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Search results - "perseus"
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NGC281 - The Pacman Nebula RGB56 viewsNGC 281 is an H II region in the constellation of Cassiopeia and part of the Perseus Spiral Arm. It includes or is near the open cluster IC 1590, the double star HD 5005, and several Bok globules. It is visible in amateur telescopes from dark sky locations. It is sometimes unofficially referred to as the Pacman Nebula owing to its fancied resemblance to the eponymous hero of the arcade game Pac-Man.
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NGC1499 - California Nebula in Perseus24 viewsThe California Nebula (NGC 1499) is an emission nebula located in the constellation Perseus. It is so named because it appears to resemble the outline of the US State of California on long exposure photographs. It is almost 2.5° long on the sky and, because of its very low surface brightness, it is extremely difficult to observe visually. It lies at a distance of about 1,000 light years f
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Double Cluster in Perseus32 views8th September 2006, Balbriggan Co.Dublin. This image was used on the Sky At Night TV show it was a proud moment for me Consedering it was one of my first images.The Double Cluster is the common name for the naked-eye open clusters NGC 884 and NGC 869, which are close together in the constellation Perseus. NGC 884 and NGC 869 are at distances of 7600 and 6800 light-years away, respectively, so they are close to one another in space as well.They are relatively young clusters, with NGC 869 5.6 million years
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Melotte15 Inside The Heart Nebula61 viewsThe Heart Nebula, IC 1805, lies some 7500 light years away from Earth and is located in the Perseus arm of the Galaxy in the constellation Cassiopeia. This is an emission nebula showing glowing gas and darker dust lanes. The nebula is formed by plasma of ionized hydrogen and free electrons.
The nebula's intense red output and its configuration are driven by the radiation emanating from a small group of stars near the nebula's center. This open cluster of stars known as Melotte 15 contains a few bright star
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Melotte-15, Core Cluster of IC180586 viewsMelotte-15, Core Cluster of IC1805. The crucible of star formation lies within giant molecular clouds scattered throughout the spiral arms of galaxies. In our own galaxy some of the best known star forming regions lie in a chain of HII clouds located in the Perseus spiral arm of our galaxy. From west to east the chain of giant HII regions are known as W3, W4, and W5, which are also catalogued as IC 1795, IC 1805, and IC 1848.
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