On 6 October 2026, NASA released a new NIRCam image of NGC 7129, a star-forming region about 3,300 light-years away. Webb observes in infrared light, revealing structures and stars hidden by dust. The display colours are assigned: gold marks hot atomic hydrogen, while red represents cooler molecular hydrogen affected by shocks from protostellar jets. [1]

The central star, LkH(alpha) 234, has an estimated mass of five to eight times the Sun’s and is still in the pre-main-sequence stage. Nearby are younger protostars, gathering matter and ejecting jets. The image provides details of different stages of star formation; it does not show stars born on publication day. [1]

Spitzer had already observed NGC 7129 in infrared light: one of its images is dated 12 February 2004. Different wavelengths were also translated into visible colours then. NASA highlights finer details in the new Webb image. Our editorial reading advice is to consult each image’s colour explanation, without inferring physical change from the different palettes alone. [2][1]