17 Lyrae
From Wikipedia, the free encyclopedia
Observation data Epoch J2000.0 |
|
---|---|
Constellation (pronunciation) |
Lyra |
Right ascension | 19h 7m 25.5807s / 19h 7m 24.8s |
Declination | +32° 30' 6.258" / +32° 30' 6" |
Apparent magnitude (V) | 5.229 / 9.1 |
Characteristics | |
Spectral type | F0V / ? |
U-B color index | +0.05 / ? |
B-V color index | +0.38 / ? |
Astrometry | |
Radial velocity (Rv) | 4.0 / -12.88 km/s |
Proper motion (μ) | RA: 123.23 / ? mas/yr Dec.: 32.08 / ? mas/yr |
Parallax (π) | 24.64 ± 0.54 mas |
Distance | 132 ± 3 ly (40.6 ± 0.9 pc) |
Other designations | |
Database references | |
SIMBAD | data |
17 Lyrae is a binary star system in the constellation Lyra, approximately 132 light years away from Earth. The main star, 17 Lyrae A, is a 5th magnitude white star of the spectral type F0V, meaning it has a surface temperature of about 7,500 kelvins. It is a dwarf star, like our Sun, yet brighter and hotter.[1] Its companion, 17 Lyrae B, is a 9th magnitude star of an unknown spectral type.[2] There was once thought to be a third star in the system, 17 Lyrae C, until it was evident that the star's parallax and proper motions were too different for it to be part of the system.[3]