The small binary asteroid (939) Isberga

The small binary asteroid (939) Isberga

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...

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Bibliographic Details
Main Authors: Carry, B. (Author), Matter, A. (Author), Scheirich, P. (Author), Pravec, P. (Author), Molnar, L. (Author), Mottola, S. (Author), Carbognani, A. (Author), Jehin, E. (Author), Marciniak, A. (Author), Birlan, M. (Author), Delbo, M. (Author), Barbotin, E. (Author), Behrend, R. (Author), Bonnardeau, M. (Author), Colas, F. (Author), Farissier, P. (Author), Fauvaud, M. (Author), Fauvaud, S. (Author), Gillier, C. (Author), Gillon, M. (Author), Hellmich, S. (Author), Hirsch, R. (Author), Leroy, A. (Author), Manfroid, J. (Author), Montier, J. (Author), Morelle, E. (Author), Richard, F. (Author), Sobkowiak, K. (Author), Strajnic, J. (Author), Vachier, F. (Author), Binzel, Richard P (Contributor), DeMeo, Francesca E (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor)
Format: Article
Language:English
Published: Elsevier, 2017-05-03T15:25:11Z.
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