If you think it’s hard to imagine the size of our Sun (it’s 333,000 times larger than the entire Earth), you’ll be pleased to know that the Hubble Space Telescope reminds us of something even bigger. There is a galaxy in space that is 1.1 trillion times larger than our parent star. he was elected NGC 612and now we have a new image.

If it makes it any easier for you, NGC 612 is not as big as the Milky Way. The galaxy we live in is approximately 1.5 trillion times larger than the Sun.

According to the new version of the new image of NGC 612, this galaxy falls into several classifications that make it particularly interesting to observe. The most interesting thing is that it is an active galaxy. In active galaxies, a supermassive black hole powers the central region, creating an incredibly energetic heart of the galaxy. This heart also sprays gas almost at the speed of light. As a result of all this, the central point becomes so bright that it outshines the total light of every single star in the galaxy.

Although the new Hubble Space Telescope image of NGC 612 was taken sideways, meaning we’re seeing it from the side, it’s easy to conclude that the show is happening in the middle. It is noteworthy that in this region there is also a protrusion called the “central protrusion”. In contrast, the orange and dark red areas in this image represent the plane of matter called the “galactic disk.” This is where dust and cold hydrogen condense and where NGC 612’s (albeit rare) star formation occurs. The absence of bulges, disks, and spiral arms together indicate that this galaxy is lenticular, which is key to star formation. What will we get to next?

The statement also states that NGC 612 is a Seyfert galaxy, meaning that it emits a lot of infrared light, although it can also be seen in visible light. Infrared waves are a form of light that the human eye cannot see. But on the bright side, we have instruments like the James Webb Space Telescope and, of course, the Hubble Space Telescope, that can receive infrared signals to reveal these hidden sources; This image was partially created this way.

“NGC 612 is a Seyfert type II, which means that material near the center of the galaxy moves fairly silently around the core,” the statement continued. “The stars in this galaxy are extremely young, ranging in age from 40 to 100 million years.”

Let’s return to the biconvex point: This galaxy is a rare example of non-elliptical galaxies that emit radio. To date, astronomers have discovered only five such radio-emitting lenticular galaxies. “One theory explains NGC 612’s unusual radio emission by a past interaction with a companion spiral galaxy,” the report said. “Another theory focuses on a bright, dominant bulge in the galaxy similar to that seen in elliptical radio galaxies.” Source