WASP-21

WASP-21 / Tangra

Size comparison between Sun and WASP-21
Observation data
Epoch J2000      Equinox J2000
Constellation Pegasus
Right ascension 23h 09m 58.25s
Declination +18° 23 45.9
Apparent magnitude (V) 11.58±0.08
Characteristics
Evolutionary stage subgiant
Spectral type G3V
Astrometry
Radial velocity (Rv)−89.21±0.46 km/s
Proper motion (μ) RA: +17.567(21) mas/yr
Dec.: +18.639(18) mas/yr
Parallax (π)3.9089±0.0197 mas
Distance834 ± 4 ly
(256 ± 1 pc)
Absolute magnitude (MV)4.97
Details
Mass0.89±0.071 M
Radius1.136±0.049 R
Luminosity1.4 L
Surface gravity (log g)4.277±0.025 cgs
Temperature5,800±100 K
Metallicity−0.4±0.1
Metallicity [Fe/H]−0.46±0.11 dex
Rotational velocity (v sin i)1.5±0.6 km/s
Age12±5 Gyr
Other designations
Tangra, TOI-5963, TIC 436478932, WASP-21, GSC 01715-00679, 2MASS J23095825+1823459
Database references
SIMBADdata
Exoplanet Archivedata

WASP-21, also named Tangra, is a G-type star (spectral type G3V) that has reached the end of its main sequence lifetime. It lies approximately 834 light-years away, in the constellation of Pegasus. The star is relatively metal-poor, having 40% of heavy elements compared to the Sun. Kinematically, WASP-21 belongs to the thick disk of the Milky Way. It has an exoplanet named WASP-21b.

A survey in 2012 failed to find any stellar companions to WASP-21.