HD 180450
Star in the constellation Lyra From Wikipedia, the free encyclopedia
Star in the constellation Lyra From Wikipedia, the free encyclopedia
HD 180450 is a single[4] star in the northern constellation of Lyra, positioned about half a degree to the NNW of the globular cluster M56.[5] At an apparent visual magnitude of 5.88,[2] it is dimly visible to the naked eye under good viewing conditions. This star is located at a distance of approximately 1,400 light years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of −64.4 km/s.[1]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Lyra |
Right ascension | 19h 15m 24.85937s[1] |
Declination | +30° 31′ 34.9760″[1] |
Apparent magnitude (V) | 5.88[2] |
Characteristics | |
Spectral type | M1IIIab[2] |
U−B color index | +2.03 |
B−V color index | +1.665±0.007[2] |
Astrometry | |
Radial velocity (Rv) | −64.43±0.23[1] km/s |
Proper motion (μ) | RA: 34.425[1] mas/yr Dec.: −26.081[1] mas/yr |
Parallax (π) | 2.37 ± 0.61 mas[1] |
Distance | approx. 1,400 ly (approx. 400 pc) |
Absolute magnitude (MV) | −2.03[2] |
Details | |
Radius | 68+12 −13[1] R☉ |
Luminosity | 1,002±34[1] L☉ |
Temperature | 3,947+433 −305[1] K |
Other designations | |
Database references | |
SIMBAD | data |
This is an aging red giant star with a stellar classification of M1IIIab,[2] It is currently on the asymptotic giant branch,[6] having exhausted the supply of hydrogen in its core and evolved of the main sequence. It has expanded to ~68 times the radius of the Sun and is radiating a thousand times the Sun' luminosity from its enlarged photosphere at en effective temperature of 3,947 K.[1]
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