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Lion Nebula (MIRI Image)

Planetary nebula NGC 2392, also called the Lion Nebula, against the black background of space. The nebula is in the center, circular in shape, and looks like a male lion’s head. In the very center is a small, bluish-white circle with eight-point diffraction spikes, a white dwarf star. Surrounding the star are light purple-red cavernous bubbles and shell-like rings. The bubbles and shells collectively form an oval with two small, wide arcs near the top, reminiscent of a lion’s face and its ears. What appears to be extended outward from the lion’s face is a thick ring of cyan material. The width of the ring is consistent throughout and resembles a mane. The area closest to the lion’s face looks cloudy, while the edges of the mane look like there are purple clumps of dust with comet-like tails and strands. In the background are distant galaxies and stars. Some galaxies appear as small purple points of light and others with visible blue spiral structures. A couple of the stars have diffraction spikes.

NASA’s James Webb Space Telescope observed planetary nebula NGC 2392 with its MIRI (Mid Infrared Instrument) instrument, revealing the presence of dust and its varying structures within this tumultuous environment. Nicknamed the Lion Nebula due to its appearance, this collection of gas and dust is created and sculpted by the remains of a dying star, which is in the center and resembles the button nose of the lion.

While some dust is being destroyed by the bubble of ionized gas that forms the lion’s face, most of the gas is being ejected and migrating away from the star due to its radiation. In this image, cyan highlights the lion’s mane, which is the interior of a dust shell that is being illuminated by the central star. Within the mane, toward its edges, are purple clumps that look like they have cometary tails. These fluffy structures are also dust, which have managed to survive so far and protect the structures behind them.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    07:29:10.76
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    +20:54:42.49
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Gemini
  • 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 5,000 light-years away
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    This image is about 1.8 arcminutes across (2.6 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: 9548 (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.
    19 Nov. 2025
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F115W, F187N, F212N, F335M, F1000W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Lion Nebula, NGC 2392, Caldwell 39
  • Object Description
    Object DescriptionThe type of astronomical object.
    Planetary nebula
  • Release Date
    August 10, 2026
  • Science Release
    Lion Nebula Roars to Life With NASA’s Webb
  • Credit
    Image: NASA, ESA, CSA, STScI; Image Processing: Alyssa Pagan (STScI)

Downloads

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Planetary nebula NGC 2392, also called the Lion Nebula, against the black background of space. The nebula is in the center, circular in shape, and looks like a male lion’s head. In the very center is a small, bluish-white circle with eight-point diffraction spikes, a white dwarf star. Surrounding the star are light purple-red cavernous bubbles and shell-like rings. The bubbles and shells collectively form an oval with two small, wide arcs near the top, reminiscent of a lion’s face and its ears. What appears to be extended outward from the lion’s face is a thick ring of cyan material. The width of the ring is consistent throughout and resembles a mane. The area closest to the lion’s face looks cloudy, while the edges of the mane look like there are purple clumps of dust with comet-like tails and strands. In the background are distant galaxies and stars. Some galaxies appear as small purple points of light and others with visible blue spiral structures. A couple of the stars have 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 instruments on the Webb Space Telescope. 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, Green: F1000W, Red: F1500W

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Details

Last Updated
Aug 10, 2026
Contact
Media

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