The UV/blue effects of space weathering manifested in S-complex asteroids II: Probing for less-weathered objects in the Solar System
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[1] F. Vilas,et al. THE UV/BLUE EFFECTS OF SPACE WEATHERING MANIFESTED IN S-COMPLEX ASTEROIDS. I. QUANTIFYING CHANGE WITH ASTEROID AGE , 2015 .
[2] D. Britt,et al. Space weathering simulations through controlled growth of iron nanoparticles on olivine , 2014, 1404.2956.
[3] A. Tsuchiyama,et al. Space weathered rims found on the surfaces of the Itokawa dust particles , 2014 .
[4] T. Hashimoto,et al. Incipient Space Weathering Observed on the Surface of Itokawa Dust Particles , 2011, Science.
[5] P. H. Hasselmann,et al. SDSS-based taxonomic classification and orbital distribution of main belt asteroids , 2010 .
[6] C. Dukes,et al. Irradiation of olivine by 4 keV He+: Simulation of space weathering by the solar wind , 2009 .
[7] Paul A. Abell,et al. Mineralogical composition of (25143) Itokawa 1998 SF36 from visible and near‐infrared reflectance spectroscopy: Evidence for partial melting , 2007 .
[8] F. Vilas,et al. The Effects of Space Weathering at UV Wavelengths: S-Class Asteroids , 2006 .
[9] D. Gandolfi,et al. Space weathering of near-Earth and main belt silicate-rich asteroids: observations and ion irradiation experiments , 2005 .
[10] Robert Jedicke,et al. An age–colour relationship for main-belt S-complex asteroids , 2004, Nature.
[11] Bruce Hapke,et al. Space weathering from Mercury to the asteroid belt , 2001 .
[12] Clark R. Chapman,et al. S-Type Asteroids, Ordinary Chondrites, and Space Weathering: The Evidence from Galileo's Fly-bys of Gaspra and Ida , 1996 .
[13] M. Skrutskie,et al. Discovery of a Main-Belt Asteroid Resembling Ordinary Chondrite Meteorites , 1993, Science.
[14] Carle M. Pieters,et al. Optical effects of space weathering: The role of the finest fraction , 1993 .
[15] Robert Jedicke,et al. Evidence for asteroid space weathering from the Sloan Digital Sky Survey , 2005 .
[16] Bruce Hapke,et al. Atlas of reflectance spectra of terrestrial, lunar, and meteoritic powders and frosts from 92 to 1800 nm , 1987 .