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Cassiopeia A (MIRI Compass Image)

An image labeled “James Webb Space Telescope, Cassiopeia A, SNR G111.7-02.1).” A roughly square image is rotated clockwise about 45 degrees, with solid black in the corners. Within the image is a roughly circular nebula with complex structure. On the circle’s exterior, particularly at the top and left, lie curtains of material glowing orange. Interior to this outer shell lies a ring of mottled filaments of bright pink studded with clumps and knots. At center right, a greenish loop extends from the right side of the ring into the central cavity. Translucent wisps of blue, green and red are throughout the image. At lower left, a scale bar is labeled 3 light-years and 1 arcminute. At lower right, a white arrow pointing up is labeled N for north, while an arrow pointing left is labeled E for east. At the bottom is a list of MIRI filters in different colors, from left to right: F560W, F770W, F1000W, F1130W, F1280W, F1800W, F2100W, and F2550W.

This image of the Cassiopeia A supernova remnant, captured by Webb’s Mid-Infrared Instrument (MIRI), shows compass arrows, scale bar, and color key for reference.

The north and east compass arrows show the orientation of the image on the sky. Note that the relationship between north and east on the sky (as seen from below) is flipped relative to direction arrows on a map of the ground (as seen from above).

The scale bar is labeled in light-years, which is the distance that light travels in one Earth-year. (It takes 0.25 years for light to travel a distance equal to the length of the scale bar.) One light-year is equal to about 5.88 trillion miles or 9.46 trillion kilometers. The field of view shown in this image is approximately 10 light-years across.

This image shows invisible mid-infrared wavelengths of light that have been translated into visible-light colors. The color key shows which MIRI filters were used when collecting the light. The color of each filter name is the visible light color used to represent the infrared light that passes through that filter.

Read the full image caption.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    23:23:24.00
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    +58:48:54.00
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Cassiopeia
  • 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.
    11,090 light-years
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is about 24 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 with Webb data from proposal: 1947 (D. Milisavljevic).

  • 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.
    August 4, 2022
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F560W, F770W, F1000W, F1130W, F1280W, F1800W, F2100W, F2550W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Cassiopeia A; SNR G111.7-02.1
  • Object Description
    Object DescriptionThe type of astronomical object.
    Supernova remnant
  • Release Date
    April 7, 2023
  • Science Release
    Webb Reveals Never-Before-Seen Details in Cassiopeia A
  • Credit
    Image: NASA, ESA, CSA, Danny Milisavljevic (Purdue University), Tea Temim (Princeton University), Ilse De Looze (UGhent); Image Processing: Joseph DePasquale (STScI)

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An image labeled “James Webb Space Telescope, Cassiopeia A, SNR G111.7-02.1).” A roughly square image is rotated clockwise about 45 degrees, with solid black in the corners. Within the image is a roughly circular nebula with complex structure. On the circle’s exterior, particularly at the top and left, lie curtains of material glowing orange. Interior to this outer shell lies a ring of mottled filaments of bright pink studded with clumps and knots. At center right, a greenish loop extends from the right side of the ring into the central cavity. Translucent wisps of blue, green and red are throughout the image. At lower left, a scale bar is labeled 3 light-years and 1 arcminute. At lower right, a white arrow pointing up is labeled N for north, while an arrow pointing left is labeled E for east. At the bottom is a list of MIRI filters in different colors, from left to right: F560W, F770W, F1000W, F1130W, F1280W, F1800W, F2100W, and F2550W.
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 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: F560W, Light Blue: F770W, Cyan: F1000W, Green: F1130W, Yellow: F1280W, Orange: F1800W, Red: F2100W+F2550W

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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

Image Credit

NASA, ESA, CSA, Danny Milisavljevic (Purdue University), Tea Temim (Princeton University), Ilse De Looze (UGhent)

Image Processing Credit

Joseph DePasquale (STScI)