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Designations:
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M27, NGC 6583
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Object
Type:
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Constellation:
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Vulpecula
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19 hr 59.6 min
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+22° 43 min
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7.3
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Size:
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8.0 X 5.7 arcminutes
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Distance:
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815 light years
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Discoverer:
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Messier 1764
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"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]
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Telescope:
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Focal Length:
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1200
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Mount:
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Camera
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Guider:
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Exposures:
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80 minutes luminance, 40 minutes for each color (red, green and blue)
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Location:
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Software:
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CCDSoft (Image Acquisition), CCDStack, Photoshop
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[2]Steven James O'Meara "The Messier Objects" by Stephen James O'Meara. Page. 102. ISBN number 0-521-55332-6