Observation data Epoch J2000.0 Equinox J2000.0 |
|
---|---|
Constellation | Lyra |
Right ascension | 18 h 53 m 43.5596 s/18 h 5 3m 48.4506 s |
Declination | +36° 58' 18.196"/+37° 01' 03.755" |
Apparent magnitude (V) | 5.569/9.8 |
Characteristics | |
Spectral type | B2.5V/K2III |
U−B color index | −0.67/+1.288 |
B−V color index | −0.15/+1.224 |
Astrometry | |
Radial velocity (Rv) | −25.8/−49.0 km/s |
Proper motion (μ) | RA: 1.49/3.70 mas/yr Dec.: −2.60/10.20 mas/yr |
Parallax (π) | 3.02 ± 0.56 mas |
Distance | approx. 1100 ly (approx. 330 pc) |
Orbit[3], p. 412 | |
Period (P) | 88.352 days yr |
Eccentricity (e) | 0.37±0.03 |
Argument of periastron (ω) (secondary) |
204.5±7.7° |
Other designations | |
Delta1 Lyrae (δ1 Lyr) is a binary star system in the constellation Lyra, approximately 1,100 light years away from Earth. The two stars complete an orbit around each other about once every 88 days. They are a spectroscopic binary, meaning the separation between the two is very small, and their orbital velocity is very high.[1][3]
The main star, IDS 18502+3650 A, is a bluish white star of the spectral type B2.5V, meaning it has a surface temperature of 11,000 to 25,000 kelvins. It is a dwarf star, like our Sun, but more than twice as hot in surface temperature and many times brighter.[1]
Its 10th magnitude companion, IDS 18502+3650 B, is an orange giant star with the spectral type K2III. It therefore possesses a surface temperature of 3,500 to 5,000 kelvins and is cooler than our Sun, yet larger and brighter.[2]
|