An article published in the journal “Astronomy & Astrophysics” reports the confirmation of the presence of 5 rocky planets in the HD 23472 star system. A team of researchers used the Espresso spectrograph on ESO’s VLT to examine these exoplanets to estimate their masses using the radial velocity method. Their sizes were already known thanks to the data collected by NASA’s TESS space telescope, which observed their transit in front of their star. The result of the examination is that three of those exoplanets are super-Earths and two are probably super-Mercuries, rare cases characterized by a larger iron core and in general a high percentage of iron.