NASA’s James WebSpace Telescope captured images of Sombero Galaxy’s mid -infrared wavelengths at the end of 2024. On June 3, 2025, NASA’s James Web released a picture of the Sombero Galaxy, when occupied with the stars when the dust lights towards the outer edges of the discs. The study of Sombero galaxy through the JWST and the Hubble telescope provides a variety of wavelengths, near infrared and mid -infrared, astronomers, as well as the mutual interference of material, as well as the formation and evolution of gas, dust and stars.
Nearest infrared image highlights the formation of dust and stars
NASA observed about this infrared snap near the JWST camera trapped near the JWST camera, the dust shows the amazing contradictions between the outer disk as well as the bright core of the galaxy. This image shows how the dust lane prevents the light coming from the stars on the edges of the galaxy. The firmly -filled central bulge contains about 2,000 2,000 star clusters, which are bright in nearly infrared wavelengths.
Comparative insights from middle infrared and nearest infrared observations
Comparing this new nearest infrared image with the old image of the web, which was released at the end of 2024, astronomers can understand the structure and evolution of dust, stars and gases inside the galaxy. The middle infrared image revealed the shining dust in the outer color, however, the infrared look shows the extent to which the wavelength passes. This shows the full stars full of stars.
Differences of the distribution of dust and dust in the splatwave have been revealed
This Split View image shows the differences in the appearance of the components of the galaxy, on the one hand, near infrastructure, and on the other side. In infrared, the red giant stars stand, while the hot blue stars are blurred, and the exterior disk looks complex due to variations in the dust distribution.
Symbols of ancient galaxy integration in Sombero Galaxy
The web survey on multi -wavelengths supports the theory that Somberiro Galaxy has at least more than one integration. The presence of internal disk, chemical diversity in globalular clusters, and dust structures lead to a complex form of interaction with other galaxies billions of years ago.
