5 Aquilae
| Observation data Epoch J2000 Equinox J2000 |
|
|---|---|
| Constellation | Aquila |
| Right ascension | 18h 46m 28.58278s[1] |
| Declination | –00° 57′ 41.9006″[1] |
| Apparent magnitude (V) | 5.90[2] (5.92/7.65)[3] |
| Characteristics | |
| Spectral type | A2 Vm + ? + F3 Vm[3][4] |
| U−B color index | +0.12[2] |
| B−V color index | +0.131[1] |
| Astrometry | |
| Radial velocity (Rv) | +17.4[5] km/s |
| Proper motion (μ) | RA: +20.44[1] mas/yr Dec.: –21.54[1] mas/yr |
| Parallax (π) | 8.94 ± 1.14[1] mas |
| Distance | approx. 360 ly (approx. 110 pc) |
| Orbit[6] | |
| Primary | 5 Aql Aa |
| Companion | 5 Aql Ab |
| Period (P) | 33.65 ± 0.78 yr |
| Semi-major axis (a) | 0.219 ± 0.016" |
| Eccentricity (e) | 0.333 ± 0.054 |
| Inclination (i) | 97.9 ± 1.4° |
| Longitude of the node (Ω) | 174.3 ± 1.9° |
| Periastron epoch (T) | 1989.71 ± 0.76 |
| Argument of periastron (ω) (secondary) |
251.7 ± 5.9° |
| Details | |
| Rotational velocity (v sin i) | 71[7] km/s |
| Other designations | |
| 5 Aql A: HIP 92117, SAO 142606.[8] | |
| 5 Aql B: HIP 92118, SAO 142607.[9] | |
5 Aquilae (abbreviated 5 Aql) is a quadruple star[3] system in the constellation of Aquila. 5 Aquilae is the Flamsteed designation. The combined apparent visual magnitude of the system is 5.9,[2] which means it is faintly visible to the naked eye. With an annual parallax shift of 8.94 mas,[1] the distance to this system is estimated as approximately 360 light-years (110 parsecs), albeit with a 13% margin of error.
Two of the components of this system, 5 Aquilae Aa and Ab, are Am stars. That is, they are chemically peculiar stars that show unusual abundances of elements other than hydrogen and helium. The two orbit each other with a period lasting 33.65 years at an eccentricity of 0.33. One of these stars is itself a close spectroscopic binary, with a 4.765 day period and a nearly circular orbit that has an eccentricity of just 0.02.[6] The fourth component, 5 Aquilae B, is a magnitude 7.65 F-type main sequence star with a stellar classification of F3 Vm. It is at an angular separation of 12.71 arcseconds from the other members of the system.[3]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 2.2 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 3.0 3.1 3.2 3.3 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.
- ↑ 6.0 6.1 Lua error in package.lua at line 80: module 'strict' not found. Preliminary orbit.
- ↑ 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.
- ↑ 9.0 9.1 Lua error in package.lua at line 80: module 'strict' not found.
