Apart from the rings of Saturn, the Ring Nebula (M57) is perhaps the most famous sky zone. We know that the bullet has come forward from the traditional point of view. When we look at our world, we look at the center of a sparkling gas cloud with a roughly barrel shape. But when we look at this fascinating photo of the combination of images taken from the ground, Hubble Space Telescope images and narrow band image data from the Subaru Telescope, we see that the folded large structures extend far beyond the familiar central zone of the Ring Nebula. Obviously, in this well-studied planetary nebula example, it is obvious that the glittering materials do not come from the planets. This shroud, which came from the gauntlet, actually came to the foreground from the outermost layers that were at the center of the cloud, and which had once thrown outwards during the death of a star that once resembled our Sun. The intense ultraviolet light from this central hot star ionizes the atoms in the gas. Ionizing oxygen atoms provide their own unique green biomass, while ionized hydrogen atoms bring the red emission to the sky. The center ring of the Ring Nebula has an approximate light width and is located at a distance of 2000 light from us. The nebula that accompanies the star skies that you can watch tonight is located in the instrument from the northern hemisphere constellations.
