5 Aquilae
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aquila |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | 5.90[2] (5.92/7.65)[3] |
| Characteristics | |
| Spectral type | A2 Vm + ? + F3 Vm[3][4] |
| U−B Template:Engvar | +0.12[2] |
| B−V Template:Engvar | +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 mas[1] |
| Distance | approx. Template:Rnd ly (approx. Template:Rnd pc) |
| Orbit[6] | |
| Primary | 5 Aql Aa |
| Companion | 5 Aql Ab |
| Period (P) | Script error: No such module "val". yr |
| Semi-major axis (a) | Script error: No such module "val".″ |
| Eccentricity (e) | Script error: No such module "val". |
| Inclination (i) | Script error: No such module "val".° |
| Longitude of the node (Ω) | Script error: No such module "val".° |
| Periastron epoch (T) | Script error: No such module "val". |
| Argument of periastron (ω) (secondary) | Script error: No such module "val".° |
| Details | |
| Rotational velocity (v sin i) | 71[7] km/s |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| BD−01 3559, HD 173654, HR 7059, WDS 18465-0058[8][9] | |
| 5 Aql A: HIP 92117, SAO 142606[8] | |
| 5 Aql B: HIP 92118, SAO 142607[9] | |
| Database references | |
| SIMBAD | 5 Aql |
| 5 Aql A | |
| 5 Aql B | |
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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 Script error: No such module "convert"., 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
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- ↑ a b Script error: No such module "citation/CS1". Preliminary orbit.
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- ↑ a b Template:Cite simbad
- ↑ a b Template:Cite simbad
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