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The western section of the Veil Nebula (NGC 6960) and the eastern section (NGC 6962-5) are about 3 degrees apart. They are both remnants of a supernova that occurred several thousand years ago. They have a low surface brightness and are hard to see through a telescope except under nice dark skies. A nebula filter such as an OIII filter can greatly enhance the view, and a large telescope can show a wealth of detail in these supernova remnants. |
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Evening visibility: | June-December | ||
Best viewed with: | telescope | ||
Printable chart (pdf) | View larger image | ||
Directions: Start by finding the Summer Triangle, which consists of the three of the brightest stars in the sky--Vega, Deneb, and Altair. The Summer Triangle is high overhead throughout the summer, and it sinks lower in the west as fall progresses. For this star hop, start from Deneb, the first-magnitude star that forms the tail of Cygnus, the swan (or if you visualize the brightest stars of Cygnus as a cross shape, Deneb is at the top of the cross). |
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From Deneb, look to the southwest for Sadr, the magnitude 2 star at the center of the Cygnus cross shape and then southeast to Epsilon (ε) on the eastern arm of the cross. Then look 4 degrees to the south for 4th magnitude 52 Cygni, which almost touches the brightest streak of NGC 6960. To find NGC 6992-5, move 3 degrees to the east. |
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Star charts created with Cartes du Ciel | |||