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The pebbles/boulders size distributions on Sais: Rosetta's final landing site on comet 67P/Churyumov-Gerasimenko

MPS-Authors
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Kovacs,  G.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Shi,  X.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Tubiana,  C.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Güttler,  C.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Sierks,  H.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Agarwal,  J.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Deller,  J.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Gicquel,  A.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Höfner,  S.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Hofmann,  M.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

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Kramm,  J. R.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Pajola, M., Lucchetti, A., Fulle, M., Mottola, S., Hamm, M., Da Deppo, V., et al. (2017). The pebbles/boulders size distributions on Sais: Rosetta's final landing site on comet 67P/Churyumov-Gerasimenko. Mon. Not. Roy. Astron. Soc., 469(Suppl_2), 636-645. doi:10.1093/mnras/stx1620.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002E-538F-E
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