This is an old revision of this page, as edited by Praemonitus (talk | contribs) at 18:45, 25 June 2018 (Non-notable). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
Revision as of 18:45, 25 June 2018 by Praemonitus (talk | contribs) (Non-notable)(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)| An editor has nominated this article for deletion. You are welcome to participate in the deletion discussion, which will decide whether or not to retain it.Feel free to improve the article, but do not remove this notice before the discussion is closed. For more information, see the guide to deletion. Find sources: "GJ 1151" – news · newspapers · books · scholar · JSTOR%5B%5BWikipedia%3AArticles+for+deletion%2FGJ+1151%5D%5DAFD |
 | The topic of this article may not meet Misplaced Pages's notability guideline for astronomical objects. Please help to demonstrate the notability of the topic by citing reliable secondary sources that are independent of the topic and provide significant coverage of it beyond a mere trivial mention. If notability cannot be shown, the article is likely to be merged, redirected, or deleted. Find sources: "GJ 1151" – news · newspapers · books · scholar · JSTOR (June 2018) (Learn how and when to remove this message) |
GJ 1151 is a red dwarf star of spectral type M4.5V, located in constellation Ursa Major at 26.7 light-years from Earth.
Distance
In 1991, Gliese et al gave parallax (πp) as 121.8 ± 3.0 mas. In 1995, van Altena gave parallax as 122.1 ± 2.9 mas. In 2014, Dittman et al gave parallax as 130.60 ± 3.60 mas.
See also
References
- ^ VizieR, Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)
- Gliese, W.; Jahreiß, H. (1991). "GI 338". Preliminary Version of the Third Catalogue of Nearby Stars.
- Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Berta-Thompson, Zachory K. (2014). "TRIGONOMETRIC PARALLAXES FOR 1507 NEARBY MID-TO-LATE M DWARFS". The Astrophysical Journal. 784 (2): 156. arXiv:1312.3241. Bibcode:2014ApJ...784..156D. doi:10.1088/0004-637X/784/2/156. ISSN 0004-637X.
| Known celestial objects within 20 light-years | |||||||||||||||||||||||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||||||||||||||||||||||||||||||||||
| |||||||||||||||||||||||||||||||||||||||||||
| |||||||||||||||||||||||||||||||||||||||||||
| |||||||||||||||||||||||||||||||||||||||||||
| Italic are systems without known trigonometric parallax. | |||||||||||||||||||||||||||||||||||||||||||
 | This star-related article is a stub. You can help Misplaced Pages by expanding it. |