Skip to content
DraconiticResearch
Search Sources API
178,970 studies31 sourcesUpdated 55 min ago
Peer-reviewedCC BY 4.0Communications Chemistry

Approaching life in a test tube with prebiotic chemistry

Abstract

The emergence of life on our planet occurred somewhere before 3.48 billion years ago, and was predated by a poorly defined period of appearance and accumulation of chemical intermediates commonly known as biomolecules – which includes amino acids, lipids, sugars and components of genetic polymers. While no fossils are known to science from that period of Earth’s development, prebiotic chemistry tried to experimentally answer the question: which chemical processes, and under which conditions, could provide our planet with biomolecules in sufficient quantity and structural diversity to enable spontaneous life formation. Here, we present a chronological overview of the hypotheses that have driven the development of prebiotic chemistry, and of seminal experiments which were intended to prove or disprove these hypotheses.

Related

  1. Origin-of-life chemistry is a problem of chemical composability
    Hengyue Xu
    ChemRxivPreprintCC BYGeneral astronomyChemRxiv
  2. Phosphorus Chemistry and the Origin of Life: From N-Phosphoryl Amino Acid to Protocell.
    Jianxi Ying, Yan Liu, Songsen Fu +2
    Accounts of chemical researchPeer-reviewedCC BY-NC-NDFull textGeneral astronomyEurope PMC
  3. Fractal Colonization of Prebiotic Niches: Mechanical Budding of Nano-vesicles and Kinetic Resource Depletion as an Oncological Atavism
    Peter Mikuláš
    ChemRxivPreprintCC BYFull textGeneral astronomyChemRxiv
  4. First Experimental Evaluation of Stray Light Noise Modeling of kilometers-long Beam Tube Arms of Gravitational Wave Detectors
    Emilia Chick, Timothy O'Hanlon, Hiro Yamamoto +3
    arXivPreprintCC BY 4.0Full textInstrumentation & methodsarXiv
  5. Collisionless stationary states of a stratified plasma in an expanding magnetic tube with stochastic heating
    Luca Barbieri, Pascal Démoulin, Daniel Verscharen
    arXivPreprintCC BY 4.0Full textSolar & stellar physicsPlasma physicsarXiv
BibTeX
@article{pianowski2026approaching,
  title = {{Approaching life in a test tube with prebiotic chemistry}},
  author = {Zbigniew L. Pianowski},
  journal = {Communications Chemistry},
  year = {2026},
  month = oct,
  doi = {10.1038/s42004-026-02257-3},
  url = {https://www.nature.com/articles/s42004-026-02257-3},
  note = {CC BY 4.0},
}
RIS
TY  - JOUR
TI  - Approaching life in a test tube with prebiotic chemistry
AU  - Zbigniew L. Pianowski
PY  - 2026
DA  - 2026/10/23
JO  - Communications Chemistry
DO  - 10.1038/s42004-026-02257-3
UR  - https://www.nature.com/articles/s42004-026-02257-3
AB  - The emergence of life on our planet occurred somewhere before 3.48 billion years ago, and was predated by a poorly defined period of appearance and accumulation of chemical intermediates commonly known as biomolecules – which includes amino acids, lipids, sugars and components of genetic polymers. While no fossils are known to science from that period of Earth’s development, prebiotic chemistry tried to experimentally answer the question: which chemical processes, and under which conditions, could provide our planet with biomolecules in sufficient quantity and structural diversity to enable spontaneous life formation. Here, we present a chronological overview of the hypotheses that have driven the development of prebiotic chemistry, and of seminal experiments which were intended to prove or disprove these hypotheses.
SN  - 2399-3669
ER  -