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Constellation | Scorpius |
Right ascension | 17 49 51.48081 |
Declination | −37° 02′ 35.8975″ |
Apparent magnitude (V) | 3.21 |
Characteristics | |
Spectral type | K2 III |
U−B color index | +1.19 |
B−V color index | +1.17 |
Astrometry | |
Radial velocity (Rv) | +24.7 km/s |
Proper motion (μ) | RA: 40.59 mas/yr Dec.: 27.24 mas/yr |
Parallax (π) | 25.92 ± 0.15 mas |
Distance | 125.8 ± 0.7 ly (38.6 ± 0.2 pc) |
Details | |
Mass | 1.44 ± 0.21 M☉ |
Radius | 16 R☉ |
Luminosity | 95 ± 6 L☉ |
Temperature | 4,538 K |
Other designations | |
G Sco, CD–37 11907, FK5 669, HD 161892, HIP 87261, HR 6630, SAO 209318. |
G Scorpii (G Sco) is a star in the constellation Scorpius. It is an orange K-type giant with an apparent magnitude of +3.19. It is approximately 126 light years from Earth. The measured angular diameter of the primary star is 3.94 ± 0.21 mas. At the estimated distance of this system, this yields a physical size of about 16 times the radius of the Sun.
Just 8.5 arcminutes to the east is the globular cluster NGC 6441.
It was formerly known as "Gamma Telescopii" (γ Tel) and "Fuyue" (傅說) in ancient China.
See also
References
- ^ van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
- ^ Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99), Bibcode:1966CoLPL...4...99J.
- Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–170, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637.
- Wilson, Ralph Elmer (1953). General Catalogue of Stellar Radial Velocities. Washington: Carnegie Institution of Washington. Bibcode:1953QB901.W495.....
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: CS1 maint: postscript (link) - ^ Stello, D.; et al. (2008), "Oscillating K Giants with the WIRE Satellite: Determination of Their Asteroseismic Masses", The Astrophysical Journal Letters, 674 (1): L53 – L56, arXiv:0801.2155, Bibcode:2008ApJ...674L..53S, doi:10.1086/528936.
- ^ Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN 3540296921. The radius (R*) is given by:
- Richichi, A.; Percheron, I.; Khristoforova, M. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431: 773–777, Bibcode:2005A&A...431..773R, doi:10.1051/0004-6361:20042039
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