Tau Piscis Austrini
Star in the constellation Piscis Austrinus / From Wikipedia, the free encyclopedia
Tau Piscis Austrini (τ Piscis Austrini) is a solitary,[9] yellow-white hued star in the southern constellation of Piscis Austrinus. It is visible to the naked eye with an apparent visual magnitude of +4.9.[2] Based upon an annual parallax shift of 54.71 mas as seen from the Earth,[1] the star is located 59.6 light years from the Sun.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Piscis Austrinus |
Right ascension | 22h 10m 08.78048s[1] |
Declination | −32° 32′ 54.2687″[1] |
Apparent magnitude (V) | +4.945[2] |
Characteristics | |
Spectral type | F6 V[3] |
U−B color index | +0.031[2] |
B−V color index | +0.488[2] |
Astrometry | |
Proper motion (μ) | RA: +428.96[1] mas/yr Dec.: +13.35[1] mas/yr |
Parallax (π) | 54.71 ± 0.28 mas[1] |
Distance | 59.6 ± 0.3 ly (18.28 ± 0.09 pc) |
Absolute magnitude (MV) | 3.58[4] |
Details | |
Mass | 1.34±0.13[5] M☉ |
Radius | 1.45±0.04[5] R☉ |
Luminosity | 2.82±0.09[5] L☉ |
Surface gravity (log g) | 4.11[6] cgs |
Temperature | 6,324[4] K |
Metallicity [Fe/H] | −0.01[6] dex |
Rotational velocity (v sin i) | 14.1±0.7[4] km/s |
Age | 1.3[7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
This is an F-type main sequence star with a stellar classification of F6 V.[3] It is about 1.3[7] billion years old with a projected rotational velocity of 14[4] km/s and exhibits a low level of activity.[10] The star has an estimated 1.34 times the mass of the Sun and 1.45 times the Sun's radius.[5] It is radiating 2.82[5] times the solar luminosity from its photosphere at an effective temperature of 6,324 K.[4] This star is a candidate for hosting a debris disk, as it displayed an initial near infrared excess that faded with further observations.[11]