Comparison of the spectra of HIP 10725 (circles) and the Sun (solid line). In the top panel, we focus on two BeII features in the UV region around 3130 Å. HIP 10725 shows extreme Be depletion compared to the Sun, which is not expected for solar analogues (Tucci Maia et al. 2015). The bottom panel shows an enhancement of the neutron-capture element Nd in HIP 10725 as well as a substantially lower iron content relative to the Sun.