53 Aquarii

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Template:Short description

53 Aquarii
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 5.56[2] (6.35/6.57)[3]
Characteristics
Spectral type G1 V + G5 V Fe–0.8 CH–1[4]
U−B Template:Engvar +0.09[2]
B−V Template:Engvar +0.61[2]
Astrometry
Radial velocity (Rv)+2.1[5] km/s
Proper motion (μ) RA: +200.59[1] mas/yr
Dec.: +14.51[1] mas/yr
Parallax (π)49.50±1.23 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)4.05[5] (4.94/4.87)[3]
Orbit[6]
Primary53 Aqr A
Companion53 Aqr B
Period (P)3500 yr
Semi-major axis (a)14.88″
Eccentricity (e)0.90
Inclination (i)44.13°
Longitude of the node (Ω)294.55°
Periastron epoch (T)B 2023
Argument of periastron (ω)
(secondary)
151.40°
Details
53 Aqr A
Mass1.01[7] Template:Solar mass
Radius1.11[8] Template:Solar radius
Luminosity1.39[8] Template:Solar luminosity
Surface gravity (log g)4.46[3] cgs
Temperature5,922[3] K
Metallicity [Fe/H]−0.10[3] dex
Rotational velocity (v sin i)8[9] km/s
Age0.18–0.37[10] Gyr
53 Aqr B
Mass0.99[7] Template:Solar mass
Surface gravity (log g)4.44[3] cgs
Temperature5,811[3] K
Metallicity [Fe/H]−0.19[3] dex
Rotational velocity (v sin i)9[9] km/s
Other designations
GJ 859, HIP 110778.[11]
53 Aqr A: BD−17 6521, HD 212698, HR 8545, LTT 9026, SAO 165078.
53 Aqr B: BD−17 6520, HD 212697, HR 8544, LTT 9025, SAO 165077.
Database references
SIMBAD53 Aqr
53 Aqr A
53 Aqr B

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53 Aquarii (abbreviated 53 Aqr) is a binary star[12] system in the equatorial constellation of Aquarius. 53 Aquarii is its Flamsteed designation though the star also bears the Bayer designation of f Aquarii. The combined apparent visual magnitude of the pair is a 5.56,[2] making it just visible to the naked eye in dark suburban skies. Based upon an annual parallax shift of 49.50 milliarcseconds for the first component, this system is located at a distance of approximately Script error: No such module "convert". from Earth.[1]

This is a wide binary star system with a projected separation of 100 astronomical units; indicating that the two stars are at least this distance apart.[8] The primary component is a solar-type main sequence star with a stellar classification of G1 V.[4] It has about 99% of the Sun's mass, 111% of the Sun's radius, and shines with 139% of the luminosity of the Sun.[8] This energy is being emitted from an outer envelope at an effective temperature of 5,922 K,[3] giving it the golden hue of a G-type star.[13] An examination of the primary component with the Spitzer Space Telescope failed to detect any infrared excess that might otherwise be an indication of a circumstellar debris disk.[8]

The companion is a slightly cooler star with an effective temperature of 5,811 K.[3] It has a stellar classification of G5 V Fe–0.8 CH–1,[4] indicating it is a chemically peculiar G-type main sequence star showing an under-abundance of iron and the molecule CH in its spectrum. As of 2008, it has an angular separation of 1.325 arcseconds along a position angle of 30.9° from the primary.[14]

This system is coeval with the Castor Moving Group of stars that share a common motion through space; hence it is a candidate member of that association. This suggests that the system is young; its estimated age is in the range of 180 to 370 million years, based upon the spectrum and X-ray luminosity, respectively.[10]

References

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Template:Stars of Aquarius