Summary of distance measurements in the literature for the Pleiades open cluster obtained from different methods. The results presented here come from: (i) moving cluster – this work (see Sect. 5.1), Röser & Schilbach (2013), Narayanan & Gould (1999); (ii) trigonometric parallax – van Leeuwen (1999), van Leeuwen (2009), Melis et al. (2014), Soderblom et al. (2005), Gatewood et al. (2000), TGAS (Gaia Collaboration 2016) – using result reported in this work (see Sect. 6.2); (iii) orbital modeling – Groenewegen et al. (2007), Southworth et al. (2005), Zwahlen et al. (2004), Munari et al. (2004), Pan et al. (2004), David et al. (2016); (iv) twin stars- Mädler et al. (2016), (v) MS and isochrone fitting – An et al. (2007), Percival et al. (2005), Stello & Nissen (2001), Pinsonneault et al. (1998), Giannuzzi (1995) and Nicolet (1981).