L 168-9
L 168-9 (also known as GJ 4332 or TOI-134, officially named Danfeng) is a red dwarf star located  away from the Solar System in the constellation of Tucana. The star has about 62% the mass and 60% the radius of the Sun. It has a temperature of  and a rotation period of 29.8 days. L 168-9 is orbited by one known exoplanet. Nomenclature
The designation L 168-9 comes from Luyten's first catalogue of stars with high proper motion. 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 China, were announced in June 2023. L 168-9 is named Danfeng and its planet is named Qingluan, after mythological birds of ancient China. Planetary system 

The exoplanet L 168-9 b, officially named Qingluan, was discovered in 2020 using TESS. It is a terrestrial super-Earth with about 4.6 times the mass and 1.39 times the radius of Earth, and an estimated equilibrium temperature of . L 168-9 b is a target for observation and atmospheric characterization with the James Webb Space Telescope, and has been observed as one of its first targets. References 

Tucana (constellation)
M-type main-sequence stars
Planetary systems with one confirmed planet
CD-60 08051
4332
115211
0134
Danfeng