WASP-69

WASP-69 / Wouri
Observation data
Epoch J2000      Equinox ICRS
Constellation Aquarius
Right ascension 21h 00m 06.19682s
Declination −05° 05′ 40.0349″
Apparent magnitude (V) 9.87±0.03
Characteristics
Evolutionary stage main sequence
Spectral type K5V
Astrometry
Radial velocity (Rv)−9.83±0.13 km/s
Proper motion (μ) RA: 33.778 mas/yr
Dec.: −93.581 mas/yr
Parallax (π)19.8858±0.0170 mas
Distance164.0 ± 0.1 ly
(50.29 ± 0.04 pc)
Details
Mass0.826±0.029 M☉
Radius0.813 R☉
Luminosity0.34 L☉
Surface gravity (log g)4.59±0.02 cgs
Temperature4,782±15 K
Metallicity [Fe/H]0.10±0.01 dex
Rotation23.07 d
Rotational velocity (v sin i)1.27±0.22 km/s
Age2 Gyr
Other designations
Wouri, BD−05 5432, TOI-5823, TIC 248853232, WASP-69, TYC 5200-1560-1, GSC 05200-01560, 2MASS J21000618-0505398
Database references
SIMBADdata
Exoplanet Archivedata

WASP-69, also named Wouri, is a K-type main-sequence star 164 light-years (50 parsecs) away from Earth in the constellation Aquarius. Its surface temperature is 4782±15 K. WASP-69 is slightly enriched in heavy elements compared to the Sun, with a metallicity Fe/H index of 0.10±0.01, and is much younger than the Sun at 2 billion years. The data regarding starspot activity of WASP-69 are inconclusive, but spot coverage of the photosphere may be very high.

Multiplicity surveys did not detect any stellar companions to WASP-69 as of 2020.

Nomenclature

The designation WASP-69 indicates that this was the 69th star found to have a planet by the Wide Angle Search for Planets.

In August 2022, this planetary system was included among 20 systems to be named by the third NameExoWorlds project. The approved names, proposed by a team from Cameroon, were announced in June 2023. WASP-69 is named Wouri and its planet is named Makombé, after the Wouri and Makombé rivers in Cameroon.

Planetary system

In 2013, one planet, named WASP-69b, was discovered on a tight, circular orbit. Its equilibrium temperature is 886 K, but the measured terminator temperature is significantly higher by at least 200 K. The planet is losing mass at a moderate rate of 0.5 M🜨 per billion years, producing a tail detected in 2024 and measured to be at least 7 times its own radius.

The planetary atmosphere is extremely hazy and contains a partial cloud deck with cloud tops rising to a pressure of 100 Pa. Its composition is mostly hydrogen and helium, and sodium was also detected in low concentration. The sodium may originate from volcanic moons, not from the planet itself.

By 2021, the presence of hazes in atmosphere of WASP-69b was confirmed, along with a solar or super-solar water abundance.

The WASP-69 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination
(°)
Radius
b / Makombé 0.260±0.017 MJ 0.04525±0.00053 3.8681382±0.0000017 0 86.71±0.20 0.945+0.007
−0.017
 RJ