“…Interest in more mafic systems has been spurred by growing evidence for the presence of zircon grains in a wide range of terrestrial mafic and ultramafic rocks such as diorites, gabbros and gabbroids, peridotites, kimberlites, dunites, chromitites, garnet-pyroxenites, dolerites, and including spectacularly large grains of zircon in carbonatites (e.g., Bea et al 2001;Belousova et al 2002Belousova et al , 2015Kaczmarek et al 2008;Kostitsyn et al 2009Kostitsyn et al , 2012Kostitsyn et al , 2015González-Jiménez et al 2017;Bychkova et al 2019aBychkova et al , 2019bBea et al 2020 and references therein) as well as in basaltic meteorites (Ireland and Wlotzka 1992;Humayun et al 2013;Valley et al 2014b;Iizukaa et al 2015;Bellucci et al 2019). However, there is a current debate concerning the formation mechanisms of zircon in terrestrial mafic and ultramafic rocks that can reach 3.2 Ga in age.…”