Integrated Study of the Physical Characteristics of Primitive Solar System Bodies

Bibcode
2003RMxAC..16...94K
Kolokolova, L.; Gustafson, B. A. S.; Lara, L. M.; Licandro, J.; Tozzi, G. P.
Referencia bibliográfica

Science with the GTC (Eds. José Miguel Rodríguez Espinosa, Francisco Garzón López, and Verónica Melo Martín) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 16, pp. 94-97 (2003) (http://www.astroscu.unam.mx/~rmaa/)

Fecha de publicación:
0
2003
Número de autores
5
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Primitive bodies (comets, Centaurs, trans-Neptunian objects, etc.) are the best-preserved remnants of the Solar Nebula. Their composition and structure harbor clues to the origin of solar and exosolar planets and the evolution of protoplanetary disks. The capabilities of the Gran Telescopio Canarias (GTC) and its instrumentation provide us a unique opportunity to accomplish an integrated study of the physical properties of these remote small bodies.
Tipo
Sin árbitro
Sistema solar
Discos protoplanetarios

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