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NGC 6072 (MIRI Image)

Colorful, mostly blue image of mid-infrared light from a glowing cloud with a distorted, asymmetrical shape. A star at the center of the image is a small point of pinkish-white light. The asymmetrical shape of the expanding cloud of gas and dust resembles paint splattered on the ground. The filaments of the expanding shells are wispy, and mostly white and blue. The shells appear as lobes stretching from roughly 11 to 5 o’clock, another from 1 to 7 o’clock, and possibly a third from 12 to 6 o’clock. These outflows push gas toward the equatorial plane, forming a disk that appears to span from 9 to 3 o’clock. A perfect circle of whitish blue dust traces the outer edges of the shells. The background of the image is black and speckled with tiny bright stars and distant galaxies.

The mid-infrared view of planetary nebula NGC 6072 from NASA’s James Webb Space Telescope shows expanding circular shells around the outflows from the dying central star, which astronomers suspect is the pinkish white dot at the center of the image. The longer wavelengths captured by Webb’s MIRI (Mid-Infrared Instrument) highlight the dust being cast off by the central dying star.

In this image, the blue represents cool molecular gas that is seen in red in the near-infrared image from Webb’s NIRCam (Near-Infrared Camera) due to color mapping.

Read the full image description.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    16:12:58.4
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    36:13:49.3
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Scorpius
  • 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.
    About 3,300 light-years
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is 2.4 arcminutes across (about 2.3 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: 6554 (M. Garcia Marin). Image processing: Alyssa Pagan (STScI).

  • 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.
    29 July 2024
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F770W, F1130W, F1280W, F1800W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    NGC 6072; IRAS F16097-3606
  • Object Description
    Object DescriptionThe type of astronomical object.
    Planetary nebula
  • Release Date
    July 30, 2025
  • Science Release
    NASA’s Webb Traces Details of Complex Planetary Nebula
  • Credit
    Image: NASA, ESA, CSA, STScI

Downloads

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    jpg (990.72 KB)
Colorful, mostly blue image of mid-infrared light from a glowing cloud with a distorted, asymmetrical shape. A star at the center of the image is a small point of pinkish-white light. The asymmetrical shape of the expanding cloud of gas and dust resembles paint splattered on the ground. The filaments of the expanding shells are wispy, and mostly white and blue. The shells appear as lobes stretching from roughly 11 to 5 o’clock, another from 1 to 7 o’clock, and possibly a third from 12 to 6 o’clock. These outflows push gas toward the equatorial plane, forming a disk that appears to span from 9 to 3 o’clock. A perfect circle of whitish blue dust traces the outer edges of the shells. The background of the image is black and speckled with tiny bright stars and distant galaxies.
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 of separate exposures acquired by the James Webb Space Telescope using the MIRI instrument. Several filters were used to sample wide 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, Cyan: F1130W, Green: F1280W, Red: F1800W

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Details

Last Updated
Sep 04, 2025
Contact
Media

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

Image Credit

NASA, ESA, CSA, STScI