Gas-phase synthesis of racemic helicenes and their potential role in the enantiomeric enrichment of sugars and amino acids in meteorites
Abstract
The molecular origins of homochirality on Earth is not understood well, particularly how enantiomerically enriched molecules of astrobiological significance like sugars and amino acids might have been synthesized on icy grains in space preceding their delivery to Earth. Polycyclic aromatic hydrocarbons (PAHs) identified in carbonaceous chondrites could have been processed in molecular clouds by circularly polarized light prior to the depletion of enantiomerically enriched helicenes onto carbonaceous grains resulting in chiral islands. However, the fundamental low temperature reaction mechanisms leading to racemic helicenes are still unknown. Here, by exploiting synchrotron based molecular beam photoionization mass spectrometry combined with electronic structure calculations, we provide compelling testimony on barrierless, low temperature pathways leading to racemates of [5] and [6]helicene. Astrochemical modeling advocates that gas-phase reactions in molecular clouds lead to racemates of helicenes suggesting a pathway for future astronomical observation and providing a fundamental understanding for the origin of homochirality on early Earth.
- Authors:
-
- University of Hawaii at Manoa, Honolulu, HI (United States)
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Lebedev Physical Institute, Samara (Russia)
- Florida International University (FIU), Miami, FL (United States)
- University of California, Berkeley, CA (United States). Applied Science and Technology; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Kavli Energy NanoScience Institute, Berkeley, CA (United States)
- Chinese Academy of Sciences (CAS), Urumqi (China)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Basic Energy Sciences (BES). Chemical Sciences, Geosciences & Biosciences Division (CSGB); Russian Federation; National Energy Research Scientific Computing Center (NERSC); USDOE
- OSTI Identifier:
- 2325993
- Alternate Identifier(s):
- OSTI ID: 1885468
- Grant/Contract Number:
- AC02-05CH11231; FG02-03ER15411; FG02-04ER15570; 075-15-2021-597
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Chemistry Chemical Physics. PCCP
- Additional Journal Information:
- Journal Volume: 24; Journal Issue: 41; Journal ID: ISSN 1463-9076
- Publisher:
- Royal Society of Chemistry
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 37 INORGANIC, ORGANIC, PHYSICAL, AND ANALYTICAL CHEMISTRY
Citation Formats
Kaiser, Ralf I., Zhao, Long, Lu, Wenchao, Ahmed, Musahid, Evseev, Mikhail M., Azyazov, Valeriy N., Mebel, Alexander M., Mohamed, Rana K., Fischer, Felix R., and Li, Xiaohu. Gas-phase synthesis of racemic helicenes and their potential role in the enantiomeric enrichment of sugars and amino acids in meteorites. United States: N. p., 2022.
Web. doi:10.1039/d2cp03084e.
Kaiser, Ralf I., Zhao, Long, Lu, Wenchao, Ahmed, Musahid, Evseev, Mikhail M., Azyazov, Valeriy N., Mebel, Alexander M., Mohamed, Rana K., Fischer, Felix R., & Li, Xiaohu. Gas-phase synthesis of racemic helicenes and their potential role in the enantiomeric enrichment of sugars and amino acids in meteorites. United States. https://doi.org/10.1039/d2cp03084e
Kaiser, Ralf I., Zhao, Long, Lu, Wenchao, Ahmed, Musahid, Evseev, Mikhail M., Azyazov, Valeriy N., Mebel, Alexander M., Mohamed, Rana K., Fischer, Felix R., and Li, Xiaohu. Sat .
"Gas-phase synthesis of racemic helicenes and their potential role in the enantiomeric enrichment of sugars and amino acids in meteorites". United States. https://doi.org/10.1039/d2cp03084e. https://www.osti.gov/servlets/purl/2325993.
@article{osti_2325993,
title = {Gas-phase synthesis of racemic helicenes and their potential role in the enantiomeric enrichment of sugars and amino acids in meteorites},
author = {Kaiser, Ralf I. and Zhao, Long and Lu, Wenchao and Ahmed, Musahid and Evseev, Mikhail M. and Azyazov, Valeriy N. and Mebel, Alexander M. and Mohamed, Rana K. and Fischer, Felix R. and Li, Xiaohu},
abstractNote = {The molecular origins of homochirality on Earth is not understood well, particularly how enantiomerically enriched molecules of astrobiological significance like sugars and amino acids might have been synthesized on icy grains in space preceding their delivery to Earth. Polycyclic aromatic hydrocarbons (PAHs) identified in carbonaceous chondrites could have been processed in molecular clouds by circularly polarized light prior to the depletion of enantiomerically enriched helicenes onto carbonaceous grains resulting in chiral islands. However, the fundamental low temperature reaction mechanisms leading to racemic helicenes are still unknown. Here, by exploiting synchrotron based molecular beam photoionization mass spectrometry combined with electronic structure calculations, we provide compelling testimony on barrierless, low temperature pathways leading to racemates of [5] and [6]helicene. Astrochemical modeling advocates that gas-phase reactions in molecular clouds lead to racemates of helicenes suggesting a pathway for future astronomical observation and providing a fundamental understanding for the origin of homochirality on early Earth.},
doi = {10.1039/d2cp03084e},
journal = {Physical Chemistry Chemical Physics. PCCP},
number = 41,
volume = 24,
place = {United States},
year = {Sat Sep 03 00:00:00 EDT 2022},
month = {Sat Sep 03 00:00:00 EDT 2022}
}
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