| Revision for Little Dumbbell Nebula | ||
| Previous Revision, by Richard Fluiraniz M. [2023-01-10 03:59:24] | → | Selected revision, by Richard Fluiraniz M. [2023-01-10 04:01:10] |
| DISCOVERER | ||
| CMDR threeleaf | → | CMDR threeleaf |
| NAME | ||
| Little Dumbbell Nebula. | → | Little Dumbbell Nebula |
| SYSTEMNAME | ||
| GCRV 950 | → | GCRV 950 |
| CATEGORY | ||
| Nebulae | → | Nebulae |
| CATEGORY 2 | ||
| → | ||
| 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 | ||
| → | ||
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.
| → |
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.
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| JOURNAL | ||
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| OBSERVATORY | ||
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