DEUTERIUM ON VENUS - OBSERVATIONS FROM EARTH

被引:134
作者
DEBERGH, C
BEZARD, B
OWEN, T
CRISP, D
MAILLARD, JP
LUTZ, BL
机构
[1] LOWELL OBSERV,FLAGSTAFF,AZ 86001
[2] UNIV HAWAII,INST ASTRON,HONOLULU,HI 96822
[3] CALTECH,JET PROP LAB,PASADENA,CA 91109
[4] INST ASTROPHYS,F-75014 PARIS,FRANCE
关键词
D O I
10.1126/science.251.4993.547
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
Absorption lines of HDO and H2O have been detected in a 0.23-wave number resolution spectrum of the dark side of Venus in the interval 2.34 to 2.43 micrometers, where the atmosphere is sounded in the altitude range from 32 to 42 kilometers (8 to 3 bars). The resulting value of the deuterium-to-hydrogen ratio (D/H) is 120 +/- 40 times the telluric ratio, providing unequivocal confirmation of in situ Pioneer Venus mass spectrometer measurements that were in apparent conflict with an upper limit set from International Ultraviolet Explorer spectra. The 100-fold enrichment of the D/H ratio on Venus compared to Earth is thus a fundamental constraint on models for its atmospheric evolution.
引用
收藏
页码:547 / 549
页数:3
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