MERCURY SOIL - PRESENCE OF FE2+

被引：77

作者：

MCCORD, TB ^{[1
]}

CLARK, RN ^{[1
]}

机构：

[1] MIT,DEPT EARTH & PLANETARY PHYS,CAMBRIDGE,MA 02139

来源：

JOURNAL OF GEOPHYSICAL RESEARCH | 1979年 / 84卷 / NB13期

关键词：

D O I：

10.1029/JB084iB13p07664

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

引用

页码：7664 / 7668

页数：5

共 22 条

[1]

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[2]

ADAMS JB, 1973, 4 P LUN SCI C GEO S4, V1, P163

[3]

ADAMS JB, 1974, J GEOPHYS RES, V79, P4329

[4]

ADAMS JE, UNPUBLISHED

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APPLIED OPTICS, 1969, 8 (11) :2215-&

[6]

CLARK RN, UNPUBLISHED

[7]

CLARK RN, 1979, ICARUS, V39

[8] PHOTOMETRIC OBSERVATIONS OF MERCURY FROM MARINER-10 [J].

HAPKE, B ;

DANIELSON, GE ;

KLAASEN, K ;

WILSON, L .

JOURNAL OF GEOPHYSICAL RESEARCH, 1975, 80 (17) :2431-2443

[9] INTERPRETATIONS OF OPTICAL OBSERVATIONS OF MERCURY AND MOON [J].

HAPKE, B .

PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 1977, 15 (2-3) :264-274

[10] TEMPERATURE-GRADIENT IN SOLAR NEBULA [J].

LEWIS, JS .

SCIENCE, 1974, 186 (4162) :440-443

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