NASA NTRS · 19740010365
Remote sensing of Mare Serenitatis
Abstract
An examination was made of earth based observations of optical color differences, infrared eclipse temperatures, and radar backscatter for Mare Serenitatis. Information is also included on orbital observations, physical properties of surface types, and correlation of surface types with geologic units. Differences in these remote observations are attributed to variations in chemical and minerological compositions.
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Thompson, T. W., Howard, K. A., Shorthill, R. W., Tyler, G. L., Zisk, S. H., Whitaker, E. A., Schaber, G. G., Moore, H. J.. 1973-01-01. Remote sensing of Mare Serenitatis. https://ntrs.nasa.gov/citations/19740010365
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