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Cat’s Head Nebula (Webb MIRI Image)

Mid-infrared image of the Cat’s Head Nebula by the James Webb Space Telescope. A bluish-gray filament of dust is in the center, stretching from the bottom to almost the very top. It has a narrow, irregular shape that resembles a cat sitting with its back toward the viewer and a tail extending downward. The tail ends at the lower one-third of the image and widens to a triangular peak of dust. The cat’s head is turned toward the right, revealing a white glowing eye. The background is mostly red, with the top left and right corners revealing the black background of space. On the cat’s left is a dome-shaped grouping of faint filaments of dust. Scattered throughout the view are yellow and blue stars, some with Webb’s signature eight-point diffraction spikes.

In NASA’s James Webb Space Telescope’s mid-infrared image, emission from warm dust and carbon-based molecules excited by starlight outlines intricate structures within the nebula. Changes in local conditions and compositions cause variations in color and brightness. Fine strands and globules are especially apparent to the left of the main pillar.

To the right of the pillar, a bright yellow light source is seen against reddish mid-infrared emission, probably an infant star embedded in dust. A narrow filament appears to cross the likely star, although its physical relationship to the star is not established. Several blue stars are scattered throughout, some with Webb’s characteristic diffraction spikes.

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About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    10:45:59.76
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -60:06:23.76
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Carina
  • 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.
    7,500 - 8,500 light-years
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is about 5.3 arcmin across (about 12.3 light-years)

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 with Webb data from proposal: 12591 (M. Garcia Marin).

  • Instrument
    InstrumentThe science instrument used to produce the data.
    MIRI
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    May 27, 2026
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F770W, F1130W, F1500W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    NGC 3372; HH 903; Cat's Head Nebula; Carina Nebula
  • Object Description
    Object DescriptionThe type of astronomical object.
    Star forming region; Emission Nebula; HII region
  • Release Date
    October 29, 2026
  • Science Release
    Ghostly Cat’s Head Nebula Lurks Within Sight of NASA’s Hubble, Webb
  • Credit
    Image: NASA, ESA, CSA, STScI; Image Processing: Joseph DePasquale (STScI)

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Mid-infrared image of the Cat’s Head Nebula by the James Webb Space Telescope. A bluish-gray filament of dust is in the center, stretching from the bottom to almost the very top. It has a narrow, irregular shape that resembles a cat sitting with its back toward the viewer and a tail extending downward. The tail ends at the lower one-third of the image and widens to a triangular peak of dust. The cat’s head is turned toward the right, revealing a white glowing eye. The background is mostly red, with the top left and right corners revealing the black background of space. On the cat’s left is a dome-shaped grouping of faint filaments of dust. Scattered throughout the view are yellow and blue stars, some with Webb’s signature eight-point diffraction spikes.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

These images were acquired by the MIRI instrument on the Webb Space Telescope. Several filters were used to sample varying 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: Blue=F770W, Green=F1130W, Red=F1500W

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Details

Last Updated
Oct 29, 2026
Contact
Media

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