Revision for Little Dumbbell Nebula | ||
Previous Revision, by Richard Fluiraniz M. [2023-01-10 04:01:10] | → | Selected revision, by CMDR Marx [2023-01-11 12:38:19] |
DISCOVERER | ||
CMDR threeleaf | → | CMDR threeleaf |
NAME | ||
Little Dumbbell Nebula. | → | Little Dumbbell Nebula |
SYSTEMNAME | ||
GCRV 950 | → | GCRV 950 |
CATEGORY | ||
Nebulae | → | Nebulae |
CATEGORY 2 | ||
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REGION | ||
Inner Orion Spur | → | Inner Orion Spur |
LATITUDE | ||
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LONGITUDE | ||
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CALLSIGN | ||
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SUMMARY | ||
The Little Dumbbell Nebula, also known as Messier 76, NGC 650/651, the Barbell Nebula, or the Cork Nebula, is a planetary nebula in the Elysian Shore. The system features stunning sights and anemones | → | The Little Dumbbell Nebula, also known as Messier 76, NGC 650/651, the Barbell Nebula, or the Cork Nebula, is a planetary nebula in the Elysian Shore. The system features stunning sights and anemones. |
DESCRIPTION | ||
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The Little Dumbbell Nebula circa 2014 (top) and from Little Dumbbell Sector ZA-N b7-0 (bottom), the closest system at 17.84 ly away
Very small compared to other planetary nebulas, The Little Dumbbell Nebula consists of 11 different stars which have (O class, T-tauris, K-class, M-class, L-class) and multiple small landables that feature geological and Prasinum Bioluminescent anemones. The second body (GCRV 950 2) is a non-landable silicate vapour atmospheric planet which features some stunning looking rings which reflect the parent O class. This is a great place to take pictures due to the multiple star sights and the ever-present O class. | → | The Little Dumbbell Nebula, also known as Messier 76, NGC 650/651, the Barbell Nebula, or the Cork Nebula, is a planetary nebula in the Elysian Shore. The system features stunning sights and anemones on the surfaces of moons. The Little Dumbbell Nebula circa 2014 (top) and from Little Dumbbell Sector ZA-N b7-0 (bottom), the closest system at 17.84 ly awayThe bodies found in the nebula's system consist of 11 different stars, an O class star orbited by a K star, T Tauri stars and red / brown dwarf stars, and multiple small landables which feature volcanism and Prasinum Bioluminescent anemones. The second body (GCRV 950 2) is a thick silicate vapour atmospheric planet which features some stunning looking rings that reflect the parent O class star's light. This is a great place to take pictures with the various stars of the system in the frame. |
JOURNAL | ||
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OBSERVATORY | ||
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