Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquila |
Right ascension | 18h 55m 27.46151s [1] |
Declination | +06° 36′ 55.1499″ [1] |
Apparent magnitude (V) | 5.57 [2] |
Characteristics | |
Spectral type | G9 III [3] |
U−B color index | +0.87 [2] |
B−V color index | +1.041±0.002 [4] |
Astrometry | |
Radial velocity (Rv) | 23.31±0.09 [5] km/s |
Proper motion (μ) |
RA: +7.972
[1]
mas/
yr Dec.: –92.211 [1] mas/ yr |
Parallax (π) | 11.5405 ± 0.1636 mas [1] |
Distance | 283 ± 4
ly (87 ± 1 pc) |
Absolute magnitude (MV) | 0.87 [4] |
Orbit [5] [6] | |
Primary | HR 7135 A |
Companion | HR 7135 B |
Period (P) | 2,994±29 d |
Semi-major axis (a) | 26.6±3.4 mas |
Eccentricity (e) | 0.243±0.026 |
Inclination (i) | 31.9±3.6° |
Longitude of the node (Ω) | 12.6±7.7° |
Periastron epoch (T) | 2444276.5±52 JD |
Argument of periastron (ω) (secondary) | 35±7° |
Semi-amplitude (K1) (primary) | 4.65±0.13 km/s |
Details | |
HR 7135 A | |
Mass | 1.54 [7] M☉ |
Radius | 10.69+0.17 −0.93 [1] R☉ |
Luminosity | 52.8±0.9 [1] L☉ |
Surface gravity (log g) | 2.7 [8] cgs |
Temperature | 4,666±51 [7] K |
Metallicity [Fe/H] | –0.26 [8] dex |
Rotational velocity (v sin i) | 0.0 [8] km/s |
Age | 3.21 [7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HR 7135 is a binary star system. Despite its Flamsteed designation of 62 Serpentis, the star can be found in the equatorial constellation of Aquila, [10] in front of a dark rift in the Milky Way near the constellation border. [5] It is visible to the naked eye as a dim, yellow-hued point of light with an apparent visual magnitude of 5.57. [2] The system is located 283 light years distant from the Sun, based on parallax, [1] and is drifting further away with a radial velocity of 23 km/s. [5]
Discovery of the binary nature of this system is credited to Canadian astronomer H. H. Plaskett in 1922. It is a single-lined spectroscopic binary with an orbital period of 8.2 years and an eccentricity of 0.24. [5] [6] The visible component is an aging giant star with a stellar classification of G9 III, [3] having exhausted the supply of hydrogen at its core and expanded to 10.7 [1] times the Sun's radius. It is a red clump giant, indicating it is on the horizontal branch and is generating energy via core helium fusion. [11] The star is 3.2 [7] billion years old with 1.54 [7] times the mass of the Sun. It is radiating 53 [1] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,666 K. [7] The star has a very low rate of spin, with the projected rotational velocity being too small to measure. [8]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquila |
Right ascension | 18h 55m 27.46151s [1] |
Declination | +06° 36′ 55.1499″ [1] |
Apparent magnitude (V) | 5.57 [2] |
Characteristics | |
Spectral type | G9 III [3] |
U−B color index | +0.87 [2] |
B−V color index | +1.041±0.002 [4] |
Astrometry | |
Radial velocity (Rv) | 23.31±0.09 [5] km/s |
Proper motion (μ) |
RA: +7.972
[1]
mas/
yr Dec.: –92.211 [1] mas/ yr |
Parallax (π) | 11.5405 ± 0.1636 mas [1] |
Distance | 283 ± 4
ly (87 ± 1 pc) |
Absolute magnitude (MV) | 0.87 [4] |
Orbit [5] [6] | |
Primary | HR 7135 A |
Companion | HR 7135 B |
Period (P) | 2,994±29 d |
Semi-major axis (a) | 26.6±3.4 mas |
Eccentricity (e) | 0.243±0.026 |
Inclination (i) | 31.9±3.6° |
Longitude of the node (Ω) | 12.6±7.7° |
Periastron epoch (T) | 2444276.5±52 JD |
Argument of periastron (ω) (secondary) | 35±7° |
Semi-amplitude (K1) (primary) | 4.65±0.13 km/s |
Details | |
HR 7135 A | |
Mass | 1.54 [7] M☉ |
Radius | 10.69+0.17 −0.93 [1] R☉ |
Luminosity | 52.8±0.9 [1] L☉ |
Surface gravity (log g) | 2.7 [8] cgs |
Temperature | 4,666±51 [7] K |
Metallicity [Fe/H] | –0.26 [8] dex |
Rotational velocity (v sin i) | 0.0 [8] km/s |
Age | 3.21 [7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HR 7135 is a binary star system. Despite its Flamsteed designation of 62 Serpentis, the star can be found in the equatorial constellation of Aquila, [10] in front of a dark rift in the Milky Way near the constellation border. [5] It is visible to the naked eye as a dim, yellow-hued point of light with an apparent visual magnitude of 5.57. [2] The system is located 283 light years distant from the Sun, based on parallax, [1] and is drifting further away with a radial velocity of 23 km/s. [5]
Discovery of the binary nature of this system is credited to Canadian astronomer H. H. Plaskett in 1922. It is a single-lined spectroscopic binary with an orbital period of 8.2 years and an eccentricity of 0.24. [5] [6] The visible component is an aging giant star with a stellar classification of G9 III, [3] having exhausted the supply of hydrogen at its core and expanded to 10.7 [1] times the Sun's radius. It is a red clump giant, indicating it is on the horizontal branch and is generating energy via core helium fusion. [11] The star is 3.2 [7] billion years old with 1.54 [7] times the mass of the Sun. It is radiating 53 [1] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,666 K. [7] The star has a very low rate of spin, with the projected rotational velocity being too small to measure. [8]