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Pillars of Creation (NIRCam and MIRI Composite Image)

Layers of semi-opaque brown- and purple-colored gas and dust that starts at the bottom left and goes toward the top right. There are three prominent pillars rising toward the top right. The top pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red areas.

By combining images of the iconic Pillars of Creation from two cameras aboard NASA’s James Webb Space Telescope, the universe has been framed in its infrared glory. Webb’s near-infrared image was fused with its mid-infrared image, setting this star-forming region ablaze with new details.

Myriad stars are spread throughout the scene. The stars primarily show up in near-infrared light, marking a contribution of Webb’s Near-Infrared Camera (NIRCam). Near-infrared light also reveals thousands of newly formed stars – look for bright orange spheres that lie just outside the dusty pillars.

In mid-infrared light, the dust is on full display. The contributions from Webb’s Mid-Infrared Instrument (MIRI) are most apparent in the layers of diffuse, orange dust that drape the top of the image, relaxing into a V. The densest regions of dust are cast in deep indigo hues, obscuring our view of the activities inside the dense pillars.

Dust also makes up the spire-like pillars that extend from the bottom left to the top right. This is one of the reasons why the region is overflowing with stars – dust is a major ingredient of star formation. When knots of gas and dust with sufficient mass form in the pillars, they begin to collapse under their own gravitational attraction, slowly heat up, and eventually form new stars. Newly formed stars are especially apparent at the edges of the top two pillars – they are practically bursting onto the scene.

At the top edge of the second pillar, undulating detail in red hints at even more embedded stars. These are even younger, and are quite active as they form. The lava-like regions capture their periodic ejections. As stars form, they periodically send out supersonic jets that can interact within clouds of material, like these thick pillars of gas and dust. These young stars are estimated to be only a few hundred thousand years old, and will continue to form for millions of years.

Almost everything you see in this scene is local. The distant universe is largely blocked from our view both by the interstellar medium, which is made up of sparse gas and dust located between the stars, and a thick dust lane in our Milky Way galaxy. As a result, the stars take center stage in Webb’s view of the Pillars of Creation.

The Pillars of Creation is a small region within the vast Eagle Nebula, which lies 6,500 light-years away.

Revisit Webb’s near-infrared image and its mid-infrared image. The Pillars of Creation was made famous by the Hubble Space Telescope’s 1995 image.

NIRCam was built by a team at the University of Arizona and Lockheed Martin’s Advanced Technology Center.

MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    18:18:48.17
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -13:48:26.03
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Serpens
  • 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.
    6,500 light-years (2,000 parsecs)
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is approximately 7 light-years across

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.

    This image was created from JWST data from proposal: 2739 (K. Pontoppidan)

  • Instrument
    InstrumentThe science instrument used to produce the data.
    JWST>NIRCam and MIRI
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    14 Aug 2022
  • Filters
    FiltersThe camera filters that were used in the science observations.
    NIRCam: F090W, F187N, F200W, F335M, F444W, F470N; MIRI: F770W, F1130W, F1500W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    M16, Eagle Nebula, NGC 6611
  • Object Description
    Object DescriptionThe type of astronomical object.
    Emission Nebula
  • Release Date
    November 30, 2022
  • Credit
    NASA, ESA, CSA, STScI; Image Processing: Joseph DePasquale (STScI), Alyssa Pagan (STScI), Anton Koekemoer (STScI)

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Layers of semi-opaque brown- and purple-colored gas and dust that starts at the bottom left and goes toward the top right. There are three prominent pillars rising toward the top right. The top pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red areas.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

These images are a composite of separate exposures acquired by the James Webb Space Telescope using the NIRCam and MIRI instruments. Several filters were used to sample different infrared wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are:    Purple: F090W, Blue: F187N and F770W, Cyan: F200W, Green: F1130W; Yellow: F335M, Orange: F444W, Red: F470N and F1500W

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Details

Last Updated
Aug 28, 2025
Contact
Media

Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov

Science Credit

NASA, ESA, CSA, STScI

Image Processing Credit

Joseph DePasquale (STScI), Alyssa Pagan (STScI), Anton Koekemoer (STScI)