Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Grus |
Right ascension | 22h 56m 47.80007s[1] |
Declination | −47° 58′ 09.1992″[1] |
Apparent magnitude (V) | 5.71[2] |
Characteristics | |
Spectral type | kA5hA7mF2[3] |
U−B color index | +0.17[2] |
B−V color index | +0.22[2] |
Astrometry | |
Radial velocity (Rv) | 6.3±0.6[4] km/s |
Proper motion (μ) | RA: −24.942[1] mas/yr Dec.: +2.848[1] mas/yr |
Parallax (π) | 12.3180 ± 0.1170 mas[1] |
Distance | 265 ± 3 ly (81.2 ± 0.8 pc) |
Absolute magnitude (MV) | +1.36[5] |
Details | |
Radius | 2.88+0.13 −0.18[1] R☉ |
Luminosity | 26.8+0.3 −0.3[1] L☉ |
Temperature | 7,735+406 −158[1] K |
Other designations | |
Database references | |
SIMBAD | data |
Tau3 Gruis is a solitary[7] star in the southern constellation of Grus. Its apparent magnitude is 5.71,[2] which is bright enough to be visible to the naked eye as a dim, white-hued star. The star is located around 265 light-years (81 pc) distant from the Sun based on parallax, and it is drifting further away with a radial velocity of 6 km/s.[4]
This is an Am star[8] with a stellar classification of kA5hA7mF2.[3] This notation indicates the spectrum displays the calcium K-line of an A5 star, the hydrogen lines of an A7 star, and the metal lines of an F2 star.[9] It has 2.9[1] times the Sun's radius and is radiating 27[1] times the luminosity of the Sun from its photosphere at an effective temperature of around 7,735 K.[1]
GaiaDR2
was invoked but never defined (see the help page).feinstein1974
was invoked but never defined (see the help page).abt1995
was invoked but never defined (see the help page).Gontcharov2006
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Eggleton2008
was invoked but never defined (see the help page).Renson2009
was invoked but never defined (see the help page).gray2009
was invoked but never defined (see the help page).