Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Scorpius |
Right ascension | 17h 04m 49.35254s[1] |
Declination | −34° 07′ 22.5483″[1] |
Apparent magnitude (V) | +4.87[2] |
Characteristics | |
Spectral type | B0.7 Ia[3] |
U−B color index | −0.69[2] |
B−V color index | +0.26[2] |
Variable type | α Cyg[4] |
Astrometry | |
Radial velocity (Rv) | 7.00[5] km/s |
Proper motion (μ) | RA: +0.600[1] mas/yr Dec.: −2.015[1] mas/yr |
Parallax (π) | 1.1161 ± 0.2097 mas[1] |
Distance | approx. 2,900 ly (approx. 900 pc) |
Absolute magnitude (MV) | −6.8[6] |
Details | |
Mass | 28[7] 19.7±1.0[8] 27.11±8.39[9] M☉ |
Radius | 36.0[6][3] R☉ |
Luminosity | 302,000[6] L☉ |
Surface gravity (log g) | 2.70[7] 2.65[3] cgs |
Temperature | 20,800[9] 22,500[3] K |
Rotational velocity (v sin i) | 47[7] km/s |
Age | 4.2±0.3[8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
V1073 Scorpii is a variable star in the constellation Scorpius. It has a non-Greek Bayer designation of k Scorpii. The star has a blue-white hue and is visible to the naked eye with an apparent visual magnitude that fluctuates around +4.87.[2] Parallax measurements yield a distance estimate of approximately 2,920 ly (896 pc) from the Sun, and it is drifting further away with a radial velocity of +7 km/s.[5] It has an absolute magnitude of −6.8[6]
This object is a massive supergiant star with a stellar classification of B0.7 Ia.[3] It is an α Cygni variable;[12] a supergiant that pulsates erratically on a timescale of days to weeks with an amplitude of less than a tenth of a magnitude. A simplistic fitting of Hipparcos data suggests a periodicity of 1.6 days.[13][11] The star is around 4.2[8] million years old and is a member of the Upper Scorpius subgroup of the Sco OB2 association.[14] V1073 Scorpii is considered a "runaway" star, showing a peculiar velocity of more than 37 km/s relative to its neighbourhood.[8] No bow shock has been detected from its motion through interstellar space.[15]
V1073 Sco has a 14th magnitude visual companion,[16] which is an unrelated background object according to its Gaia Data Release 2 parallax.[17]
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