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Three-dimensional spectral analysis of compositional heterogeneity at Arruntia crater on (4) Vesta using Dawn FC

MPS-Authors
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Thangjam,  Guneshwar
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Nathues,  Andreas
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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Schäfer,  Michael
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Hoffmann,  Martin
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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Platz,  Thomas
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Schäfer,  Tanja
Department Planets and Comets, 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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Citation

Thangjam, G., Nathues, A., Mengel, K., Schäfer, M., Hoffmann, M., Cloutis, E. A., et al. (2016). Three-dimensional spectral analysis of compositional heterogeneity at Arruntia crater on (4) Vesta using Dawn FC. Icarus, 267, 344-363. doi:10.1016/j.icarus.2015.11.031.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0029-3417-E
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