Artículo

Results of the investigation of the asteroid (2121) Sevastopol based on photometric observations of mutual phenomena

Sokova, Iraida A.; Sokov, Eugenii N.; Gorshanov, Denis L.; Fernandez Lajus, Eduardo EusebioIcon ; Di Sisto, Romina PaulaIcon ; Bretton, Marc; Marchini, Alessandro; Vasilkova, Olga O.; Knight, Carl R.; Colazo, Carlos Roberto; Quiñones, Cecilia; Girardini, Carla
Fecha de publicación: 05/2019
Editorial: Pergamon-Elsevier Science Ltd
Revista: Planetary and Space Science
ISSN: 0032-0633
Idioma: Inglés
Tipo de recurso: Artículo publicado
Clasificación temática:

Resumen

The asteroid (2121) Sevastopol is a binary asteroid from the main belt. The duplicity of the asteroid was discovered based on photometric observations of mutual phenomena (eclipses and occultations) that were detected in its light curves (Higgins et al., 2010). We organized a photometrical observational campaign for the observations of mutual phenomena in binary system of the asteroid (2121) Sevastopol and an investigation of the properties of the asteroid's satellite. The observations allowed us to define mass, density, taxonomical class and preliminary orbit of the satellite of the asteroid (2121) Sevastopol.
Palabras clave: ASTEROIDS , ASTEROIDS , CELESTIAL MECHANICS , DYNAMICS , ROTATION , SATELLITES OF ASTEROIDS
 
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info:eu-repo/semantics/restrictedAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)
Identificadores
URI: http://hdl.handle.net/11336/125639
URL: https://linkinghub.elsevier.com/retrieve/pii/S003206331830415X
DOI: http://dx.doi.org/10.1016/j.pss.2019.05.007
Colecciones
Articulos(IALP)
Articulos de INST.DE ASTROFISICA LA PLATA
Citación
Sokova, Iraida A.; Sokov, Eugenii N.; Gorshanov, Denis L.; Fernandez Lajus, Eduardo Eusebio; Di Sisto, Romina Paula; et al.; Results of the investigation of the asteroid (2121) Sevastopol based on photometric observations of mutual phenomena; Pergamon-Elsevier Science Ltd; Planetary and Space Science; 175; 5-2019; 25-33
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