Grevesse, NAsplund, MartinSauval, JScott, Pat2015-12-132100-014Xhttp://hdl.handle.net/1885/84400We show why the solar chemical composition of [1] (GN93) and the similar values of [2] (AG89) and [3] (GS98), characterized by values of the metallicity of the order of 0.017 to 0.020, largely used in solar and stellar modeling, are now obsolete. They sho201310.1051/epjconf/201343010042015-12-12