G 9-38
| Astrometry | |
|---|---|
| Parallax (π) | 191.3 ± 2.5[1] mas |
| Distance | 17.0 ± 0.2 ly (5.23 ± 0.07 pc) |
| Other designations | |
| Database references | |
| SIMBAD | The system |
| A | |
| B | |
G 9-38, also known as EI Cancri and GJ 1116, is a binary star system consisting of two M-type stars.[7] At 17.04 light-years from the Sun, the system is relatively nearby.[8]
References
- 1 2 Gliese, W.; Jahreiß, H. (1991). "GJ 1116". Preliminary Version of the Third Catalogue of Nearby Stars. Retrieved 2014-11-23.
- ↑ Van Altena W. F.; Lee J. T.; Hoffleit E. D. (1995). "GCTP 2835.01". The General Catalogue of Trigonometric Stellar Parallaxes (Fourth ed.).
- ↑ Luyten, Willem Jacob (1979). "LHS 2076". LHS Catalogue, 2nd Edition.
- ↑ Luyten, Willem Jacob (1979). "NLTT 20638". NLTT Catalogue.
- ↑ Luyten, Willem Jacob (1979). "LHS 2077". LHS Catalogue, 2nd Edition.
- ↑ Luyten, Willem Jacob (1979). "NLTT 20637". NLTT Catalogue.
- ↑ Vizier query: Name=G* 1116, Centre de Données astronomiques de Strasbourg , accessed 30 December 2012.
- ↑ Nearby Stars Catalog (NSC), Planetary Habitability Laboratory, University of Puerto Rico at Aerecibo accessed 31 December 2012.
- 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. Table with parallaxes.
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