WASP-121

WASP-121 / Dilmun
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Puppis
Right ascension 07h 10m 24.06046s
Declination −39° 05 50.5712
Apparent magnitude (V) 10.4
Characteristics
Evolutionary stage main sequence
Spectral type F6V
Apparent magnitude (B) 11.00
Apparent magnitude (V) 10.51
Apparent magnitude (J) 9.625
Apparent magnitude (H) 9.439
Apparent magnitude (K) 9.374
Astrometry
Radial velocity (Rv)38.25±0.22 km/s
Proper motion (μ) RA: −3.735 mas/yr
Dec.: 25.663 mas/yr
Parallax (π)3.7996±0.0104 mas
Distance858 ± 2 ly
(263.2 ± 0.7 pc)
Details
Mass1.330±0.019 M
Radius1.461±0.015 R
Surface gravity (log g)4.251±0.003 cgs
Temperature6,628±66 K
Metallicity [Fe/H]+0.17±0.05 dex
Rotational velocity (v sin i)11.90±0.31 km/s
Age1.11±0.14 Gyr
Other designations
Dilmun, CD−38 3220, TOI-495, WASP-121, TYC 7630-352-1, 2MASS J07102406-3905506
Database references
SIMBADdata

WASP-121, also known as CD-38 3220 and formally named Dilmun, is a magnitude 10.4 star located approximately 858 light-years (263 parsecs) away in the constellation Puppis. WASP-121 has a mass and radius similar to the Sun's. It hosts one known exoplanet.

The star, although metal-rich in terms of overall contents of heavy elements, is depleted of carbon. The carbon to oxygen molar ratio of 0.23±0.05 for WASP-121 is well below the solar ratio of 0.55.