53 Aquarii

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53 Aquarii
Diagram showing star positions and boundaries of the Aquarius constellation and its surroundings
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Location of 53 Aquarii (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 22h 26m 34.2753s[1]
Declination –16° 44′ 31.697″[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 color index +0.09[2]
B−V color index +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[1] mas
Distance 66 ± 2 ly
(20.2 ± 0.5 pc)
Absolute magnitude (MV) 4.05[5] (4.94/4.87)[3]
Details
53 Aqr A
Mass 0.99[6] M
Radius 1.11[6] R
Luminosity 1.39[6] L
Surface gravity (log g) 4.46[3] cgs
Temperature 5,922[3] K
Metallicity [Fe/H] –0.10[3] dex
Rotational velocity (v sin i) 8[7] km/s
Age 0.18–0.37[8] Gyr
53 Aqr B
Surface gravity (log g) 4.44[3] cgs
Temperature 5,811[3] K
Metallicity [Fe/H] –0.19[3] dex
Rotational velocity (v sin i) 9[7] km/s
Other designations
GJ 859, HIP 110778.[9]
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.

53 Aquarii (abbreviated 53 Aqr) is a binary star[10] 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 65 light-years (20 parsecs) 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.[6] 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.[6] 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.[11] 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.[6]

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.[12]

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.[8]

References

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