Did life originate from low-temperature areas of the Universe?
@article{Krasnokutski2020DidLO, title={Did life originate from low-temperature areas of the Universe?}, author={Serge A. Krasnokutski}, journal={arXiv: Earth and Planetary Astrophysics}, year={2020} }
The biological molecules delivered to Earth on the board of meteorites and comets were called one of the possible causes of the origin of life. Therefore, our understanding of the routes of formation of biomolecules in space should shed the light on the possibility of the existence of habitable extrasolar planets. The large abundance of organic molecules is found in the space regions with the lowest temperature. Different routes of the organics formation in these areas were suggested. In this…
7 Citations
Glycine Peptide Chain Formation in the Gas Phase via Unimolecular Reactions.
- Chemistry, PhysicsThe journal of physical chemistry. A
- 2023
Peptide chain formation from amino acids such as glycine is a key step in the emergence of life. Unlike their synthesis by living systems, how peptide chains grow under abiotic conditions is an open…
Unraveling sulfur chemistry in interstellar carbon oxide ices
- Chemistry, PhysicsNature Communications
- 2022
Formyl radical (HCO•) and hydroxycarbonyl radical (HOCO•) are versatile building blocks in the formation of biorelevant complex organic molecules (COMs) in interstellar medium. Understanding the…
Intrinsic disorder, extraterrestrial peptides, and prebiotic life on the earth.
- BiologyJournal of biomolecular structure & dynamics
- 2022
Bioinformatics analyses strongly predict such homo-polymeric peptides to be intrinsically disordered underscoring the potential involvement of IDPs in the origin of life which, even in its simplest form, could emerge spontaneously by autocatalysis of the primordial IDP in self-organizing systems that evolved over time following natural selection.
A pathway to peptides in space through the condensation of atomic carbon
- Physics, ChemistryNature Astronomy
- 2022
Organic molecules are widely present in the dense interstellar medium, and many have been synthesized in the laboratory on Earth under the conditions typical for an interstellar environment. Until…
Formation pathways of proteins in space
- Physics
- 2021
Until now, experiments demonstrated the possible formation of relatively small prebiotic molecules under typical space conditions. We demonstrated experimentally that condensation of atomic carbon…
Discovery in space of ethanolamine, the simplest phospholipid head group
- PhysicsProceedings of the National Academy of Sciences
- 2021
Significance The detection of ethanolamine (NH2CH2CH2OH) in a molecular cloud in the interstellar medium confirms that a precursor of phospholipids is efficiently formed by interstellar chemistry.…
Chemistry and physics of dopants embedded in helium droplets.
- PhysicsMass spectrometry reviews
- 2021
Development of experimental techniques and methods and recent results they enabled to grow complexes and clusters at conditions that are perfect to simulate cold and dense regions of the interstellar medium are summarized.
References
SHOWING 1-10 OF 49 REFERENCES
An Experimental and Theoretical Investigation into the Formation of Ketene (H2CCO) and Ethynol (HCCOH) in Interstellar Analog Ices
- Chemistry, PhysicsThe Astrophysical Journal
- 2020
The formation of isomers of C2H2O—ketene (H2CCO), ethynol (HCCOH), and oxirene (c-CHCHO)—was investigated in interstellar ice analogs composed of carbon monoxide and water. Using tunable…
A cryogenic ice setup to simulate carbon atom reactions in interstellar ices.
- PhysicsThe Review of scientific instruments
- 2020
The design, implementation, and performance of a customized carbon atom beam source for the purpose of investigating solid-state reaction routes in interstellar ices in molecular clouds are discussed, which includes the flux of the carbon atoms hitting the ice sample, their temperature, and the potential impact of temperature on ice reactions.
Sensitivity of gas-grain chemical models to surface reaction barriers
- ChemistryAstronomy & Astrophysics
- 2020
Context. The feasibility of contemporary gas-grain astrochemical models depends on the availability of accurate kinetics data, in particular, for surface processes.
Aims. We study the sensitivity of…
Condensation of Atomic Carbon: Possible Routes toward Glycine
- Chemistry, PhysicsThe Astrophysical Journal
- 2020
Many organic molecules including amino acids and nucleobases are expected to be formed in astrophysical environments. In this article, we used both experimental and computational approaches to test…
Fullerene Oligomers and Polymers as Carriers of Unidentified IR Emission Bands
- Physics, ChemistryThe Astrophysical Journal
- 2019
Several unidentified infrared emission bands (UIBs) have been assigned to neutral C60 molecules present in circumstellar and interstellar environments. However, due to the similarity of the infrared…
The Formation of Formaldehyde on Interstellar Carbonaceous Grain Analogs by O/H Atom Addition
- Physics, Chemistry
- 2017
An understanding of possible scenarios for the formation of astrophysically relevant molecules, particularly complex organic molecules, will bring us one step closer to the understanding of our…
Growth and Destruction of PAH Molecules in Reactions with Carbon Atoms
- Chemistry, Physics
- 2017
A very high abundance of atomic carbon in the interstellar medium (ISM), and the high reactivity of these species toward different hydrocarbon molecules including benzene, raise questions regarding…
Complex Organic Interstellar Molecules
- Physics
- 2009
Of the over 150 different molecular species detected in the interstellar and circumstellar media, approximately 50 contain 6 or more atoms. These molecules, labeled complex by astronomers if not by…
Composite interstellar grains
- Physics
- 1989
The possibility that interstellar grains are composite collections of very small particles, loosely attached to one another, is investigated. The grains are assumed to include a substantial…