Observation data Epoch J2000.0[1] Equinox J2000.0[1] | |
---|---|
Constellation | Corona Australis |
Right ascension | 18h 12m 25.83474s |
Declination | −37° 45′ 09.2713″ |
Apparent magnitude (V) | 7.953[2] |
Characteristics | |
Spectral type | A5pSrCrEu[2] |
B−V color index | 0.42[3] |
J−H color index | -0.018[4] |
J−K color index | -0.026[4] |
Variable type | α2 CVn variable[2] |
Astrometry | |
Radial velocity (Rv) | −22.5±3.0 km/s |
Proper motion (μ) | RA: -2.767[1] mas/yr Dec.: −12.785[1] mas/yr |
Parallax (π) | 7.1672 ± 0.0337 mas[1] |
Distance | 455 ± 2 ly (139.5 ± 0.7 pc) |
Absolute magnitude (MV) | 1.60,[5] 2.197[6] |
Details[5] | |
Mass | 2.29 M☉ |
Radius | 2.25 R☉ |
Luminosity | 18.03 L☉, 9.811[6] L☉ |
Surface gravity (log g) | 4.00 cgs |
Temperature | 7760 K |
Rotation | 3836 ± 30 d |
Age | 1.00 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 166473 is a rapidly oscillating Ap star (roAp star) and an α2 CVn variable located about 455 light-years (140 parsecs) away in the southern constellation of Corona Australis. It has the variable star designation V694 Coronae Australis (sometimes abbreviated to V694 CrA). With an apparent magnitude of 7.953, it is too faint to be seen by the naked eye from Earth, but can be observed using binoculars.[7]
EDR3
was invoked but never defined (see the help page).Bychkov2021
was invoked but never defined (see the help page).TYC2000
was invoked but never defined (see the help page).simbad
was invoked but never defined (see the help page).Glagolevskij2019
was invoked but never defined (see the help page).Scholz2019
was invoked but never defined (see the help page).bino
was invoked but never defined (see the help page).