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The rotation state of 67P/Churyumov-Gerasimenko from approach observations with the OSIRIS cameras on Rosetta

MPS-Authors
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Snodgrass,  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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Kramm,  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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Agarwal,  J.
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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Oklay,  N.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
IMPRS on Physical Processes in the Solar System and Beyond, 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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Vincent,  J.-B.
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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Citation

Mottola, S., Lowry, S., Snodgrass, C., Lamy, P. L., Toth, I., Rozek, A., et al. (2014). The rotation state of 67P/Churyumov-Gerasimenko from approach observations with the OSIRIS cameras on Rosetta. Astronomy and Astrophysics, 569: L2. doi:10.1051/0004-6361/201424590.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0027-7BD1-C
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