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NGC 346 (NIRCam Image)

NGC 346, shown here in this image from NASA’s James Webb Space Telescope Near-Infrared Camera (NIRCam), is a dynamic star cluster that lies within a nebula 200,000 light years away. Webb reveals the presence of many more building blocks than previously expected, not only for stars, but also planets, in the form of clouds packed with dust and hydrogen.
The plumes and arcs of gas in this image contains two types of hydrogen. The pink gas represents energized hydrogen, which is typically as hot as around 10,000 °C (approximately 18,000 °F) or more, while the more orange gas represents dense, molecular hydrogen, which is much colder at around -200 °C (approximately -300 °F) or less, and associated dust.
The colder gas provides an excellent environment for stars to form, and, as they do, they change the environment around them. The effect of this is seen in the various ridges throughout, which are created as the light of these young stars breaks down the dense clouds. The many pillars of glowing gas show the effects of this stellar erosion throughout the region.
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.00:59:04.95
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.-72:10:09.15
- 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.200,000 light-years away (61,300 parsecs)
- DimensionsDimensionsThe physical size of the object or the apparent angle it subtends on the sky.This image is about 3.9 arcminutes across (240 light-years).
About the Data
- Data DescriptionData 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: 1227 (M. Meixner).
- InstrumentInstrumentThe science instrument used to produce the data.NIRCam
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.16 June 2022, 26 June 2022, 10 Oct 2022
- FiltersFiltersThe camera filters that were used in the science observations.F200W; F277W; F335M; F444W
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.NGC 346
- Object DescriptionObject DescriptionThe type of astronomical object.Cluster and Nebulosity in the Small Magellanic Cloud
- Release DateJanuary 11, 2023
- Science ReleaseNASA’s Webb Uncovers Star Formation in Cluster’s Dusty Ribbons
- CreditNASA, ESA, CSA, Olivia Jones (UK ATC), Guido De Marchi (ESTEC), Margaret Meixner (USRA); Image Processing: Alyssa Pagan (STScI), Nolan Habel (USRA), Laura Lenkić (USRA), Laurie Chu (NASA Ames)

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 specific 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: Red: F444W, Orange: F335M, Cyan: F277W, Blue: F200W

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NGC 346 (NIRCam Compass Image)
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Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov
NASA, ESA, CSA, Olivia Jones (UK ATC), Guido De Marchi (ESTEC), Margaret Meixner (USRA)
Alyssa Pagan (STScI), Nolan Habel (USRA), Laura Lenki? (USRA), Laurie Chu (NASA Ames)