10.1126/science.149.3682.443
Crossref journal-article
American Association for the Advancement of Science (AAAS)
Science (221)
Abstract

Nagy's report of an optical rotation of -0.023° to -0.084° in the Orgueil meteorite has not been confirmed. The highest rotation found in several fatty-acid and hydrocarbon fractions isolated from the meteorite was -0.002°, less than that of optically inactive controls. The "rotations" observed by Nagy may have been caused by scattered depolarized light from colloidal particles, reduced instrument sensitivity due to low transmittance of the solutions, or a combination of both.

Bibliography

Hayatsu, R. (1965). Optical Activity in the Orgueil Meteorite. Science, 149(3682), 443–447.

Authors 1
  1. Ryoichi Hayatsu (first)
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Dates
Type When
Created 18 years, 11 months ago (Oct. 5, 2006, 6:04 a.m.)
Deposited 1 year, 7 months ago (Jan. 10, 2024, 9:24 p.m.)
Indexed 1 year, 7 months ago (Jan. 11, 2024, 4:21 p.m.)
Issued 60 years, 1 month ago (July 23, 1965)
Published 60 years, 1 month ago (July 23, 1965)
Published Print 60 years, 1 month ago (July 23, 1965)
Funders 0

None

@article{Hayatsu_1965, title={Optical Activity in the Orgueil Meteorite}, volume={149}, ISSN={1095-9203}, url={http://dx.doi.org/10.1126/science.149.3682.443}, DOI={10.1126/science.149.3682.443}, number={3682}, journal={Science}, publisher={American Association for the Advancement of Science (AAAS)}, author={Hayatsu, Ryoichi}, year={1965}, month=jul, pages={443–447} }