Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Lyra |
Right ascension | 19h 07m 18.13251s[2] |
Declination | +36° 06′ 00.5592″[2] |
Apparent magnitude (V) | 5.22[3] |
Characteristics | |
Spectral type | B6IV[4] |
Variable type | Be star[5] |
Astrometry | |
Radial velocity (Rv) | −26.0±4.6[6] km/s |
Proper motion (μ) | RA: −1.437[2] mas/yr Dec.: −3.876[2] mas/yr |
Parallax (π) | 3.5858 ± 0.1924 mas[2] |
Distance | 910 ± 50 ly (280 ± 10 pc) |
Absolute magnitude (MV) | −1.94[7] |
Orbit[8] | |
Period (P) | 216.93 yr |
Semi-major axis (a) | 0.172″ |
Eccentricity (e) | 0.637 |
Inclination (i) | 145.5° |
Longitude of the node (Ω) | 171.4° |
Periastron epoch (T) | B 1997.28 |
Argument of periastron (ω) (secondary) | 201.2° |
Details | |
Mass | 5.2[9] M☉ |
Radius | 6.7[10] R☉ |
Luminosity | 854[10] L☉ |
Surface gravity (log g) | 3.54[9] cgs |
Temperature | 12,059[10] K |
Metallicity [Fe/H] | −0.11[9] dex |
Rotational velocity (v sin i) | 224[11] km/s |
Age | 168[12] Myr |
Other designations | |
Database references | |
SIMBAD | data |
ι Lyrae, Latinised as Iota Lyrae, is a binary star[3] in the northern constellation of Lyra. It is visible to the naked eye as a dim, blue-white hued star with an apparent visual magnitude that fluctuates around 5.22.[3] This object is located approximately 910 light years distant from the Sun based on parallax, but is drifting nearer with a radial velocity of −26 km/s.[6]
This is a wide binary system with a computed orbital period of 217 years and an eccentricity of 0.6.[8] The primary component has a stellar classification of B6IV,[4] matching a B-type subgiant star. It is a Be star,[14] displaying emission lines in its spectrum, and is spinning rapidly with a projected rotational velocity of 224 km/s.[11] The star ranges in brightness from magnitude 5.20 down to 5.27.[5] It has about five times the mass of the Sun and is radiating 854 times the Sun's luminosity from its photosphere at an effective temperature of 12,059 K.
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