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Multiwavelength View of NGC 346 (Spitzer, NTT, XMM-Newton)

A multiwavelength view of NGC 346. The center of the image contains wispy green-yellow material, and arcs of orange and pink gas that form a boat-like shape. Among the center is a large cluster of blue-white stars.

This image of the star-forming cloud NGC 346 is a combination of multiwavelength light from NASA's Spitzer Space Telescope (infrared), the European Southern Observatory's New Technology Telescope (visible), and the European Space Agency's XMM-Newton space telescope (X-ray). Webb’s sharper infrared vision will allow astronomers to survey in greater detail developing stars still encased in their natal cocoons of gas and dust.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    00h 59m 18s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -72° 10' 48.0"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Tucana
  • 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.
    210,000 light-years away (64,000 parsecs)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    NGC 346
  • Object Description
    Object DescriptionThe type of astronomical object.
    Star-forming region in the Small Magellanic Cloud
  • Release Date
    December 12, 2018
  • Science Release
    NASA’s Webb Telescope Will Provide Census of Fledgling Stars in Stellar Nursery
  • Credit
    Image: NASA, Caltech, Dimitrios Gouliermis (MPIA)

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    jpg (3.97 MB)

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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, Caltech, Dimitrios Gouliermis (MPIA)