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Prebiotic chemical origin of biomolecular complementarity
Y Sajeev1,2
1Theoretical Chemistry Section, Bhabha Atomic Research Centre, Mumbai, India. sajeevy@barc.gov.in.
Early Earth
Area of Science:
- Astrobiology
- Origin of Life Studies
- Prebiotic Chemistry
Background:
- The early Earth lacked a protective ozone layer, exposing it to intense UV radiation and very low energy electrons (vLEEs).
- This harsh environment necessitated the proliferation of molecules intrinsically stable against these damaging agents.
- Such stable molecules could have evolved into the complex building blocks of life.
Purpose of the Study:
- To investigate the stability of nucleobases and their complementary pairs under early Earth conditions.
- To determine if complementary base pairing enhances molecular stability against UV photons and vLEEs.
- To understand the role of base pairing in the chemical evolution of life's precursors.
Main Methods:
- Examined the inherent stability of individual nucleobases.
- Assessed the stability of complementary nucleobase pairs.
- Simulated the effects of shortwave UV photons and vLEEs on nucleobases and their pairs.
Main Results:
- Nucleobases exhibit enhanced stability when present as complementary pairs.
- Complementary base pairing significantly increases resistance to UV photons and vLEEs.
- This enhanced stability suggests a mechanism for nucleobase survival and evolution.
Conclusions:
- Complementary base pairing was crucial for nucleobase survival and proliferation on the early Earth.
- Base pairing provided essential molecular stability in a harsh prebiotic environment.
- This stability is a key aspect of chemical evolution leading to the origin of life.
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