Insoluble organic matter in chondrites: Archetypal melanin-like PAH-based multifunctionality at the origin of life?

Insoluble organic matter Melanins Polycyclic aromatic hydrocarbons (PAHs) Primordial multifunctional organic entity (PRiME)

Journal

Physics of life reviews
ISSN: 1873-1457
Titre abrégé: Phys Life Rev
Pays: Netherlands
ID NLM: 101229718

Informations de publication

Date de publication:
07 2021
Historique:
received: 12 03 2021
accepted: 12 03 2021
pubmed: 29 3 2021
medline: 15 12 2021
entrez: 28 3 2021
Statut: ppublish

Résumé

An interdisciplinary review of the chemical literature that points to a unifying scenario for the origin of life, referred to as the Primordial Multifunctional organic Entity (PriME) scenario, is provided herein. In the PriME scenario it is suggested that the Insoluble Organic Matter (IOM) in carbonaceous chondrites, as well as interplanetary dust particles from meteorites and comets may have played an important role in the three most critical processes involved in the origin of life, namely 1) metabolism, via a) the provision and accumulation of molecules that are the building blocks of life, b) catalysis (e.g., by templation), and c) protection of developing life molecules against radiation by excited state deactivation; 2) compartmentalization, via adsorption of compounds on the exposed organic surfaces in fractured meteorites, and 3) replication, via deaggregation, desorption and related physical phenomena. This scenario is based on the hitherto overlooked structural and physicochemical similarities between the IOM and the dark, insoluble, multifunctional melanin polymers found in bacteria and fungi and associated with the ability of these microorganisms to survive extreme conditions, including ionizing radiation. The underlying conceptual link between these two materials is strengthened by the fact that primary precursors of bacterial and fungal melanins (collectively referred to herein as allomelanins) are hydroxylated aromatic compounds like homogentisic acid and 1,8-dihydroxynaphthalene, and that similar hydroxylated aromatic compounds, including hydroxynaphthalenes, figure prominently among possible components of the organic materials on dust grains and ices in the interstellar matter, and may be involved in the formation of IOM in meteorites. Inspired by this rationale, a vis-à-vis review of the properties of IOM from various chondrites and non-nitrogenous allomelanin pigments from bacteria and fungi is provided herein. The unrecognized similarities between these materials may pave the way for a novel scenario at the origin of life, in which IOM-related complex organic polymers delivered to the early Earth are proposed to serve as PriME and were preserved and transformed in those primitive forms of life that shared the ability to synthesize melanin polymers playing an important role in the critical processes underlying the establishment of terrestrial eukaryotes.

Identifiants

pubmed: 33774429
pii: S1571-0645(21)00013-0
doi: 10.1016/j.plrev.2021.03.002
pii:
doi:

Substances chimiques

Cosmic Dust 0
Melanins 0
Organic Chemicals 0

Types de publication

Journal Article Research Support, Non-U.S. Gov't Review

Langues

eng

Sous-ensembles de citation

IM

Pagination

65-93

Commentaires et corrections

Type : CommentIn
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Informations de copyright

Copyright © 2021 Elsevier B.V. All rights reserved.

Déclaration de conflit d'intérêts

Declaration of Competing Interest The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

Auteurs

Marco d'Ischia (M)

Department of Chemical Sciences, University of Naples Federico II, Via Cintia 4, 80126 Naples, Italy. Electronic address: dischia@unina.it.

Paola Manini (P)

Department of Chemical Sciences, University of Naples Federico II, Via Cintia 4, 80126 Naples, Italy.

Zita Martins (Z)

Centro de Química Estrutural and Departamento de Engenharia Química, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais 1, 1049-001 Lisboa, Portugal.

Laurent Remusat (L)

Institut de minéralogie, de physique des matériaux et de cosmochimie, UMR CNRS 7590, Sorbonne Université, Muséum National d'Histoire Naturelle, 61 rue Buffon, 75005 Paris, France.

Conel M O'D Alexander (CM)

Earth and Planets Laboratory, Carnegie Institution for Science, 5241 Broad Branch Road, NW Washington, DC 20015-1305, USA.

Cristina Puzzarini (C)

Department of Chemistry "Giacomo Ciamician", University of Bologna, Via F. Selmi 2, Bologna, I-40126, Italy.

Vincenzo Barone (V)

Scuola Normale Superiore, Piazza dei Cavalieri 7, Pisa, I-56126, Italy.

Raffaele Saladino (R)

Biological and Ecological Sciences Department (DEB), University of Tuscia, Via S. Camillo de Lellis 01100 Viterbo, Italy.

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Classifications MeSH