Hertzsprung-Russel diagram with Siess et al. (2000) evolutionary tracks from 0.2 to 0.8 M_⊙ (dashed lines). Isochrones corresponding to 1, 2, 3, 4, 5, and 10 Myr (solid lines) are also represented. The circle corresponds to the value determined in this work and the square to the value of Hillenbrand (1997), rescaled to the distance derived from the Gaia DR2 parallax. The cyan star represents the value for JW180 assuming a distance of 414 ± 7 pc.