Sigma Aquarii

Sigma Aquarii, Latinized from σ Aquarii, is a double star in the equatorial constellation of Aquarius, positioned about 1.3° to the south of the ecliptic. Due to its proximity to the ecliptic, this star is subject to occultation by the Moon. It has a white hue and is visible to the naked eye with an apparent visual magnitude of 4.81. Based upon parallax measurements, the distance to this star is approximately 175 light-years (54 parsecs). It is drifting further away with a radial velocity of +11 km/s.

Sigma Aquarii
Location of σ Aquarii (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 22h 30m 38.82286s
Declination −10° 40 40.7031
Apparent magnitude (V) 4.81
Characteristics
Spectral type A0 IVs
U−B color index −0.14
B−V color index −0.08
Astrometry
Radial velocity (Rv)+11.7±0.6 km/s
Proper motion (μ) RA: −5.708 mas/yr
Dec.: −25.626 mas/yr
Parallax (π)18.6424 ± 0.6871 mas
Distance175 ± 6 ly
(54 ± 2 pc)
Absolute magnitude (MV)0.29±0.23
Details
Mass2.87 M
Radius2.87 R
Luminosity105 L
Surface gravity (log g)4.07 cgs
Temperature10,115 K
Metallicity [Fe/H]+0.44 dex
Rotational velocity (v sin i)21 km/s
Age30 Myr
Other designations
σ Aqr, 57 Aquarii, BD–11°5850, FK5 1591, HD 213320, HIP 111123, HR 8573, SAO 165134
Database references
SIMBADdata

The stellar classification of Sigma Aquarii is A0 IVs, indicating that it is a subgiant star. The s qualifier means that its absorption lines are sharp (narrow) in comparison with standard stars, caused by a relatively slow rotation. It has been categorized as a hot Am star, meaning that it is a chemically peculiar, although this is now considered doubtful. The spectrum displays at least double the normal abundances of elements like magnesium, aluminum and silicon, while helium and scandium are under-abundant. Calcium, normally deficient in Am stars, has near-normal abundance.

The Hipparcos catalogue identified Sigma Aquarii as a possible astrometric binary with an orbital period of 654 days.

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