Lunar mineral mapping in Sinus Iridum in consideration of mineral grain sizes

doi:10.6046/gtzyyg.2018.02.20

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Abstract

The distribution of the mineral abundances on lunar surface has a significant meaning. Hapke model is one of the most usually used methods for studying lunar surface, and particle size is one of the parameters that must be clearly understood in doing model calculation. Nevertheless, the research on grain size remains very insufficient. To study the distribution of the abundances of five main minerals, i.e., clinopyroxene, orthopyroxene, plagioclase, olivine and ilmenite, the authors considered the influence of grain size and built inverse models of these five minerals by using fully constrained linear-unmixing method with Relab data based on Hapke radioative transfer model, with the correlation coefficients of these five minerals being 0.98, 0.98, 0.83, 0.91 and 0.50. Furthermore, the accuracy of this models was verified by using data of Apollo sampling points . At last, the lunar minerals abundance distribution maps of Sinus Iridum were compiled by applying the models to the M ³ hyperspectral data,which shows that the fully constrained linear-unmixing method in consideration of mineral grain sizes can be used to study lunar mineral abundance distribution.

Keywords Sinus Iridum mineral grain size full constrained linear-unmixing M ³

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Corresponding Authors: Weihua LIN E-mail: 963339577@qq.com;22384138@qq.com

Issue Date: 30 May 2018

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	Xiaoying DONG
	Weihua LIN
	Fujiang LIU
	Qi ZHANG
	Yuan CHANG

Cite this article:

Xiaoying DONG,Weihua LIN,Fujiang LIU, et al. Lunar mineral mapping in Sinus Iridum in consideration of mineral grain sizes[J]. Remote Sensing for Land & Resources, 2018, 30(2): 147-153.

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https://www.gtzyyg.com/EN/10.6046/gtzyyg.2018.02.20 OR https://www.gtzyyg.com/EN/Y2018/V30/I2/147

Tab.1 Main technical and performance indicates of M³

Tab.2 Optical constant information of endmember mineralsin Relab spectral library (nm)

Fig.1 Statistical relations between the unmixing abundance and the real abundance of different endmember minerals

Tab.3 Comparison between the inversed abundance and the measured abundance of different endmember minerals in Apollo(%)

Fig.2 Statistical relations between the inversed abundance and the measured abundance of different endmember minerals in Apollo

Fig.3 Process flowchart of M³ data

Fig.4 Mineral abundance distribution in Sinus Iridum

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