A Spectroscopically Unique Main Belt Asteroid: 10537 (1991 RY16)
  We present visible and near-infrared reflectance spectra and interpreted surface mineralogy for asteroid 10537 (1991 RY16). The spectrum of this object is without precedent amongst the Main Belt asteroids. A unique absorption band centered at 0.63 microns could be attributed to one of several mineralogies. Pronounced 1- and 2-micron absorption bands suggest that the composition of 10537 is a mixture of pyroxenes and olivine and that it originated from a parent body that was partially or fully differentiated. The closest available analog is the large Main Belt asteroid 349 Dembowska but 10537 may be an isolated fragment from a completely eroded parent body. 
Nicholas A. Moskovitz (1), Samuel Lawrence (2), Robert Jedicke (1),   Mark Willman (1), Nader Haghighipour (1 and 3), Schelt...