  Using high dispersion high quality spectra of HD 30963 obtained with the
echelle spectrograph SOPHIE at Observatoire de Haute Provence in November 2015,
we show that this star, hitherto classified as a B9 III superficially normal
star, is actually a new Chemically Peculiar star of the HgMn type. Spectrum
synthesis reveals large overabundances of Mn, Sr, Y, Zr , Pt and Hg and
pronounced underabundances of He and Ni which are characteristic of HgMn stars.
We therefore propose that this interesting object be reclassified as a B9 HgMn
star.
