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Serpens Center Crop (NIRCam Image)

A young star-forming region is filled with wispy orange, red, and blue layers of gas and dust. The upper left corner of the image is filled with mostly orange dust, and within that orange dust, there are several small red plumes of gas that extend from the top left to the bottom right, at the same angle. The center of the image is filled with mostly blue gas. At the center, there is one particularly bright star, that has an hourglass shadow above and below it. To the right of that is what looks a vertical eye-shaped crevice with a bright star at the center. The gas to the right of the crevice is a darker orange. Small points of light are sprinkled across the field, brightest sources in the field have extensive eight-pointed diffraction spikes that are characteristic of the Webb Telescope.

This image shows the center of the Serpens Nebula as seen by NASA’s James Webb Space Telescope’s Near-Infrared Camera (NIRCam).

The Serpens Nebula, located 1,300 light-years from Earth, is home to a particularly dense cluster of newly forming stars (~100,000 years old), some of which will eventually grow to the mass of our Sun. Webb’s image of this nebula revealed a grouping of aligned protostellar outflows (seen in the top left). These jets are signified by bright clumpy streaks that appear red, which are shock waves from the jet hitting surrounding gas and dust.

In this image, throughout the region, filaments and wisps of different hues represent reflected starlight from still-forming protostars within the cloud. In some areas, there is dust in front of that reflection, which appears here with an orange, diffuse shade.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    18:29:56.91
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    +1:14:45.77
  • 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.
    1,300 light-years
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is about 4.8 arcminutes across (1.4 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.

    The Webb observations include those from program 1611 (K. Pontoppidan). Image Processing: Alyssa Pagan (STScI)

  • Instrument
    InstrumentThe science instrument used to produce the data.
    NIRCam
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    26 April 2023, 12 May 2023
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F140M, F210M, F360M, F480M
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Serpens Nebula, HBC 672, [EC 92] 82
  • Object Description
    Object DescriptionThe type of astronomical object.
    Reflection nebula and star forming region
  • Release Date
    June 20, 2024
  • Science Release
    First-of-Its-Kind Detection Made in Striking New Webb Image
    Read the release
  • Credit
    Image: NASA, ESA, CSA, STScI, Klaus Pontoppidan (NASA-JPL), Joel Green (STScI)

Downloads

  • Full Res (For Print), 9658 × 8036
    tif (89.92 MB)
  • Full Res (For Display), 9658 × 8036
    png (95.58 MB)
  • 2000 × 1664
    png (4.01 MB)
A young star-forming region is filled with wispy orange, red, and blue layers of gas and dust. The upper left corner of the image is filled with mostly orange dust, and within that orange dust, there are several small red plumes of gas that extend from the top left to the bottom right, at the same angle. The center of the image is filled with mostly blue gas. At the center, there is one particularly bright star, that has an hourglass shadow above and below it. To the right of that is what looks a vertical eye-shaped crevice with a bright star at the center. The gas to the right of the crevice is a darker orange. Small points of light are sprinkled across the field, brightest sources in the field have extensive eight-pointed diffraction spikes that are characteristic of the Webb Telescope.
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 NIRCam instrument. Several filters were used to sample medium 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: F140M, Cyan: F210M, Orange: F360M, Red: 480M

Related Images & Videos

A rectangular image with black vertical rectangles at the bottom left and top right to indicate missing data. A young star-forming region is filled with wispy orange, red, and blue layers of gas and dust. The upper left corner of the image is filled with mostly orange dust, and within that orange dust, there are several small red plumes of gas that extend from the top left to the bottom right, at the same angle. The center of the image is filled with mostly blue gas. At the center, there is one particularly bright star, that has an hourglass shadow above and below it. To the right of that is what looks a vertical eye-shaped crevice with a bright star at the center. The gas to the right of the crevice is a darker orange. Small points of light are sprinkled across the field, brightest sources in the field have extensive eight-pointed diffraction spikes that are characteristic of the Webb Telescope.

Serpens (NIRCam Image)

In this image of the Serpens Nebula from the Near-Infrared Camera (NIRCam) on NASA’s James Webb Space Telescope, astronomers found a grouping of aligned protostellar outflows within one small region (the top left corner). In the Webb image, these jets are signified by bright...

A portion of the young star-forming region Serpens Nebula. It’s filled with wispy orange and red layers of gas and dust, and within that orange dust, there are several small red plumes of gas that extend from the top left to the bottom right, at the same angle. There are wispy blue filaments of glass in the bottom right corner of the image. Small points of light are sprinkled across the field, brightest sources in the field have extensive eight-pointed diffraction spikes that are characteristic of the Webb Telescope.

Serpens North – Aligned Outflows Crop (NIRCam Image)

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An image labeled “James Webb Space Telescope, Serpens Nebula.” At the center of the image is a nebula on the black background of space. A young star-forming region is filled with wispy orange, red, and blue layers of gas and dust. The upper left corner of the image is filled with mostly orange dust, and within that orange dust, there are several small red plumes of gas that extend from the top left to the bottom right, at the same angle. The center of the image is filled with mostly blue gas. Small points of light are sprinkled across the field, brightest sources in the field have extensive eight-pointed diffraction spikes. At lower left, a white arrow pointing in the 8 o’clock direction is labeled N for north, while an arrow pointing in the 5 o‘clock direction is labeled E for east. At top right, a scale bar is labeled .25 light-years. At the bottom is a list of NIRCam filters in different colors, from left to right: F140M (blue), F210M (cyan), F360W (orange), F480M (red).

Serpens (NIRCam Compass Image)

This image of the Serpens Nebula, captured by Webb’s Near-Infrared Camera (NIRCam), 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...

A young star-forming region is filled with wispy orange, red, and blue layers of gas and dust. The upper left corner of the image is filled with mostly orange dust, and within that orange dust, there are several small red plumes of gas that extend from the top left to the bottom right, at the same angle. The center of the image is filled with mostly blue gas. At the center, there is one particularly bright star, that has an hourglass shadow above and below it. To the right of that is what looks a vertical eye-shaped crevice with a bright star at the center. The gas to the right of the crevice is a darker orange. Small points of light are sprinkled across the field, brightest sources in the field have extensive eight-pointed diffraction spikes that are characteristic of the Webb Telescope.

A Tour of the Serpens Nebula

This video tours the Serpens Nebula, a star-forming region that lies 1,300 light-years away from Earth. A new image of Serpens from NASA’s James Webb Space Telescope shows an intriguing group of aligned protostellar outflows within one region of the nebula. Protostellar outflows...

Telescope image including distant stars is overlaid with a semi-transparent graphic representing the constellations Serpens, Scutum, and Sagittarius. Thin blue lines connect the actual stars of the constellations.

Zoom to the Serpens Nebula

This zoom-in video shows the relative location of the Serpens Nebula on the sky. It begins with a ground-based photo by the late astrophotographer Akira Fujii, then transitions into a plate from the Digitized Sky Survey. Next, an image from NASA’s Spitzer Space Telescope...

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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, STScI, Klaus Pontoppidan (NASA-JPL), Joel Green (STScI)

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