Psi Scorpii

White-hued star in the constellation Scorpius From Wikipedia, the free encyclopedia

Psi Scorpii, which is Latinized from ψ Scorpii, is a star in the zodiac constellation of Scorpius. It is white in hue and has an apparent visual magnitude of 4.94,[2] which is bright enough to be faintly visible to the naked eye. Based upon parallax measurements,[1] it is located at a distance of around 162 light years from the Sun. Data collected during the Hipparcos mission suggests it is an astrometric binary, although nothing is known about the companion.[11][12] The system is drifting closer to the Sun with a radial velocity of −5 km/s.[4]

Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...
ψ Scorpii
Observation data
Epoch J2000      Equinox J2000
Constellation Scorpius
Right ascension 16h 12m 00.01043s[1]
Declination −10° 03 50.8353[1]
Apparent magnitude (V) 4.94[2]
Characteristics
Spectral type A1 V[3]
U−B color index +0.11[2]
B−V color index +0.09[2]
Astrometry
Radial velocity (Rv)−5.10[4] km/s
Proper motion (μ) RA: −18.000[1] mas/yr
Dec.: −36.188[1] mas/yr
Parallax (π)20.1801 ± 0.2617 mas[1]
Distance162 ± 2 ly
(49.6 ± 0.6 pc)
Absolute magnitude (MV)+1.55[5]
Details
Mass2.0[6] M
Radius2.2[7] R
Luminosity18.6[8] L
Surface gravity (log g)4.00[6] cgs
Temperature8,846±301[6] K
Rotational velocity (v sin i)42.3±0.6[9] km/s
Age451[6] Myr
Other designations
ψ Sco, 15 Scorpii, BD−09°4324, FK5 3280, GC 21780, HD 145570, HIP 79375, HR 6031, SAO 141022[10]
Database references
SIMBADdata
Close

The visible component is an A-type main sequence star with a stellar classification of A1 V;[3] a class of star that is still fusing hydrogen at its core. It has around twice[6] the mass and 2.2[7] times the radius of the Sun, and is shining with 18.6 times the Sun's luminosity.[8] The effective temperature of the star's outer atmosphere is 8,846 K. Psi Scorpii is around 451 million years old and is spinning with a projected rotational velocity of 42.3 km/s.[6]

References

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