For comparison, this is equivalent to a mass of galaxies for adults, although the age of the universe at that time was only about 5-10 percent of the current age. Not only large ones, these red monsters also show the effectiveness of amazing star formation.
While galaxies can usually turn only about 20 percent of conventional material (gas and dust) in a halo of dark material into stars. This galaxy is able to convert almost 50 percent of the material, two to three times more effective than galaxies in the older times.
Initially, scientists suspected that the Supermasi -block hole was a trigger for this rapid growth. However, the distribution of light through these galaxies actually spreads evenly, which indicates that the process of forming stars is not concentrated in the center, as usual in active galaxies with the core of the supermasic galaxy.
NIRCAM/GRISM Spectroscope tool from James Webb plays an important role in this discovery. This advanced technology allows you to observe the infrared light from the stars forming zone, even if they are covered with dark dust grains, like soot.
This is what Webb makes us capable of “get into the fog” and reveal the size and true structure of the red monster. According to the λcdm model, Hello Dark Material acts as a space frame, pulling gas, which then cools and forms a star.
