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

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. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.00h 59m 18s
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.-72° 10' 48.0"
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Tucana
- DistanceDistanceThe 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 NameObject NameA name or catalog number that astronomers use to identify an astronomical object.NGC 346
- Object DescriptionObject DescriptionThe type of astronomical object.Star-forming region in the Small Magellanic Cloud
- Release DateDecember 12, 2018
- Science ReleaseNASA’s Webb Telescope Will Provide Census of Fledgling Stars in Stellar Nursery
- CreditImage: NASA, Caltech, Dimitrios Gouliermis (MPIA)
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Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov
NASA, Caltech, Dimitrios Gouliermis (MPIA)







