G 9-38

GJ 1116
Astrometry
Parallax (π)191.3 ± 2.5[1] mas
Distance17.0 ± 0.2 ly
(5.23 ± 0.07 pc)
Other designations
The system:
A:
B:
Database references
SIMBADThe 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. 1 2 Gliese, W.; Jahreiß, H. (1991). "GJ 1116". Preliminary Version of the Third Catalogue of Nearby Stars. Retrieved 2014-11-23.
  2. Van Altena W. F.; Lee J. T.; Hoffleit E. D. (1995). "GCTP 2835.01". The General Catalogue of Trigonometric Stellar Parallaxes (Fourth ed.).
  3. Luyten, Willem Jacob (1979). "LHS 2076". LHS Catalogue, 2nd Edition.
  4. Luyten, Willem Jacob (1979). "NLTT 20638". NLTT Catalogue.
  5. Luyten, Willem Jacob (1979). "LHS 2077". LHS Catalogue, 2nd Edition.
  6. Luyten, Willem Jacob (1979). "NLTT 20637". NLTT Catalogue.
  7. Vizier query: Name=G* 1116, Centre de Données astronomiques de Strasbourg , accessed 30 December 2012.
  8. Nearby Stars Catalog (NSC), Planetary Habitability Laboratory, University of Puerto Rico at Aerecibo accessed 31 December 2012.
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