The Jovian stratosphere after comet Shoemaker-Levy/9: Unusual isotopic ratios in molecular trace constituents

被引:7
作者
Matthews, HE
Marten, A
Moreno, R
Owen, T
机构
[1] Joint Astron Ctr, Hilo, HI 96720 USA
[2] Observ Paris, LESIA, F-92195 Meudon, France
[3] Inst Radio Astron Millimetr, F-38406 St Martin Dheres, France
[4] Univ Hawaii Manoa, Astron Inst, Honolulu, HI 96822 USA
[5] Natl Res Council Canada, Herzberg Inst Astrophys, Victoria, BC V9E 2E7, Canada
关键词
comets : individual (Shoemaker-Levy/9); planets and satellites : individual (Jupiter); submillimeter;
D O I
10.1086/343108
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Since the collision of comet Shoemaker-Levy/9 with Jupiter in 1994 July, a number of minor molecular species have been observed to persist in the stratosphere of the planet. Here we report observations acquired in 1998 September at frequencies near 350 GHz ( wavelength 850 mum) of HCN and CS and their respective isotopomers H(13)CN, HC(15)N, and C(34)S. Through radiative transfer modeling of the observed lines, we find that the isotopic abundance ratios (12)C/(13)C, (14)N/(15)N, and (32)S/(34)S are considerably elevated with respect to their terrestrial values. We speculate that this result indicates an unusual composition for comet Shoemaker-Levy/9, or that cometary grains evaporated in the collisions significantly modified the isotope ratios.
引用
收藏
页码:598 / 605
页数:8
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