Water production of comet C/1999 S4 (LINEAR) observed with the SWAN instrument

被引:46
作者
Teemu, J
Mäkinen, T
Bertaux, JL
Combi, MR
Quémerais, E
机构
[1] Finnish Meteorol Inst, FIN-00101 Helsinki, Finland
[2] CNRS, Serv Aeron, F-91371 Verrieres Buisson, France
[3] Univ Michigan, Space Phys Res Lab, Ann Arbor, MI 48109 USA
关键词
D O I
10.1126/science.1060858
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 SWAN (Solar Wind ANisotropies) Lyman-alpha all-sky camera on the SOHO spacecraft observed the hydrogen coma of comet C/1999 S4 (LINEAR) from the end of May through mid-August 2000. A systematic set of water-production rates was obtained for this well-documented event of complete fragmentation of a cometary nucleus. The observations indicate that the lower limit for the sunlit surface area of the nucleus was about 1 square kilometer before the fragmentation and that the amount of water released throughout the observing period was 3.3 x 10(9) kilograms. Evidence suggests that the activity of the comet was dominated by successive fragmentation. There were four major outbursts, occurring about every 16 days. The 21 July event led to the complete fragmentation and sublimation of what remained of the nucleus, producing the last 3 x 10(8) kilograms of water. A model where the fragment size distribution follows the power Law N(R) similar to R-2.7, where N and R are the number and radius of fragments, reproduces the observed dissipation. This distribution possibly reflects the internal structure of the nucleus.
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页码:1326 / 1329
页数:4
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