The topic of this articlemay not meet Wikipedia'sgeneral notability guideline. Please help to demonstrate the notability of the topic by citingreliable secondary sources that areindependent of the topic and provide significant coverage of it beyond a mere trivial mention. If notability cannot be shown, the article is likely to bemerged,redirected, ordeleted. Find sources: "Sh 2-312" – news ·newspapers ·books ·scholar ·JSTOR(October 2025) (Learn how and when to remove this message) |
| Nebula | |
|---|---|
Sh 2-312 seen very faintly,Gamma Pyxidis in lower-right corner | |
| Observation data:J2000epoch | |
| Right ascension | 08h 59m 12s |
| Declination | −25° 41′ 00″[1] |
| Apparent magnitude (V) | 17.82 |
| Apparent dimensions (V) | 12° x 3° |
| Constellation | Pyxis |
| Designations | LBN 1077 |
| See also:Lists of nebulae | |
Sh 2-312 is anebula in the southern constellation ofPyxis. It is very large and diffuse, making it largely ignored and unstudied outside of its relation to theGum Nebula. Sh 2-312 is located approximately 56 parsecs away fromRCW 22,[2] another nebula postulated to be a part of the larger Gum Nebula,[3] which is itself estimated to be approximately 300 parsecs in width based onangular diameter approximation.[4][5] It responds well toHydrogen-alpha filters; however, it requires extended exposure time to become visible during observation.[6]
This nebula-related article is astub. You can help Wikipedia byexpanding it. |