53 Aquarii
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 | |
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
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 2.2 2.3 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 3.8 3.9 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 4.0 4.1 4.2 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 5.0 5.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 6.0 6.1 6.2 6.3 6.4 6.5 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 7.0 7.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 8.0 8.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found. See also the children entries.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.