Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.

Site Tools

  • AAAS
  • Subscribe
  • Feedback

Site Search

Search Advanced

Science 20 February 1998:
Vol. 279. no. 5354, pp. 1181 - 1184
DOI: 10.1126/science.279.5354.1181

Reports

The Formation of HCS and HCSH Molecules and Their Role in the Collision of Comet Shoemaker-Levy 9 with Jupiter

R. I. Kaiser, * C. Ochsenfeld, M. Head-Gordon, Y. T. Lee dagger

The reaction of hydrogen sulfide with ground-state atomic carbon was examined with crossed molecular beams experiments and ab initio calculations. The thiohydroxycarbene molecule, HCSH, was the reactive intermediate, which fragmented into atomic hydrogen and the thioformyl radical HCS. This finding may account for the unassigned HCS source and an unidentified HCSH radical needed to match observed CS abundances from the collision of comet Shoemaker-Levy 9 into Jupiter. In the shocked jovian atmosphere, HCS could further decompose to H and CS, and CS could react with SH and OH to yield the observed CS2 and COS.

Department of Chemistry, University of California, Berkeley and Chemical Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA.
*   Present address: Academia Sinica, Institute of Atomic and Molecular Sciences, 1, Section 4, Roosevelt Road, Taipei, 116, Taiwan, Republic of China, and Department of Physics, Technical University Chemnitz-Zwickau, 09107 Chemnitz, Germany.

dagger    Present address: Academia Sinica, Institute of Atomic and Molecular Sciences, 1, Section 4, Roosevelt Road, Taipei, 116, Taiwan, Republic of China.


Read the Full Text





To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)