Deepsky Top-100 (14): NGC 457
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When you scan Cassiopeia and its neighbouring constellations with binoculars, the star fields in Cassiopeia seem to be much richer than in Perseus and Cepheus. The reason for this is that in the Perseus and Cepheus Milky Way, large nearby dust clouds of our own spiral arm (the Orion arm) block the view, while in the Cassiopeia Milky Way there are no dust clouds to block the view. You actually look through a "window", across an inter-arm gap towards the Perseus arm, the next spiral arm toward the exterior of our galaxy. |
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Click here to download a printable finder chart (PDF)
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With a magnitude of 6.4, NGC 457 is one of the brightest open clusters in Cassiopeia. It contains about 80 to 100 stars, spread over an area of 16'. When you first look at the cluster through big binoculars or a telescope, you might think you see a little man, a bird (owl), or even ET waving at you. To me NGC 457 looks like a man with two bright sparkling eyes, his arms widely spread to welcome me. The two eyes are two bright stars, that will draw your attention immediately. They stand out well from the rest of the cluster. The brighter of the two stars is Phi Cassiopeia, a yellow star of magnitude 5.0. The other is HD 7902, a blue star of magnitude 7. |
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