G 161-71
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Hydra |
Right ascension | 09h 44m 54.224s |
Declination | −12° 20′ 54.43″ |
Characteristics | |
Spectral type | M5 |
Astrometry | |
Distance | 20.2±2.6[1] ly (6.2±0.8[1] pc) |
Other designations | |
G 161-71 NLTT 22503 2MASS J09445422-1220544 | |
Database references | |
SIMBAD | data |
G 161-71 is a red dwarf star, located in constellation Hydra at 6.2 parsecs (20.2 light-years) from Earth.[1]
Distance
G 161-71 distance estimates
Source | Parallax, mas | Distance, pc | Distance, ly | Distance, Pm | Ref. |
---|---|---|---|---|---|
Reid et al. (2002) | 6.2±0.8 | 20.2±2.6 | 191.3±24.7 | [1] | |
Scholz et al. (2005) | ~ 6.9 | ~ 22.5 | ~ 212.9 | [2] | |
Kirkpatrick et al. (2012) | ~ 153[nb 1] | ~ 6.5 | ~ 21.3 | ~ 201.7 | [3] |
Non-trigonometric distance estimates are marked in italic. The most precise estimate is marked in bold.
References
- ↑ 1.0 1.1 1.2 1.3 Reid, I. Neill; Kilkenny, D.; Cruz, K. L. (2002). "Meeting the Cool Neighbors. II. Photometry of Southern NLTT Stars". The Astronomical Journal 123 (5): 2822–2827. arXiv:astro-ph/0202460. Bibcode:2002AJ....123.2822R. doi:10.1086/339700.
- ↑ Scholz, R.-D.; Meusinger, H.; Jahreiß, H. (2005). "Search for nearby stars among proper motion stars selected by optical-to-infrared photometry. III. Spectroscopic distances of 322 NLTT stars". Astronomy and Astrophysics 442 (1): 211–227. arXiv:astro-ph/0507284. Bibcode:2005A&A...442..211S. doi:10.1051/0004-6361:20053004. Table1.dat.
- ↑ Kirkpatrick, J. D.; Gelino, C. R.; Cushing, M. C.; Mace, G. N.; Griffith, R. L.; Skrutskie, M. F.; Marsh, K. A.; Wright, E. L.; Eisenhardt, P. R.; McLean, I. S.; Mainzer, A. K.; Burgasser, A. J.; Tinney, C. G.; Parker, S.; Salter, G. (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal 753 (2): 156. arXiv:1205.2122. Bibcode:2012ApJ...753..156K. doi:10.1088/0004-637X/753/2/156.
Notes
- ↑ Averaged estimate derived from distances taken from Reid et al. (2003) (7.1 pc) and Riaz et al. (2006) (6 pc). Note: Kirkpatrick et al. (2012) says that 7.1 pc estimate is from Reid et al. (2007), but really it is from Reid et al. (2003), and LP 71-82 was not mentioned in Reid et al. (2007) at all.
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