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We show that the open cluster Trumpler 20, contrary to the earlier findings, is actually an old Galactic open cluster. New CCD photometry and high‐resolution spectroscopy are used to derive the main parameters of this cluster. At [Fe/H]=−0.11 for a single red giant star, the metallicity is slightly subsolar. The best fit to the colour–magnitude diagrams is achieved using a 1.3‐Gyr isochrone with convective overshoot. The cluster appears to have a significant reddening at   E ( B − V ) = 0.46  (for B0 spectral type), although for red giants this high reddening yields the colour temperature exceeding the spectroscopic  T  eff  by about 200 K. Trumpler 20 is a very rich open cluster, containing at least 700 members brighter than   M   V  =+4 . It may extend over the field of view available in our study at  20 × 20  arcmin 2 .

Trumpler 20 – an old and rich open cluster ★ †‡