@Article{MarchiMerVenPraMis:2021:EfSoRa,
               author = "Marchi, Luis Ot{\'a}vio and Merguizo Sanchez, Diogo and Venditti, 
                         F. C. F. and Prado, Antonio Fernando Bertachini de Almeida and 
                         Misra, A. K.",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {University of Central 
                         Florida} and {Instituto Nacional de Pesquisas Espaciais (INPE)} 
                         and {McGill University}",
                title = "On the effects of solar radiation pressure on the deviation of 
                         asteroids",
              journal = "Revista Mexicana de Astronomia y Astrofisica",
                 year = "2021",
               volume = "57",
               number = "2",
                pages = "279--295",
             keywords = "Balloons, Celestial mechanics, Minor planets, asteroids: general, 
                         Minor planets, asteroids: individual: PHAs.",
             abstract = "In this work, we study the effects of solar radiation pressure 
                         (SRP) on the problem of changing the orbit of an asteroid to 
                         support planetary defense, scientific research, or exploitation of 
                         materials. This alternative considers a tethered reflective 
                         balloon (or a set of reflective balloons) attached to the 
                         asteroid, with a high area-to-mass ratio, to use the SRP to 
                         deflect a potentially hazardous asteroid (PHA) or to approximate 
                         the target asteroid to Earth. The tether is assumed to be 
                         inextensible and massless, and the motion is described only in the 
                         orbital plane of the asteroid around the Sun. The model is then 
                         used to study the effects that the tether length, the reflectivity 
                         coefficient, and the area-to-mass ratio have on the deviation of 
                         the trajectory of the asteroid.",
                  doi = "10.22201/ia.01851101p.2021.57.02.03",
                  url = "http://dx.doi.org/10.22201/ia.01851101p.2021.57.02.03",
                 issn = "0185-1101",
             language = "en",
           targetfile = "marchi_effects.pdf",
        urlaccessdate = "03 maio 2024"
}