LARGE LUNAR SECONDARY CRATERS - SIZE-RANGE RELATIONSHIPS

被引：19

作者：

ALLEN, CC

机构：

来源：

GEOPHYSICAL RESEARCH LETTERS | 1979年 / 6卷 / 01期

关键词：

D O I：

10.1029/GL006i001p00051

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

The relationship between primary crater diameter and mean maximum secondary crater diameter for lunar craters is essentially linear for primary diameters from 0.5 to 260 km. The mean range from the primary to the largest secondary craters is also nearly linearly related to primary diameter. Extrapolation of these results to lunar basin scale supports the contention that basin secondaries of large diameter are to be found across much of the Moon. © 1979 by the Chinese Geophysical Society

引用

页码：51 / 54

页数：4

共 14 条

[1]

Baldwin R.B., 1949, THE FACE OF THE MOON

[2]

Head J. W., 1974, Moon, V11, P327, DOI 10.1007/BF00589168

[3] ORIGIN OF LUNAR SMOOTH-PLAINS [J].

OBERBECK, VR ;

HORZ, F ;

MORRISON, RH ;

QUAIDE, WL ;

GAULT, DE .

MOON, 1975, 12 (01) :19-54

[4] COMPARATIVE STUDIES OF LUNAR, MARTIAN, AND MERCURIAN CRATERS AND PLAINS [J].

OBERBECK, VR ;

QUAIDE, WL ;

ARVIDSON, RE ;

AGGARWAL, HR .

JOURNAL OF GEOPHYSICAL RESEARCH, 1977, 82 (11) :1681-1698

[5]

OBERBECK VR, 1974, P LUNAR PLANET SCI C, P111

[6]

OBERBECK VR, 1978, LUNAR PLANETARY SCI, V9, P829

[7]

Scott David H., 1977, GEOLOGIC MAP W SIDE

[8]

SCOTT DH, 1972, GEOLOGIC MAP MAUROLY

[9]

SHOEMAKER EM, 1962, PHYSICS ASTRONOMY MO

[10]

TRASK NJ, 1965, ASTROGEOL STUDIES AN, P3

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