A possibility of prognosticating the lunar surface composition prediction from optical measurement data

1Shkuratov, Yu.G, 2Kaydash, VG, 3Opanasenko, NV, 3Stankevich, DG, 4Evsyukov, NN, 5Parusimov, VG
1Institute of Astronomy of V. N. Karazin Kharkiv National University, Kharkiv, Ukraine; Institute of Radio Astronomy of the National Academy of Sciences of Ukraine, Kharkiv, Ukraine
2Institute of Astronomy of V. N. Karazin Kharkiv National University, Kharkiv, Ukraine
3Institute of Astronomy of V.N. Karazin National University of Kharkiv, Kharkiv, Ukraine
4V.N. Karazin National University of Kharkiv,Kharkiv, Ukraine
5Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Kyiv, Ukraine
Kosm. nauka tehnol. 1996, 2 ;(3):78–88
Section: Space Astronomy
Publication Language: Russian
Maps of rock-forming oxides (Ti02 and FeO) were drawn for Ihe Moon's visible side. For this purpose we used new albedo (0.65 / 0.42 μm) and color-index (0.65 / 0.42 μm) distribution data and new calibration relationships between these optical parameters and the content of chromophore elements (iron and titanium). Comparison of the lunar albedo-color diagram with the chemical diagram for lunar rocks presented in the albedo-color axes allowed us to outline four clusters in the lunar diagram which correspond to some lunar rock types. For example, one of the clusters corresponds to the region formed by ilmenite and ilmenite-olivine basalts. This data allowed us to map the distribution of some lunar rock types corresponding to the classification of Bogatikov et al. (1985). Such a method of composition prediction may be applied to the analysis of the data obtained in the «Clementine» survey of the lunar surface.
Keywords: lunar surface, optical measurements
Akimov L. A. Disk brightness distribution of the moon and planets. Astron. Zhurnal, 56, 412—418 (1979) [in Russian].
Akimov L. A., Latynina I. I., Olifer N. S. Reference catalogue of optical characteristics of selected areas on the lunar surface.
(Dep. v UkrNIINTI 18.11.86; No. 2689), 31 p. (Khar'k. univ., Khar'kov, 1986) [in Russian].
Bogatikov O. A., Gon'shakova V. I., Frih-Har D. I. Classification of lunar igneous rocks, 72 p. (Nedra, Moscow, 1985) [in Russian].
Wood J. A. Overview of types of lunar rocks and comparison of lunar and earth's crust.. In: Cosmochemistry Moon and planets, Ed. by A. P. Vinogradov, 29—45 (Nauka, Moscow, 1975) [in Russian].
Evsyukov N. N. Albedo map of the visible hemisphere of the Moon. (Nauk. dumka, Kiev, 1973) [in Russian].
Evsyukov N. N. Colour’s map of the visible hemisphere of the Moon. (Nauk. dumka, Kiev, 1973) [in Russian].
Evsjukov N. N. A connection of optical characteristics with the chemical and mineralogical composition of the lunar rocks.  Astron. zhurn., 51, 1316—1325 (1974) [in Russian].
Evsyukov N. N. Algorithm reliability of remote optical analysis of lunar mature rock chemical composition. Astron. Vestn., 26 (3), 59—73 (1994) [in Russian].
Evsjukov N. N., Shestopalov D. I. On mineral composition of lunar soils. Astron. Vestn., 12 (1), 18— 26 (1978) [in Russian].
King E. A. Space geology [Kosmicheskaja geologija], 379 p. (Mir, Moscow, 1979) [in Russian].
Kislyuk V. S., Shkuratov Yu. G., Yatskiv Ya. S. Exploration of the Moon from space: tasks, potentialities, and prospects of the Ukrainian science and engineering. Kosm. nauka tehnol., 2 (1-2), 3—14 (1996) [in Ukrainian].
Mason B., Melson W. G. The lunar rocks. [Lunnye porody]: Transl. from Eng., 165 p. (Mir, Moscow, 1973) [in Russian].
Nava D. F., Philpotts J. A. A model for differentiation of the moon in the light of new data on the chemical composition of regolith returned by Luna 20. Regolith from the highland region of the moon, Ed. by V. L. Barsukov, 337—344 (Nauka, Moscow, 1979) [in Russian].
Nemoshkalenko V. V. Investigation of the lunar regolith. Kosm. nauka tehnol., 2 (1-2), 16—23 (1996) [in Ukrainian].
Nikolaeva O. V. The Earth is the Past of the Moon, but the Moon, Earth's Future. Priroda,  No. 10, 13—25 (1995) [in Russian].
Parusimov V. G. Automatic Digital Two-Coordinate Microphotometer for Input of Photographic Images Into Computer. Astrometriia i Astrofizika, Is. 45, 86—99 (1981) [in Russian].
Phinney W. C., Warner J. L., Simonds C. H. Types of lunar continental rocks and their relation to the impact of fractionation processes. In: Cosmochemistry Moon and planets, Ed. by A. P. Vinogradov, 54—88 (Nauka, Moscow, 1975) [in Russian].
Florenskii K. P., Bazilevskii A. T., Burba G. A., et al. Sketches on comparative planetology, 328 p. (Nauka, Moscow, 1981) [in Russian].
Shkuratov Yu. G. The lunar albedo. Vestn. Khar'kov. Univ., No. 232, Astrometrija i fizika Solnechnoj sistemy, Is. 17, 22—31 (1982) [in Russian].
Charette M., McCord T. B., Pieters C. et al. Application of remote spectral reflectance measurements to lunar geology classification and determination of titanium content of lunar soils. J. Geophys. Res., 79, 1605—1613 (1974).
Charette M., Soderblom L., Adams J. et al. Age-color relationships in the lunar highland. Proc. Lunar Sci. Conf. 7th, P. 2579—2592 (LPI Houston, 1976).
Fisher E., Pieters C. Composition and exposure age of the Apollo 16 Cayley and Descartes regions from Clementine data: normalizing the optical effect of space weathering. J. Geophys. Res., 101E (1), 2225—2234 (1996).
Johnson T. V., Saunders S., Matson D., Mosher J. A Ti02 abundance map for northern maria. Proc. Lunar Sci. Conf. 8th, P. 1029—1036 (LPI Houston, 1977).
Johnson J. R., Larson S. M., Singer R. B. Remote sensing of potential lunar resourses. I. Near-side composition properties. J. Geophys. Res., 96E (3), 18861 — 18882 (1991).
Kaydash V. G., Shkuratov Yu. G., Slankevich D. G., et al. Mapping of the Fe content in lunarregolith by albedo and color-index measurements. Abstr. of papers subm. to 22nd Russian-American microsymposium, October 1995,  P. 27—29 (Moscow, 1995).
Lucey P., Blewett D., Johnson J. Lunar titanium content from UV-VIS measurements. Abstr. of papers subm. to 27th Lunar and Planetary Science Conf., P. 781 (Houston, 1996).
Lucey P., Taylor G., Malaret E. Abundance and distribution of iron on the Moon. Science, 268, 1150—1153 (1995).
Morris R. Origin and evolution of the grain-size dependence of concentration of tined-grained metal in lunar soils: The maturation of lunar soils to steady-state stage. Proc. Lunar Planet.  Sci. Conf.  9th, P. 2287— 2297 (LPI Houston, 1978).
Opanasenko N. V., Shkuratov Yu. G., Kaydash V. G. Estimations of iron content in lunar regolith by measurements of spectral slope in 0.95 µm absorption band. Abstr. of papers subm. to 24nd Russian-American microsymposiurn, October 1996, P. 70—71 (Moscow, 1996).
Pieters C. A summary of spectral reflectance data. Proc. Lunar Sci. Conf. 9th, P. 2825—2849 (LPI Houston, 1978).
Pieters C., McCord T. Characterization of lunar mare basalt types. Proc. Lunar Sci. Conf. 7th,  P. 2677—2690 (LPI Houston, 1976).
Ryder J., McEwen H. G., Marvin U. B. Basalts from Mare Crisium. The Moon, 17, 263—287 (1977).
Shkuratov Yu. G., Opanasenko N. V. Polarimetric and photometric properties of the Moon: telescope observation and laboratory simulation. 2. Icarus, 99, 468—484 (1992).
Shkuratov Yu. G., Opanasenko N. V., Kreslavsky M. A. Polarimetric and photometric properties of the Moon: telescope observation and laboratory simulation. 1. Icarus, 95, 282—299 (1992).

Taylor S. Lunar science: Post Apollo Era, 370 p. (N. Y., 1972).