Astronomy:Xi Gruis
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Short description: Star in the constellation Grus
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Grus |
| Right ascension | 21h 32m 05.87583s[1] |
| Declination | −41° 10′ 45.5242″[1] |
| Apparent magnitude (V) | 5.29[2] |
| Characteristics | |
| Spectral type | K0 III[3] |
| B−V color index | +1.10[2] |
| Astrometry | |
| Radial velocity (Rv) | −9.81±0.13[1] km/s |
| Proper motion (μ) | RA: +19.427[1] mas/yr Dec.: +11.278[1] mas/yr |
| Parallax (π) | 7.5904 ± 0.1226[1] mas |
| Distance | 430 ± 7 ly (132 ± 2 pc) |
| Absolute magnitude (MV) | −0.47[4] |
| Details | |
| Radius | 19.2±0.6[1] R☉ |
| Luminosity | 161.7±3.1[1] L☉ |
| Temperature | 4,703+76 −74[1] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
ξ Gruis, Latinised as Xi Gruis, is a solitary[6] star in the southern constellation of Grus, near the constellation border with Microscopium. It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.3.[2] The star is located about 430 light-years distant from the Sun, based on parallax, but is drifting closer with a radial velocity of −10 km/s.[1]
This is an evolved giant star with a stellar classification of K0 III,[3] having exhausted the supply of hydrogen at its core then cooled and expanded. It now has 19 times the girth of the Sun and is radiating 12 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,703 K.[1]
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 Johnson, H. L. et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99): 99, Bibcode: 1966CoLPL...4...99J.
- ↑ 3.0 3.1 Houk, N. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, 2, Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
- ↑ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ "ksi Gru -- Star", SIMBAD Astronomical Database (Centre de Données astronomiques de Strasbourg), http://simbad.u-strasbg.fr/simbad/sim-id?Ident=ksi+Gru, retrieved 2017-06-26.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869–879, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E.
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