Comptes Rendus Physique, 6, pp. 303-312, http://dx.doi.org./10.1016/j.crhy.2004.12.015
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In understanding the composition and internal structure of asteroids, their density is perhaps the most diagnostic quantity. We aim here at characterizing the surface composition, mutual orbit, size, mass, and density of the small main-belt binary asteroid (939) Isberga. For that, we conduct a suite of multi-technique observations, including...
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