“Part of the Primordial Soup”

1995 ◽  
Vol 64 (1) ◽  
pp. 220-221
Author(s):  
Paul G. McDonough ◽  
Wilfried Feichtinger
Keyword(s):  
Author(s):  
Ognjen Miljanic ◽  
Thamon Puangsamlee

Complex mixtures are found in biological and petrochemical feedstocks, and in the primordial soup implicated in the origins of life. Reacting individual compounds within these mixtures is challenging because of the difficulty in controlling the chemoselectivity of such reactions. We show that the selectivity of imine oxidation can be controlled within doubly dynamic combinatorial libraries, wherein two coupled equilibria determine whether the most oxidizable aldehyde precursor is made available to the oxidant or sequestered away from it. Under the slow oxidation conditions, the most electron-rich precursor can traverse the shallow energy landscape and its oxidation product dominates the final mixture. Faster oxidation captures the imine mixture composition, favoring the products derived from electron poorer push-pull imines. <br>


2019 ◽  
Vol 116 (12) ◽  
pp. 5387-5392 ◽  
Author(s):  
Andrew J. Surman ◽  
Marc Rodriguez-Garcia ◽  
Yousef M. Abul-Haija ◽  
Geoffrey J. T. Cooper ◽  
Piotr S. Gromski ◽  
...  

Many approaches to the origin of life focus on how the molecules found in biology might be made in the absence of biological processes, from the simplest plausible starting materials. Another approach could be to view the emergence of the chemistry of biology as process whereby the environment effectively directs “primordial soups” toward structure, function, and genetic systems over time. This does not require the molecules found in biology today to be made initially, and leads to the hypothesis that environment can direct chemical soups toward order, and eventually living systems. Herein, we show how unconstrained condensation reactions can be steered by changes in the reaction environment, such as order of reactant addition, and addition of salts or minerals. Using omics techniques to survey the resulting chemical ensembles we demonstrate there are distinct, significant, and reproducible differences between the product mixtures. Furthermore, we observe that these differences in composition have consequences, manifested in clearly different structural and functional properties. We demonstrate that simple variations in environmental parameters lead to differentiation of distinct chemical ensembles from both amino acid mixtures and a primordial soup model. We show that the synthetic complexity emerging from such unconstrained reactions is not as intractable as often suggested, when viewed through a chemically agnostic lens. An open approach to complexity can generate compositional, structural, and functional diversity from fixed sets of simple starting materials, suggesting that differentiation of chemical ensembles can occur in the wider environment without the need for biological machinery.


2009 ◽  
Vol 160 (7) ◽  
pp. 437-440 ◽  
Author(s):  
Mario Vaneechoutte ◽  
Renato Fani

2016 ◽  
Vol 13 (115) ◽  
pp. 20151086 ◽  
Author(s):  
Andreas Wagner ◽  
Scott Ortman ◽  
Robert Maxfield

Standards are specifications to which the elements of a technology must conform. Here, we apply this notion to the biochemical ‘technologies' of nature, where objects like DNA and proteins, as well as processes like the regulation of gene activity are highly standardized. We introduce the concept of standards with multiple examples, ranging from the ancient genetic material RNA, to Palaeolithic stone axes, and digital electronics, and we discuss common ways in which standards emerge in nature and technology. We then focus on the question of how standards can facilitate technological and biological innovation. Innovation-enhancing standards include those of proteins and digital electronics. They share common features, such as that few standardized building blocks can be combined through standard interfaces to create myriad useful objects or processes. We argue that such features will also characterize the most innovation-enhancing standards of future technologies.


2010 ◽  
Vol 10 (2) ◽  
pp. 83-98 ◽  
Author(s):  
Carl H. Gibson ◽  
Rudolph E. Schild ◽  
N. Chandra Wickramasinghe

AbstractThe origin of life and the origin of the Universe are among the most important problems of science and they might be inextricably linked. Hydro-gravitational-dynamics cosmology predicts hydrogen–helium gas planets in clumps as the dark matter of galaxies, with millions of planets per star. This unexpected prediction is supported by quasar microlensing of a galaxy and a flood of new data from space telescopes. Supernovae from stellar over-accretion of planets produce the chemicals (C, N, O, P, etc.) and abundant liquid-water domains required for first life and the means for wide scattering of life prototypes. Life originated following the plasma-to-gas transition between 2 and 20 Myr after the big bang, while planetary core oceans were between critical and freezing temperatures, and interchanges of material between planets constituted essentially a cosmological primordial soup. Images from optical, radio and infrared space telescopes suggest life on Earth was neither first nor inevitable.


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