Atmospheric reaction systems as null-models to identify structural traces of evolution in metabolism
Petter Holme, Mikael Huss, Sang Hoon Lee

TL;DR
This study compares planetary atmospheric reaction systems with biological metabolism networks to identify structural traces of evolution, revealing that chemical constraints shape these networks more than evolutionary processes.
Contribution
It introduces atmospheric reaction systems as null-models for analyzing metabolic structure and highlights the influence of chemical constraints versus evolution in network organization.
Findings
Metabolic networks have more complex modular organization than atmospheric networks.
Degree distributions differ significantly between atmospheric and metabolic networks.
Chemical properties of molecules strongly influence network structure, overshadowing evolutionary effects.
Abstract
The metabolism is the motor behind the biological complexity of an organism. One problem of characterizing its large-scale structure is that it is hard to know what to compare it to. All chemical reaction systems are shaped by the same physics that gives molecules their stability and affinity to react. These fundamental factors cannot be captured by standard null-models based on randomization. The unique property of organismal metabolism is that it is controlled, to some extent, by an enzymatic machinery that is subject to evolution. In this paper, we explore the possibility that reaction systems of planetary atmospheres can serve as a null-model against which we can define metabolic structure and trace the influence of evolution. We find that the two types of data can be distinguished by their respective degree distributions. This is especially clear when looking at the degree…
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