V1073 Scorpii

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V1073 Scorpii
Scorpius constellation map.svg
Red circle.svg
Location of V1073 Scorpii (circled)
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
k Sco, V1073 Sco, CD 33°11706, HD  154090, HIP  83574, HR  6334, SAO  208377 [10]
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]

A light curve for V1073 Scorpii, adapted from Lefevre et al. (2009) V1073ScoLightCurve.png
A light curve for V1073 Scorpii, adapted from Lefèvre et al. (2009)

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]

Related Research Articles

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−13.8
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References

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