Little Red Dot Abell2744-QSO1 (NIRCam Image)
This is an image from NIRCam (Near Infrared Camera) on Webb that shows Abell2744-QSO1, magnified and triply imaged by galaxy cluster Abell 2744.
Abell2744-QSO1 (QSO1) is a prototypical Little Red Dot, one of the first of hundreds of tiny glowing flecks of infrared light that Webb has found speckling the early Universe. QSO1 is roughly 1,300 light-years across and with a cosmological redshift (z) of 7, its light dates back to just 700 million years after the Big Bang, when the Universe was only 5% of its current age.
QSO1 is ideal for study because it is gravitationally lensed, both magnified and triply imaged by Abell 2744, the intervening mega-cluster of galaxies that warps its surrounding space-time.
Detailed study of the brightest of the three lensed images, QSO1A (upper right), shows that the object consists of a central supermassive black hole 50 million times the mass of the Sun, surrounded by a cloud of hydrogen and helium gas with very small amounts of heavier elements like oxygen. Unlike supermassive black holes in nearby galaxies, which make up only a tiny fraction of their host galaxy’s total mass, QSO1’s black hole contains twice as much mass as the galactic material surrounding it.
[Image description: Image showing hundreds of bright objects of different size, colour, and shape on the black background of space. Colours range from white to deep red. Shapes include elliptical, spiral, dot-like, dash-like, and arcuate.Three objects in the central part of the image are called out with small white boxes that contain images of the three objects. From top to bottom these are labeled QSO1A, QSO1B, and QSO1C. At the centre of each box is a tiny, circular red dot. QSO1A (top) is notably larger, brighter, and clearer than the other two. QSO1B, in the middle, is the smallest and fuzziest, and is somewhat washed out by the light of a larger white object next to it.]
Credit:NASA, ESA, CSA, L. Furtak (Ben-Gurion University), R. Maiolino (Cambridge), F. D'Eugenio (Cambridge), I. Juodžbalis (Cambridge), H. Übler (MPE), C. Marconcini (University of Florence). Image processing: A. Pagan
About the Image
| Id: | weic2609a | |
|---|---|---|
| Type: | Collage | |
| Release date: | 27 May 2026, 17:00 | |
| Related releases: | weic2609 | |
| Size: | 11542 x 8657 px | |