701 Oriola /ɒrˈrələ/ is a main belt asteroid. This C-type asteroid shows possible broad absorption which may be explained by either magnesium-rich amorphous pyroxene or crystalline silicate. This likely accounts for the relatively high albedo as an outer-belt asteroid.[2]

References

  1. ^ a b c d e f g h "701 Oriola (A910 ND)". JPL Small-Body Database (2020-06-16 last obs). NASA/Jet Propulsion Laboratory. Retrieved 24 July 2020.
  2. ^ Kasuga, Toshihiro; et al. (February 2015), "Near-Infrared Spectra of High-Albedo Outer Main-Belt Asteroids", The Astronomical Journal, 149 (2): 8, Bibcode:2015AJ....149...37K, doi:10.1088/0004-6256/149/2/37, 37.


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