REFLECTANCE SPECTROPHOTOMETRY (APPROXIMATELY-0.5-1.0-MU-M) OF OUTER-BELT ASTEROIDS - IMPLICATIONS FOR PRIMITIVE, ORGANIC SOLAR-SYSTEM MATERIAL

被引：83

作者：

VILAS, F ^{[1
]}

SMITH, BA ^{[1
]}

机构：

[1] UNIV ARIZONA,LUNAR & PLANETARY LAB,TUCSON,AZ 85721

来源：

ICARUS | 1985年 / 64卷 / 03期

关键词：

D O I：

10.1016/0019-1035(85)90071-5

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：503 / 516

页数：14

共 25 条

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[2]

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[3]

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[4]

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BELL, JF ;

GAFFEY, MJ ;

BROWN, RH ;

HOWELL, R ;

BEERMAN, C ;

ROGNSTAD, M .

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[6]

Degewij J., 1979, ASTEROIDS, P417

[7] MASS REMOVED BY OUTER PLANETS IN EARLY SOLAR-SYSTEM [J].

FERNANDEZ, JA .

ICARUS, 1978, 34 (01) :173-181

[8] DETECTION OF A CH4 ATMOSPHERE ON PLUTO [J].

FINK, U ;

SMITH, BA ;

BENNER, DC ;

JOHNSON, JR ;

REITSEMA, HJ ;

WESTPHAL, JA .

ICARUS, 1980, 44 (01) :62-71

[9]

FREIDEN BR, 1983, PROBABILITY STATISTI

[10]

Gaffey M. J., 1979, ASTEROIDS, P688

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