The 2.5-5.1 μm reflectance spectra of HED meteorites and their constituent 
minerals: Implications for Dawn

Cloutis, E. A.; Mann, P.; Izawa, M. R. M.; Nathues, A.; Reddy, V.; Hiesinger, H.; Le Corre, L.; Palomba, E.

doi:10.1016/j.icarus.2013.04.022

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The 2.5-5.1 μm reflectance spectra of HED meteorites and their constituent minerals: Implications for Dawn

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

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Le Corre, L.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Cloutis, E. A., Mann, P., Izawa, M. R. M., Nathues, A., Reddy, V., Hiesinger, H., et al. (2013). The 2.5-5.1 μm reflectance spectra of HED meteorites and their constituent minerals: Implications for Dawn. Icarus, 225(1), 581-601. doi:10.1016/j.icarus.2013.04.022.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-0C13-1

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