TY Coronae Australis
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Corona Australis |
| Right ascension | 19h 01m 40.83122s |
| Declination | −36° 52′ 33.8018″ |
| Apparent magnitude (V) | 9.39 |
| Characteristics | |
| Spectral type | B9e |
| Astrometry | |
| Proper motion (μ) | RA: −2.147 ± 0.239 mas/yr Dec.: −32.723 ± 0.226 mas/yr |
| Parallax (π) | 7.3290±0.1456 mas |
| Distance | 445 ± 9 ly (136 ± 3 pc) |
| Details | |
| Other designations | |
| TY CrA, SAO 210829, CD−37° 13024 | |
| Database references | |
| SIMBAD | data |
TY Coronae Australis (abbreviated as TY CrA), is a young star system around 3 million years old in the constellation Corona Australis. It is composed of a blue-white B-class star around triple the Sun's mass and a cooler smaller companion around half its mass (or 1.6 times that of the Sun). The system is an eclipsing binary with a period of 2.8 days.
Robert T. A. Innes announced his discovery that the star is a variable star, in 1916.