MARTIAN SURFACE MATERIALS - EFFECT OF PARTICLE SIZE ON SPECTRAL BEHAVIOR

被引:33
作者
SALISBUR.JW
HUNT, GR
机构
[1] Lunar-Planetary Research Branch, Air Force Cambridge Research Laboratories, L. G. Hanscom Field, Bedford
关键词
D O I
10.1126/science.161.3839.365
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The presence of abundant limonite on Mars has long been the subject of controversy. Some advocates of abundant limonite also suggest that the albedo differences between Martian light and dark areas are caused by different sizes of particles in those areas. We show that the relative albedo is reversed from the blue to the red for samples of limonite with particles of different sizes. Observations of Mars reveal no blue-red albedo reversal between the light and dark areas. Consequently, the hypothesis of particle size control of albedo is incompatible with the presence of abundant limonite on Mars.
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页码:365 / &
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共 18 条
[11]  
RZHIGA ON, 1967, SOV ASTRON, V11, P113
[12]  
SAGAN C, 1966, ASTRON J, V71, P178
[13]   MARINER 4 OBSERVATIONS AND POSSIBILITY OF IRON OXIDES ON MARTIAN SURFACE [J].
SAGAN, C .
ICARUS, 1966, 5 (01) :102-&
[14]   TOTAL REFLECTION SPECTROPHOTOMETRY AND THERMOGRAVIMETRIC ANALYSIS OF SIMULATED MARTIAN SURFACE MATERIALS [J].
SAGAN, C ;
PHANEUF, JP ;
IHNAT, M .
ICARUS, 1965, 4 (01) :43-&
[15]  
SHARONOV VV, 1961, SOV ASTRON, V5, P199
[16]  
TIKHOV GA, 1956, IZV AKAD NAUK SSSR K, V16, P159
[17]   COMPOSITION OF MARTIAN SURFACE [J].
VANTASSEL, RA ;
SALISBURY, JW .
ICARUS, 1964, 3 (03) :264-&
[18]   A SEARCH FOR LIMONITE NEAR-INFRARED SPECTRAL FEATURES ON MARS [J].
YOUNKIN, RL .
ASTROPHYSICAL JOURNAL, 1966, 144 (02) :809-&