M27 - The Dumbbell nebula


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Designations:
M27, NGC 6583
Object Type:
Constellation:
Vulpecula
19 hr 59.6 min
+22° 43 min
7.3
Size:
8.0 X 5.7 arcminutes
Distance:
Discoverer:
Messier 1764

Visual Description:

"The August sky contains many delightful planetary nebulae - ephemeral spheres of blue and green gas that float amid the pearly star currents of the Milky Way. Certainly one of the most observed is the Dumbbell nebula, M27 in Vulpecula".[1] "M27, the most famous of planetary nebulae, got its nickname many years after its discovery from its resemblance to a bodybuilder's hand weight. M27 is one of the closer planetaries (815 light years away) and its physical diameter of 1.2 light years also makes it one of the larger. The gaseous material was blown from the blue-dwarf star now at its center during one of the star's death throes 48,000 years ago which makes M27 more than twice as old as typical planetaries. M27 is a multiple-shell planetary. One shell, of doubly ionized oxygen, is expanding at a velocity of 9 miles per second, while another shell, of ionized nitrogen, is expanding at 20 miles per second. From our vantage point, the whole gaseous ring is swelling 6 sec per century. The gas shells glow from excitation by ultra-violet radiation emitted by the hot central star." [2]
 


Telescope:
Focal Length:
1200
Mount:
Camera
Guider:
Exposures:
80 minutes luminance, 40 minutes for each color (red, green and blue)
Location:
Software:
CCDSoft (Image Acquisition), CCDStack, Photoshop



[1]Walter Scott Houston "Deep-Sky Wonders" with selections and commentary by Stephen James O'Meara. Page 182
ISBN number 0-933346-93-X.

[2]Steven James O'Meara "The Messier Objects" by Stephen James O'Meara. Page. 102. ISBN number 0-521-55332-6







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