Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Scorpius |
Right ascension | 16h 15m 37.27028s[1] |
Declination | –08° 22′ 09.9821″[1] |
Apparent magnitude (V) | 5.503[2] |
Characteristics | |
Spectral type | G2 Va[3] |
U−B color index | +0.18[4] |
B−V color index | +0.64[4] |
Variable type | Sun-like[5] |
Astrometry | |
Radial velocity (Rv) | 11.71±0.12[1] km/s |
Proper motion (μ) | RA: 232.230 mas/yr[1] Dec.: −495.378 mas/yr[1] |
Parallax (π) | 70.7371 ± 0.0631 mas[1] |
Distance | 46.11 ± 0.04 ly (14.14 ± 0.01 pc) |
Absolute magnitude (MV) | 4.77[2] |
Details[6] | |
Mass | 1.01±0.02 M☉ |
Radius | 1.007±0.011 R☉ |
Luminosity | 1.043±0.005 L☉ |
Surface gravity (log g) | 4.437±0.013 cgs |
Temperature | 5,817±4[7] K |
Metallicity [Fe/H] | 0.06±0.03 dex |
Rotation | 22.7±0.5 d[8] |
Age | 2.9±0.5[9] Gyr 5.64 or 7.18[7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
18 Scorpii is a solitary star located at a distance of some 46.1 light-years (14.13 parsecs) from the Sun at the northern edge of the Scorpius constellation. It has an apparent visual magnitude of 5.5,[2] which is bright enough to be seen with the naked eye outside of urban areas. The star is drifting further away with a radial velocity of +11.6.[2]
18 Scorpii has some physical properties in common with the Sun, a G-type star. Cayrel de Strobel (1996) included it in her review of the stars most similar to the Sun,[10] and Porto de Mello & da Silva (1997) identified it as a younger solar twin.[11][12] Some scientists therefore believe the prospects for life in its vicinity are good.
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