• Order and Timing of Key Events: It
remains debated whether metabolic networks
predate genetic systems (“metabolism first”)
or vice versa (“genetics first”). It is possible
that partial, rudimentary versions of both
emerged in tandem, reinforcing each other’s
development (Di Rocco & Coons, 2018).
• Alternatives to RNA: Although RNA stands
out as a prime candidate for the first genetic
polymer, alternative nucleic-acid analogs
(like PNA, TNA, or GNA) cannot be ruled
out. Evidence suggests that these analogs
may polymerize more readily or be more
stable under certain conditions, which might
have preceded or co-existed with RNA
(Jeilani et al., 2016).
• Catalytic Efficiency and Fidelity: How did
early enzymatic activities maintain sufficient
fidelity for evolutionary progress without the
refined proofreading mechanisms seen in
modern DNA replication?
• Emergence of Homochirality: While
models of chiral amplification exist,
experimental demonstrations that replicate
the full transition from near-racemic mixtures
to predominantly homochiral biomolecules in
plausible conditions remain a work in
progress (Toxvaerd, 2018, 2019).
• Extraterrestrial Influences: Some theories
propose that organic precursors arrived via
meteoritic or cometary infall. If so, the early
Earth received a “head start” on complex
chemistry (Ershov, 2022). How significant
was this exogenous delivery compared to in
situ synthesis?
Addressing these questions will require an
interdisciplinary approach, combining geochemical
modeling, laboratory simulations of prebiotic
environments, and computational explorations of
vast chemical reaction networks. Additionally,
exploring extreme Earth environments (e.g., deep-
sea vents, hot springs, hyper-saline lakes) continues
to provide insights into how life can persist and
perhaps how it originated in habitats similar to those
of the early Earth.
8 CONCLUSIONS
Abiogenesis is a multifaceted process, not a singular
event. Its study spans the formation of small organic
molecules to the rise of self-replicating,
compartmentalized systems capable of Darwinian
evolution. Key themes identified in this discourse
include:
• Prebiotic Synthesis of Organic Molecules:
Early Earth conditions coupled with catalytic
minerals and various energy sources
produced amino acids, nucleobases, and other
critical monomers.
• Autocatalysis and Homochirality: Self-
sustaining reaction cycles (e.g., CompACs)
and the preferential establishment of one
molecular handedness likely set the
biochemical stage for higher complexity.
• Environmental Catalysts: Hydrothermal
vents, saline environments, and mineral
surfaces provided unique conditions for
concentrating reactants, stabilizing
intermediates, and accelerating key reactions.
• Energy Inputs: Solar radiation, geothermal,
and radioactive decay each supplied the
energetic “push” necessary for forming
increasingly complex and ordered structures.
• Molecular Evolution and Replication: The
emergence of self-replicating polymers (e.g.,
RNA, DNA) was a watershed moment,
enabling heredity and cumulative
evolutionary change.
• Compartmentalization: Protocells formed
from amphiphilic molecules—helping to
localize chemical networks, increase
efficiency, and protect nascent genetic and
metabolic machineries.
• Integration of Genetic and Metabolic
Systems: Early metabolic pathways and
genetic elements likely co-evolved, leading to
the intricate interplay that characterizes
modern cells.
Through these processes, life transitioned from
simple chemistry to complex, evolving biochemical
systems. The references cited illustrate the breadth
of experimental and theoretical research dedicated to
unveiling how matter organized itself into the living
forms that eventually spread across our planet.
Although myriad details await further clarification,
the converging picture is that abiogenesis was driven
by a synergy of geological, chemical, and physical
processes operating on a young Earth replete with
reactive environments and potent energy sources.
The implications of these findings extend far
beyond Earth: if these processes are not Earth-
specific but universal, then life may be a common
outcome wherever compatible environments exist.
Future investigations ranging from laboratory-based
origin-of-life simulations to the in-depth analysis of
other planetary bodies will continue to refine our