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El asteroide de tipo E (2867) Steins, fotografiado por OSIRIS a bordo de la nave Rosetta

H U Keller1, C Barbieri, D Koschny

  • 1Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany. keller@linmpi.mpg.de

Science (New York, N.Y.)
|January 9, 2010
PubMed
Resumen

La misión Rosetta reveló que el asteroide Steins es un montón de escombros, no una roca sólida. Las imágenes proporcionan evidencia directa del efecto Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) que está cambiando la forma de los asteroides.

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