Due to the lapse in federal government funding, NASA is not updating this website.

Suggested Searches

1 min read

Dwarf Galaxy WLM (NIRCam Image)

Image showing thousands of clearly differentiated objects (stars and background galaxies) of various color, size, shape, and brightness.

A portion of the dwarf galaxy Wolf–Lundmark–Melotte (WLM) captured by the James Webb Space Telescope’s Near-Infrared Camera. The image demonstrates Webb’s remarkable ability to resolve faint stars outside the Milky Way. Color translation: 0.9-micron light is shown in blue, 1.5-micron in cyan, 2.5-micron in yellow, and 4.3-micron in red (filters F090W, F150W, F250M, and F430M). 

 Read the story, watch a zoom-in, or explore a side-by-side comparison.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    00:01:57.429
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -15:28:52.49
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Cetus
  • 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 million light-years away
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    The image is about 2 arcminutes across (1,700 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 from JWST data from proposal: 1334 (D. Weisz)

  • 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.
    23-24 July 2022
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F090W, F150W, F250M, F430M
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Wolf–Lundmark–Melotte (WLM)
  • Object Description
    Object DescriptionThe type of astronomical object.
    Barred, irregular, dwarf galaxy
  • Release Date
    November 9, 2022
  • Credit
    NASA, ESA, CSA, Kristen McQuinn (Rutgers University); Image Processing: Zoltan Levay (STScI)

Downloads

  • Full Res (For Display), 4134 × 4134
    png (26.7 MB)
  • Full Res (For Print), 4134 × 4134
    tif (48.92 MB)
  • 2000 × 2000
    png (7.17 MB)
Image showing thousands of clearly differentiated objects (stars and background galaxies) of various color, size, shape, and brightness.
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 NIRCam instrument. Several filters were used to sample different infrared 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: F090W, Cyan: F150W, Yellow: F250M, Red: F430M

Share

Details

Last Updated
Aug 28, 2025
Contact
Media

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

Science Credit

NASA, ESA, CSA, Kristen McQuinn (Rutgers University)

Image Processing Credit

Zoltan Levay (STScI)