NGC 346 - JWST - MIRI - Magnification and reconstruction via AI.

            This is our version, via our artificial intelligence model, of the image provided by the JWST team on October 10, 2023 at 14.00 UTC. This is what the JWST observed with the MIRI (Mid-InfraRed Instrument) with the observations of October 10, 2022 (yes, exactly 1 year ago) regarding NGC 346. The image traces the emission of cold gases and dust. In this image, the blue represents silicates and chemical molecules known as polycyclic aromatic hydrocarbons, or PAHs. The red, more diffuse emission comes from the hot dust heated by the brightest and most massive stars in the heart of the region. Bright spots and filaments mark areas with an abundant number of protostars.

The file is available at 149.7 million pixels for download at a resolution of 11976x12500 pixels.

Map of wavelengths/colours from MIRI:
Red F2100W;
Yellow F1500W;
Green F1130W
Cyan F1000W;
Blue F770W.

Constellation: Tucana.
Object Description: Cluster and Nebulosity in the Small Magellanic Cloud.
Distance: 200,000 light-years.
Dimensions:  This image is about 3.4 arcminutes across (200 light-years).
Exposure Date: October 10, 2022.
Release Date: October 10, 2023 14:00 UTC.
 
Credit for science:  NASA, ESA, CSA, STScI, Nolan Habel (NASA-JPL); for image processing: Patrick Kavanagh (Maynooth University). Magnification and reconstruction via AI by PipploIMP.

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Taken on: October 10, 2022

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