Gliese 625

GJ 625
Observation data
Epoch J2000      Equinox J2000
Constellation Draco
Right ascension 16h 25m 24.62333s
Declination 54° 18 14.7733
Apparent magnitude (V) 10.17
Characteristics
Spectral type M2.0V
Astrometry
Parallax (π)153.46 ± 0.99[1] mas
Distance21.3 ± 0.1 ly
(6.52 ± 0.04 pc)
Other designations
AC +54 1646
G 202-48
G 226-7
G 225-62
NLTT 42804
GJ 625
PLX 3740.03
HIP 80459
TYC 3878-1193-1
2MASS J16252459+5418148
LSPM J1625+5418
Database references
SIMBADdata

Gliese 625 is a red dwarf star of spectral type M2.0V, located in constellation Draco at 21.3 light-years from Earth.[1]

Distance

Gliese 625 distance estimates

Source Parallax, mas Distance, pc Distance, ly Distance, Pm Ref.
Woolley et al. (1970) ~ 69 ~ 14.5 ~ 47.3 ~ 447.2 [2]
Gliese & Jahreiß (1991) 159.3±4.6 6.28+0.19
−0.18
20.5±0.6 193.7+5.8
−5.4
[3]
van Altena et al. (1995) 151.1±2.5 6.62±0.11 21.6±0.4 204.2+3.4
−3.3
[4]
Perryman et al. (1997) (Hipparcos) 151.93±1.11 6.58±0.05 21.47±0.16 203.1±1.5 [5]
Perryman et al. (1997) (Tycho) 126.70±27.00 7.9+2.1
−1.4
25.7+7
−4.5
243.5+66
−42.8
[6]
van Leeuwen (2007) 153.46±0.99 6.52±0.04 21.25±0.14 201.1±1.3 [1]
RECONS TOP100 (2012) 153.14±0.92[nb 1] 6.53±0.04 21.3±0.13 201.5±1.2 [7]

Non-trigonometric distance estimates are marked in italic. The most precise estimate is marked in bold.

References

  1. 1.0 1.1 1.2 van Leeuwen F. (2007). "HIP 80459". Validation of the new Hipparcos reduction.
  2. Woolley R.; Epps E. A.; Penston M. J.; Pocock S. B. (1970). "Woolley 625". Catalogue of stars within 25 parsecs of the Sun.
  3. Gliese, W. and Jahreiß, H. (1991). "Gl 625". Preliminary Version of the Third Catalogue of Nearby Stars.
  4. Van Altena W. F., Lee J. T., Hoffleit E. D. (1995). "GCTP 3740.03". The General Catalogue of Trigonometric Stellar Parallaxes (Fourth ed.).
  5. Perryman et al. (1997). "HIP 80459". The Hipparcos and Tycho Catalogues.
  6. Perryman et al. (1997). "HIP 80459". The Hipparcos and Tycho Catalogues.
  7. "RECONS TOP100". THE ONE HUNDRED NEAREST STAR SYSTEMS brought to you by RECONS (Research Consortium On Nearby Stars). 2012.

Notes

  1. Weighted parallax based on parallaxes from van Altena et al. (1995) and van Leeuwen (2007).