So what we need is something analogous, at least those low-resolution maps that I just showed you, to be able to tell whether there's overlap between where the hydrogen cyanide is and where these planets can access it as they are forming.
Necesitamos algo análogo, al menos a esos mapas de baja resolución que acabo de mostrarles para poder saber si hay superposición entre donde está el cianuro de hidrógeno y las zonas de acceso al mismo durante la formación del planeta.