Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Tucana |
Right ascension | 00h 55m 00.31129s[1] |
Declination | −69° 31′ 37.5025″[1] |
Apparent magnitude (V) | +5.45[2] |
Characteristics | |
Spectral type | K2 III[3] |
B−V color index | +1.10[2] |
Astrometry | |
Radial velocity (Rv) | +5.1±2.8[4] km/s |
Proper motion (μ) | RA: +6.842[1] mas/yr Dec.: −43.735[1] mas/yr |
Parallax (π) | 14.6214 ± 0.0817 mas[1] |
Distance | 223 ± 1 ly (68.4 ± 0.4 pc) |
Absolute magnitude (MV) | +1.29[5] |
Details[2] | |
Mass | 1.75 M☉ |
Radius | 9.84+0.22 −0.42[1] R☉ |
Luminosity | 39.2±0.3[1] L☉ |
Surface gravity (log g) | 2.74 cgs |
Temperature | 4,605+101 −52[1] K |
Metallicity [Fe/H] | −0.07±0.14 dex |
Rotational velocity (v sin i) | 3.14 km/s |
Other designations | |
Database references | |
SIMBAD | data |
Lambda2 Tucanae is a solitary[7] star in the southern constellation of Tucana. It is faintly visible to the naked eye with an apparent visual magnitude of +5.45.[2] Based upon an annual parallax shift of 14.6 mas as seen from Earth, it is located around 223 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.09 due to interstellar dust.[2]
This is an orange-hued K-type giant star on the red giant branch,[2] with a stellar classification of K2 III.[3] It has an estimated 1.75[2] times the mass of the Sun but after evolving away from the main sequence it has expanded to 9.8 times the Sun's radius. The star is radiating 39 times the solar luminosity from its photosphere at an effective temperature of 4,605 K.[1]
GaiaDR2
was invoked but never defined (see the help page).Jones2011
was invoked but never defined (see the help page).houk1979
was invoked but never defined (see the help page).deBruijne2012
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).