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 +4.8. 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. It has an absolute magnitude of −6.8
This object is a massive supergiant star with a stellar classification of B0.7 Ia. It was found to be a variable star in 1996, when the Hipparcos data was analysed. It was given its variable star designation in 1999. It is an α Cygni variable; 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. The star is around 4.2 million years old and is a member of the Upper Scorpius subgroup of the Sco OB2 association. V1073 Scorpii is considered a "runaway" star, showing a peculiar velocity of more than 37 km/s relative to its neighbourhood. No bow shock has been detected from its motion through interstellar space. V1073 Sco has a 14th magnitude visual companion, which is an unrelated background object according to its Gaia Data Release 2 parallax.
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![V1073 Scorpii: A light curve for V1073 Scorpii, adapted from Lefèvre et al. (2009)[12]](https://upload.wikimedia.org/wikipedia/commons/thumb/1/12/V1073ScoLightCurve.png/1280px-V1073ScoLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
