RADIATIVE TRANSFER MODELING OF NEAR-INFRARED REFLECTANCE DATA OF MERCURY
To address this issue, our model also includes optical constants for opaque metal and mineral phases. The model used for this study was adapted from the work of [17], which uses optical constants for metals (Fe, Ni) to introduce the darkening and/or reddening effects macroscopic and submicroscopic metal on reflectance spectra. We have two main goals of the current study. First, we seek to extend the opaque phases available for spectral mixing and space weathering, which were previously centered on the Fe-rich nature of the Moon (e.g., metallic Fe), including sufides (FeS, MgS, CaS) and graphite (C). Second, we aim to dissociate the microphase and the nanophase metal phases within the model. Results of these models for planetary spectra will be presented.
References: [1] Hapke, B. (1981). [2] Hapke, B. (1993). [3] Hapke, B. (2001. [4] Lucey (1998). [5] Wilcox et al. (2006). [7] Keller and McKay (1997). [8] Pieters et al. (2000). [9] Noble, et al. (2007). [10] Britt and Pieters (1994). [11] Pieters et al. (2000). [12] Noble and Pieters (2003). [13] Nobel et al. (2006). [14] Lucey and Noble (2008). [15] Lucey and Riner (2011). [16] Lawrence and Lucey (2007). [17] Cahill et al. (2015).