Integrating Chemistry, Geology, and Life’s Origin Coauthored with Bruce Damer

Author(s):  
David W. Deamer

Chapter 8 recalled John Platt’s recommendation that testing alternative hypotheses is a preferred way to perform research rather than focusing on a single hypothesis. Karl Popper proposed an additional way to evaluate research approaches, which is that a strong hypothesis is one that can be falsified by one or more crucial experiments. This chapter proposes that life can begin with chance ensembles of encapsulated polymers, some of which happen to store genetic information in the linear sequences of their monomers while others catalyze polymerization reactions. These interact in cycles in which genetic polymers guide the synthesis of catalytic polymers, which in turn catalyze the synthesis of the genetic polymers. At first, the cycle occurs in the absence of metabolism, driven solely by the existing chemical energy available in the environment. At a later stage, other polymers incorporated in the encapsulated systems begin to function as catalysts of primitive metabolic reactions described in Chapter 7. The emergence of protocells with metabolic processes that support polymerization of self-reproducing systems of interacting catalytic and genetic polymers marks the final step in the origin of life. The above scenario can be turned into a hypothesis if it can be experimentally tested— or falsified, as described in the epigraph. The goal of falsification tends to be uncomfortable for active researchers. It’s a very human tendency to be delighted with a creative new idea and want to prove it correct. This can be such a strong emotion that some fall in love with their idea and actually hesitate to test it. They begin to dislike colleagues who are critical and skeptical. However, my experience after 50 years of active research is that we need to think of our ideas as mental maps and expect that most of them will not match the real world very well. And so, I say to my students, “When you have a new idea it’s OK to enjoy it and share it with others, but then you must come up with an experiment that lets you discard it.

2020 ◽  
Author(s):  
Stephanie J. Zhang ◽  
Daniel Duzdevich ◽  
Jack W. Szostak

ABSTRACTThe nonenzymatic replication of ribonucleic acid (RNA) oligonucleotides may have enabled the propagation of genetic information during the origin of life. RNA copying can be initiated in the laboratory with chemically activated nucleotides, but continued copying requires a source of chemical energy for in situ nucleotide activation. Recent work has illuminated a potentially prebiotic cyanosulfidic chemistry that activates nucleotides, but its application to nonenzymatic RNA copying remains a challenge. Here we report a novel pathway that enables the activation of RNA nucleotides in a manner that is compatible with template-directed nonenzymatic polymerization. We show that this pathway selectively yields the reactive imidazolium-bridged dinucleotide intermediate required for nonenzymatic template-directed RNA copying. Our results will enable more realistic prebiotic chemical simulations of RNA copying based on continuous in situ nucleotide activation.


2017 ◽  
Vol 13 ◽  
pp. 620-624 ◽  
Author(s):  
David Deamer

In origins of life research, it is important to understand the difference between conjecture and hypothesis. This commentary explores the difference and recommends alternative hypotheses as a way to advance our understanding of how life can begin on the Earth and other habitable planets. As an example of how this approach can be used, two conditions have been proposed for sites conducive to the origin of life: hydrothermal vents in salty seawater, and fresh water hydrothermal fields associated with volcanic landmasses. These are considered as alternative hypotheses and the accumulating weight of evidence for each site is described and analyzed.


1997 ◽  
Vol 161 ◽  
pp. 419-429 ◽  
Author(s):  
Antonio Lazcano

AbstractDifferent current ideas on the origin of life are critically examined. Comparison of the now fashionable FeS/H2S pyrite-based autotrophic theory of the origin of life with the heterotrophic viewpoint suggest that the later is still the most fertile explanation for the emergence of life. However, the theory of chemical evolution and heterotrophic origins of life requires major updating, which should include the abandonment of the idea that the appearance of life was a slow process involving billions of years. Stability of organic compounds and the genetics of bacteria suggest that the origin and early diversification of life took place in a time period of the order of 10 million years. Current evidence suggest that the abiotic synthesis of organic compounds may be a widespread phenomenon in the Galaxy and may have a deterministic nature. However, the history of the biosphere does not exhibits any obvious trend towards greater complexity or «higher» forms of life. Therefore, the role of contingency in biological evolution should not be understimated in the discussions of the possibilities of life in the Universe.


1997 ◽  
Vol 161 ◽  
pp. 23-47 ◽  
Author(s):  
Louis J. Allamandola ◽  
Max P. Bernstein ◽  
Scott A. Sandford

AbstractInfrared observations, combined with realistic laboratory simulations, have revolutionized our understanding of interstellar ice and dust, the building blocks of comets. Since comets are thought to be a major source of the volatiles on the primative earth, their organic inventory is of central importance to questions concerning the origin of life. Ices in molecular clouds contain the very simple molecules H2O, CH3OH, CO, CO2, CH4, H2, and probably some NH3and H2CO, as well as more complex species including nitriles, ketones, and esters. The evidence for these, as well as carbonrich materials such as polycyclic aromatic hydrocarbons (PAHs), microdiamonds, and amorphous carbon is briefly reviewed. This is followed by a detailed summary of interstellar/precometary ice photochemical evolution based on laboratory studies of realistic polar ice analogs. Ultraviolet photolysis of these ices produces H2, H2CO, CO2, CO, CH4, HCO, and the moderately complex organic molecules: CH3CH2OH (ethanol), HC(= O)NH2(formamide), CH3C(= O)NH2(acetamide), R-CN (nitriles), and hexamethylenetetramine (HMT, C6H12N4), as well as more complex species including polyoxymethylene and related species (POMs), amides, and ketones. The ready formation of these organic species from simple starting mixtures, the ice chemistry that ensues when these ices are mildly warmed, plus the observation that the more complex refractory photoproducts show lipid-like behavior and readily self organize into droplets upon exposure to liquid water suggest that comets may have played an important role in the origin of life.


BMJ ◽  
1912 ◽  
Vol 2 (2711) ◽  
pp. 1692-1692
Author(s):  
H. C. Bastian

1967 ◽  
Vol 101 (919) ◽  
pp. 223-231 ◽  
Author(s):  
Roger G. Hart

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