Discovery of the interstellar chiral molecule propylene oxide (CH3CHCH2O)

被引:240
作者
McGuire, Brett A. [1 ,2 ]
Carroll, P. Brandon [2 ]
Loomis, Ryan A. [3 ]
Finneran, Ian A. [2 ]
Jewell, Philip R. [1 ]
Remijan, Anthony J. [1 ]
Blake, Geoffrey A. [2 ,4 ]
机构
[1] Natl Radio Astron Observ, Edgemont Rd, Charlottesville, VA 22903 USA
[2] CALTECH, Div Chem & Chem Engn, Pasadena, CA 91125 USA
[3] Harvard Univ, Dept Astron, Cambridge, MA 02138 USA
[4] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
基金
美国国家科学基金会;
关键词
GBT PRIMOS SURVEY; ORGANIC-MOLECULES; AMINO-ACIDS; TELESCOPE; CHEMISTRY; METEORITE; REGIONS; C-C2H4O; ICE;
D O I
10.1126/science.aae0328
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
Life on Earth relies on chiral molecules that is, species not superimposable on their mirror images.This manifests itself in the selection of a single molecular handedness, or homochirality, across the biosphere. We present the astronomical detection of a chiral molecule, propylene oxide (CH3CHCH2O), in absorption toward the Galactic center. Propylene oxide is detected in the gas phase in a cold, extended molecular shell around the embedded, massive protostellar clusters in the Sagittarius B2 star-forming region. This material is representative of the earliest stage of solar system evolution in which a chiral molecule has been found.
引用
收藏
页码:1449 / 1452
页数:4
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