Gliese 892

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Gl 892
Observation data
Epoch J2000      Equinox J2000
Constellation Cassiopeia
Right ascension 23h 13m 16.98s [1]
Declination +57° 10′ 06.1″ [1]
Apparent magnitude (V) 5.57
Characteristics
Spectral type K3 V
U−B color index 0.89
B−V color index 0.99
Variable type Suspected
Astrometry
Radial velocity (Rv) -18.5 km/s
Proper motion (μ) RA: 2075.07 ± 0.33 [1] mas/yr
Dec.: 295.45 ± 0.25 [1] mas/yr
Parallax (π) 152.76 ± 0.29[1] mas
Distance 21.35 ± 0.04 ly
(6.55 ± 0.01 pc)
Absolute magnitude (MV) 6.50
Details
Mass 0.81 M
Radius 0.80 ± 0.04[2] R
Luminosity 0.21 L
Temperature 4900 ± 7.9 [3] K
Metallicity 100%
Rotation ?
Age ? years
Other designations
Gl 892, HR 8832, BD +56°2966, HD 219134, HIP 114622, GCTP 5616.00, LHS 71, LFT 1767, LTT 16826, SAO 35236, FK5 875, Bradley 3077.

Coordinates: Sky map 23h 13m 16.98s, +57° 10′ 06.1″

Gliese 892 is a main sequence star in the constellation of Cassiopeia. It is smaller and less luminous than our Sun, with a spectral class of K3V, which makes it an orange-red hued star. Gl. 892 is relatively close to our system, with an estimated distance of 21.25 light years. This star is close to the limit of apparent magnitude that can still be seen by the unaided eye. The limit is considered to be magnitude 6 for most observers.

[edit] References

  1. ^ a b c d e van Leeuwen, F. (2007). "HIP 114622". Hipparcos, the New Reduction. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=I/311/hip2&recno=114236. Retrieved 2010-02-15. 
  2. ^ Perrin, M.-N.; Karoji, H. (1987). "Stellar radius determination from IRAS 12-micron fluxes". Astronomy and Astrophysics 172: 235–240. Bibcode 1987A&A...172..235P. 
  3. ^ Kovtyukh et al.; Soubiran, C.; Belik, S. I.; Gorlova, N. I. (2003). "High precision effective temperatures for 181 F-K dwarfs from line-depth ratios". Astronomy and Astrophysics 411 (3): 559–564. arXiv:astro-ph/0308429. Bibcode 2003A&A...411..559K. doi:10.1051/0004-6361:20031378. http://www.aanda.org/articles/aa/full/2003/46/aa3944/aa3944.html. 

[edit] External links


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