M 27 | ||
 Click photo to see a larger image. | ||
| Description: | Known as the "Dumbbell Nebula," M27 is formed from gases expelled by an aging, giant star. These gases are ionized by radiation from this star and re-emit light in the visible wavelengths. | |
| Constellation: | Vulpecula | |
| Distance: | 1 thousand light years | |
| Apparent Size: | 5.8' | |
| Date: | July, August 2005 | |
| Equipment: | 12"RC @ f/9, ST10XME, AP1200 | |
| Exposure: | Ha(HaR)GB 4 hours 6nm Ha, RGB: 45 minutes each | |