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A View of the Pillars of Creation in Visible and in Near-Infrared Light

Framed side-by-side comparison of the Pillars of Creation. Title text toward the bottom reads “M16, Eagle Nebula, Hubble Space Telescope, WFC3/UVIS/IR.” At left is the visible-light view, and at right is the near-infrared-light view.

These images by NASA's Hubble Space Telescope reveal how different the iconic Pillars of Creation appear in visible and in near-infrared light.

In the visible-light image at left, astronomers combined several exposures to show a wider view of the pillars and the surrounding region. The towering pillars are about 5 light-years tall. The tenuous-looking base of the columns is shown.

The near-infrared image at right transforms the pillars into eerie, wispy silhouettes, which are seen against a background of myriad stars. The near-infrared light can penetrate much of the gas and dust, revealing stars behind the nebula as well as hidden away inside the pillars. Some of the gas and dust clouds are so dense that even the near-infrared light cannot penetrate them. New stars embedded in the tops of the pillars, however, are apparent as bright sources that are unseen in the visible image.

The ghostly bluish haze around the dense edges of the pillars is material getting heated up by the intense ultraviolet radiation from a cluster of young, massive stars and evaporating away into space. The stellar grouping is above the pillars and cannot be seen in the image. At the top edge of the left-hand pillar, a gaseous fragment has been heated up and is flying away from the structure, underscoring the violent nature of star-forming regions.

Both images were taken with Hubble's versatile Wide Field Camera 3. For the near-infrared image, astronomers used filters that isolate the light from newly formed stars, which are invisible in the visible-light image. At these wavelengths, astronomers are seeing through the pillars and even through the back wall of the nebula cavity and can see the next generations of stars just as they're starting to emerge from their formative nursery. In the visible-light image, oxygen is represented in blue, sulfur in orange, and hydrogen and nitrogen in green.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    18h 18m 48.17s
  • 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)

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.
    Data of M16 were obtained from the HST proposal 13926, P.I. Z. Levay, J. Mack, C. Christian, L. Frattare, M. Livio, S. Meyett, M. Mutchler, and J. Sokol (STScI/AURA), and K. Noll (NASA/GSFC).
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>WFC3/UVIS (left) and HST>WFC3/IR (right)
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    September 2014
  • Filters
    FiltersThe camera filters that were used in the science observations.
    WFC3/UVIS: F502N ([O III]), F657N (H-alpha + [N II]), and F673N ([S II])WFC3/IR: F110W (YJ) and F160W (H)
  • 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
    January 5, 2015
  • Science Release
    Hubble Goes High Def to Revisit the Iconic ‘Pillars of Creation’
  • Credit
    NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

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Framed side-by-side comparison of the Pillars of Creation. Title text toward the bottom reads “M16, Eagle Nebula, Hubble Space Telescope, WFC3/UVIS/IR.” At left is the visible-light view, and at right is the near-infrared-light view.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

These images are composites of separate exposures acquired by the WFC3 instrument on the Hubble Space Telescope. Several filters were used to sample broad and narrow 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: WFC3/UVIS Image of M16: Blue: F502N ([O III]) Green: F657N (Hα + [N II]) Red: F673N ([S II]) WFC3/IR Image of M16: Blue: F110W (YJ) Yellow: F160W (H)

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