Bibcode
                                    
                            DellaGiustina, D. N.; Burke, K. N.; Walsh, K. J.; Smith, P. H.; Golish, D. R.; Bierhaus, E. B.; Ballouz, R. -L.; Becker, T. L.; Campins, H.; Tatsumi, E.; Yumoto, K.; Sugita, S.; Deshapriya, J. D. Prasanna; Cloutis, E. A.; Clark, B. E.; Hendrix, A. R.; Sen, A.; Al Asad, M. M.; Daly, M. G.; Applin, D. M.; Avdellidou, C.; Barucci, M. A.; Becker, K. J.; Bennett, C. A.; Bottke, W. F.; Brodbeck, J. I.; Connolly, H. C.; Delbo, M.; de Leon, J.; Drouet d'Aubigny, C. Y.; Edmundson, K. L.; Fornasier, S.; Hamilton, V. E.; Hasselmann, P. H.; Hergenrother, C. W.; Howell, E. S.; Jawin, E. R.; Kaplan, H. H.; Le Corre, L.; Lim, L. F.; Li, J. Y.; Michel, P.; Molaro, J. L.; Nolan, M. C.; Nolau, J.; Pajola, M.; Parkinson, A.; Popescu, M.; Porter, N. A.; Rizk, B.; Rizos, J. L.; Ryan, A. J.; Rozitis, B.; Shultz, N. K.; Simon, A. A.; Trang, D.; Van Auken, R. B.; Wolner, C. W. V.; Lauretta, D. S.
    Bibliographical reference
                                    Science
Advertised on:
    
                        11
            
                        2020
            
  Journal
                                    
                            Citations
                                    98
                            Refereed citations
                                    96
                            Description
                                    Visible-wavelength color and reflectance provide information about the geologic history of planetary surfaces. Here we present multispectral images (0.44 to 0.89 micrometers) of near-Earth asteroid (101955) Bennu. The surface has variable colors overlain on a moderately blue global terrain. Two primary boulder types are distinguishable by their reflectance and texture. Space weathering of Bennu surface materials does not simply progress from red to blue (or vice versa). Instead, freshly exposed, redder surfaces initially brighten in the near-ultraviolet region (i.e., become bluer at shorter wavelengths), then brighten in the visible to near-infrared region, leading to Bennu’s moderately blue average color. Craters indicate that the time scale of these color changes is ~105 years. We attribute the reflectance and color variation to a combination of primordial heterogeneity and varying exposure ages.
                            Related projects
                 
Small Bodies of the Solar System
            
    This project studies the physical and compositional properties of the so-called minor bodies of the Solar System, that includes asteroids, icy objects, and comets. Of special interest are the trans-neptunian objects (TNOs), including those considered the most distant objects detected so far (Extreme-TNOs or ETNOs); the comets and the comet-asteroid
            
            Julia de
            
                        León Cruz