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We have performed spectrophotometry of (32) Pomona, (704) Interamnia, (779) Nina, (330825) 2008 ХЕ3, and 2012 QG42 accessible for observation in September 2012 including two NEAs, one of which is PHA, to study absorption features in their reflectance spectra with the aim to get new mineralogical information on the surface matter and its correspondence to a spectral type. The obtained results could be useful in investigations of Moon and other atmosphereless bodies at identification of residues of fallen asteroids.