense pillars of gas and dust that may be the homes of fledgling stars to the hot, young, massive stars that have emerged from their gas-and-dust cocoons and are shaping the nebula with their powerful ultraviolet light.

The Orion Nebula is a perfect laboratory to study how stars are born because it is 1,500 light-years away, a relatively short distance within our 100,000 light-year wide galaxy. Astronomers have a clear view into this crowded stellar maternity ward because massive stars in the center of the nebula have blown out most of the dust and gas in which they formed, carving a cavity in the dark cloud. In this bowl of stars, we see the entire star formation history of Orion printed into the features of the nebula: arcs, blobs, pillars, and rings of dust that resemble cigar smoke. Each feature tells a story of stellar winds from young stars that impact the stellar environment and the material ejected from other stars. Our Sun was probably born 4.5 billion years ago in such a cloud.

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"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Orion
  • Distance
    DistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
    The distance to the Orion Nebula is 1,500 light-years (460 parsecs).
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    The image is 7.9 arcminutes (3.4 light-years or 1.1 parsecs) wide.

About the Data

  • Data Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
    The Hubble image was created from HST data from proposal 10246: M. Robberto (STScI/ESA), and 13826, M. Robberto (STScI/ESA)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>ACS/WFC, HST>WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    Oct. 2004 – Apr. 2005 (ACS), and Feb. 2015 – Oct. 2015 (WFC3/IR)
  • Filters
    FiltersThe camera filters that were used in the science observations.
    ACS/WFC: F435W (B), F555W (V), and F775W (i) WFC3/IR: F139M
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Orion Nebula, M42, NGC 1976
  • Object Description
    Object DescriptionThe type of astronomical object.
    Emission Nebula
  • Release Date
    March 17, 2017
  • Science Release
    Hubble Discovery of Runaway Star Yields Clues to Breakup of Multiple-Star System
  • Credit
    NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team

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Orion Nebula
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

This image is a composite mosaic of many separate exposures made by the ACS and WFC3 instruments on the Hubble Space Telescope using several different filters isolating the light of specific elements or of specific broad wavelength ranges. The color arises by assigning different hues (colors), to each monochromatic image. In this case, the colors are: Blue: F435W (B) Cyan: F555W (V) Yellow: F775W (i) Red: F139M

Compass and Scale
Compass and ScaleAn astronomical image with a scale that shows how large an object is on the sky, a compass that shows how the object is oriented on the sky, and the filters with which the image was made.

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Details

Last Updated
Mar 28, 2025
Contact
Media

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