Closure of Earth’s biosphere: evolution and current state

Potential of living organisms. Stages of the formation of the biosphere in the context of closure and possible approaches to resolving the paradox. The effect of stoichiometric constraints on the formation of closed material flow in simple ecosystems.

Рубрика Биология и естествознание
Вид статья
Язык английский
Дата добавления 13.04.2022
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Closure of Earth's biosphere: evolution and current state

S.I. Bartsev, A.G. Degermendzhi, A.B. Sarangova

Annotation

The existence of the biosphere is determined by the presence of a constant circulation of substances, carried out by a highly branched trophic network of mainly closed material loops. How this largely selfcontained system formed remains unclear. The theory of evolution cannot help answer this question since the closure of the biosphere is not an adaptive trait of an individual - this is the essence of the Vernadsky-Darwin paradox. The present paper discusses stages of the formation of the biosphere in the context of closure - a key property and parameter of the biosphere - and possible approaches to resolving the paradox. The authors assume that the appearance of the first living organisms did not mean the appearance of the biosphere as a system of interacting components. The formation of the biosphere in the true sense of the word was associated with the appearance ofpredation approximately 500 million years ago and the emergence of a highly branched trophic network. The authors obtain simple estimates showing that, on the one hand, living organisms are potentially capable of changing their environment at the global level in a negligible geological time period but, on the other hand, are capable of maintaining an accurate balance of global material cycling for several tens of thousands of years. A simple model was used to show the effect of stoichiometric constraints on the formation of closed material flow in simple ecosystems and to demonstrate the need for increased diversity at trophic levels to overcome these stoichiometric constraints.

Keywords: Vernadsky-Darwin paradox, biosphere origin, biosphere closure formation.

Аннотация

Замкнутость земной биосферы: эволюция и текущее состояние

С.И. Барцев А.Г. Дегерменджи, А.Б. Сарангова

Существование биосферы определяется наличием постоянного круговорота веществ, осуществляемого высокоразветвленной трофической сетью, с высокой степенью замкнутости вещественных потоков. Каким образом была сформирована столь согласованная система с высоким уровнем замкнутости, остается неясным. Простое обращение к теории эволюции нам помочь не может, поскольку замкнутость биосферы не является приспособительным признаком особи - в этом суть парадокса Вернадского-Дарвина. В статье обсуждаются этапы формирования биосферы в контексте замкнутости - ключевого свойства и параметра биосферы, а также обсуждаются подходы к разрешению парадокса. Выдвинут тезис о том, что появление первых живых организмов не означает появления биосферы как системы взаимодействующих компонентов. Говорить о биосфере в полном смысле этого слова можно после появления хищничества около 500 млн лет назад и возникновения разветвленной трофической сети. Приведены простые оценки, показывающие, что, с одной стороны, живые организмы потенциально способны изменить среду обитания на глобальном уровне за ничтожное по геологическим масштабам время. Но, с другой стороны, они десятки тысяч лет способны обеспечивать точный баланс глобального круговорота веществ. На простой модели показано влияние стехиометрических ограничений на возможность формирования замкнутого потока веществ в простых экосистемах и продемонстрирована необходимость увеличения разнообразия на трофических уровнях для преодоления этих стехиометрических ограничений.

Ключевые слова: парадокс Вернадского-Дарвина, происхождение биосферы, формирование замкнутости биосферы.

Introduction

The generally accepted broad definition of the biosphere as the zone of life on Earth is descriptive (morphological) and cannot explain the origin of its main property - closure. To discuss the properties of the biosphere, it should be considered as a system consisting of certain elements (components) and interactions between them. A population of organisms represents a relatively homogeneous component of the biosphere. We consider one of the most important properties of the population, using a school task for illustration purposes.

Potential of living organisms: simple estimates

biosphere ecosystem living organism

Let one bacterium occupy a volume of approximately one cubic micrometer and divide into two identical cells every hour. After 35 hours, the offspring of one bacterium fill a one-liter jar. The question is as follows: How long does it take the bacteria to fill half the jar? The answer is almost obvious - 34 hours.

We continue to solve the tasks. Suppose that an ancient bacterium on ancient Earth can feed on air (hardly an unrealistic assumption if it performs photosynthesis and the concentration of carbon dioxide in the atmosphere is high) and, similar to the bacterium from the previous task, it divides into two cells every hour. The question is as follows: After what time will the offspring of this bacterium cover the globe with a one-meter-thick layer? One can make rather simple calculations and find that the required time is approximately 86 hours, or 3.6 days. An additional question is as follows: After what time will the offspring cover the globe with a layer 10 km thick? The answer is approximately 100 hours, or slightly more than four days.

These simple examples illustrate the potential for living systems to reproduce in the absence of limiting factors. If there is no resource deficiency nor any other limitations, the results of the vital activity of living organisms will be evident at the global level instantaneously at a geological time scale. A self-replicating system without limitations very quickly consumes all the available resources of a finite, albeit arbitrarily large, volume and stops growing. The following question arises: How has life capable of consuming all available planetary resources in a short period of time managed to survive on Earth for 4 billion years? Find the answer in the following task.

The carbon cycle

The annual net primary production from photosynthesis of terrestrial vegetation is approx i match 60 СПС; in other words, this amount of carbon is rumored from Fartlbs atmosphere and transferred to biomass.

At the same time, since the beginning of the Industrial Revolution in the 18th century, the atmospheric CO2 concentration has been steadily increasing, and the biosphere cannot bring it back to its previous level. This indicates that the level reached during the development of the biosphere resulted from the adjustment of the components of the global carbon cycle in response to each other rather than a permanent mechanism capable of compensating for the flow of carbon from the outside.

The closure of the biosphere and the Vernadsky-Darwin paradox

These simple calculations clearly show that the key feature of the biosphere that ensures its long-term existence is the balance of the material cycles therein, which is termed “closure”. In thermodynamics, a closed system is a system that exchanges only energy with the environment. Ecological closure, in addition to the absence of material exchange with the environment, suggests the presence of an internal material cycle carried out by living organisms.

In accordance with V.I. Vernadsky's ideas, life in Earth's biosphere can exist only because cyclic transformations of substances carried out by all living organisms using the energy of the Sun are largely closed loops. Whatever is produced by an organism, including itself, is consumed by other organisms, and the cycle continues. Thus, a continuous cyclic network of metabolic chemical transformations is established in the biosphere, and its functioning enables living organisms to use the same atoms of chemical elements repeatedly.

Here, we face a paradox, which was named the Vernadsky paradox by the authors (Barlow, Volk, 1990). The authors formulated it in the form of two questions: “How can an aggregate of opensystem life forms evolve and persist for billions of years within a global system that is largely closed to matter influx and outflow?” and “How do the inputs and outputs of myriad open systems form a life mesh in such a way that material closure as a boundary condition of the planet does not destroy the organized subsystems?”

If we accept that the current highly closed state of the biosphere, with which it entered the Industrial Revolution, is the result of its evolutionary and ecological development, then this paradox can be formulated as follows: “The closure of the biosphere is not an adaptive trait of an individual.” Indeed, natural selection leads to the survival of an individual that captures more resources and leaves behind a larger number of viable offspring; in other words, natural selection leads to the success of an organism with an advantage that provides gains here and now. The consequences of breaking the closure will become evident much later than the immediate results of selection. As the closure of the biosphere takes place along with natural selection, whose direction is orthogonal to if not the opposite of that of biosphere closure, an extension to the name of this paradox suggests itself - the Vernadsky-Darwin paradox.

Energy epochs of life on Earth

To propose a possible solution to this paradox, let us consider the history of the origin of the terrestrial biosphere. Very many published studies have been devoted to reconstructions of the history of Earth's biosphere based on existing geological and paleontological data (Lazcano, Miller, 1996; Russell et al., 2010; Lane et al., 2010; Dibrova et al., 2012; Sousa et al., 2013; Weiss et al., 2016; Lanier, Williams, 2017; Russell, Hall, 2006; Wachtershauser, 2006; Kitadai, Maruyama, 2018; Amenabar, Boyd, 2019), and there is no sense in restating them here. One of the more interesting studies (Judson, 2017) divides the development of the biosphere into four epochs differing in the energy source available to living beings: 1) geochemical energy; 2) solar energy; 3) energy from oxidative phosphorylation; and 4) energy from the consumption of living flesh, or predation. We trace the history of the biosphere in the context of the formation of its closure, relating the change in the closure level to energy epochs. In what follows, all factual material without references will be taken from the previously mentioned work (Judson, 2017).

The failure of the heterotrophic hypothesis of the origin of life

The very first question is as follows: When did the biosphere appear, not as a place where living organisms exist, but rather as a system of interacting organisms, populations, and ecosystems? Most experts are inclined to believe that life on Earth originated under anaerobic conditions around the hydrothermal sources that supply energy for chemoautotrophic synthesis (Lazcano, Miller, 1996; Judson, 2017; Russell, Hall, 2006; Amenabar, Boyd, 2019). An alternative hypothesis, suggesting the heterotrophic nature of the first organisms, encounters a number of objections.

First, there are no data suggesting the presence of a very large amount of organic matter in the ocean of the ancient Earth (Lazcano, Miller, 1996).

Second, the organic broth resulting from abiogenic synthesis should be a very heterogeneous racemic mixture of various organic substances. The digestive system of modern heterotrophs is “tuned” to a highly specific type of organic matter (for example, proteins, fats, and carbohydrates). There are corresponding metabolic pathways for the consumption of these types of matter. The assumption that the primary organism contained an equally diverse set of metabolic pathways for utilizing organic matter in the broth seems improbable. If the organism had a limited number of metabolic pathways for utilizing the respective substrates, then because of the expected small amounts of these substrates, it would suffer a constant, acute, and possibly fatal nutrient deficiency.

Third, even if an ocean with organic substances did exist and primary organisms were able to utilize them, the solution to the task considered at the beginning of this paper suggests that they would be quickly consumed and that heterotrophic organisms would die out or their biomass growth would be terminated by an increase in the concentration of metabolites - fermentation products.

In any case, if the heterotrophic hypothesis were valid, no closure of the matter flow would occur, and thus, there would be no biosphere as a system of interactions.

Origin of life - no biosphere yet

The scenario of chemoautotrophic generation of life (Lazcano, Miller, 1996; Judson, 2017; Russell, Hall, 2006; Amenabar, Boyd, 2019) suggests isolated oases of life around hydrothermal springs. There was virtually no interaction between them because of the limited availability of resources. The possibility for anoxygenic photosynthesis is not a significant factor, as there must be reduced substrates in the medium - hydrogen sulfide, thiosulfate, organic compounds, or molecular hydrogen - to perform it. Therefore, it could be carried out only around the sources of these substrates.

Thus, the origin of life does not mean the emergence of the biosphere as a system of interacting components. The level of closure of matter flows was globally minimal, and the conditions corresponding to the Vernadsky- Darwin paradox had not yet arisen.

The Great Oxidation - the birth of the biosphere

The appearance of cyanobacteria, which are capable of oxygenic photosynthesis, dates to approximately 2.5 billion years ago. This event started the period called the Great Oxidation. The oxygen concentration began to rise from the initial 10-5-th fraction of the current atmospheric oxygen level, reaching 0.1-1% of the current level by ~2 billion years ago. However, a tricky question arises regarding the Great Oxidation. Genetic, fossil and geochemical data confirm that cyanobacteria appeared at least 300 million years before the Great Oxidation event. However, if cyanobacteria appeared hundreds of millions of years before the Great Oxidation event, why did the accumulation of oxygen take so long?

One hypothesis (Goldblatt et al., 2006) is that the oxygen released by cyanobacteria was associated with substances present in the atmosphere and in the ocean of early Earth (hydrogen, methane, and ferrous iron). However, as shown in the solutions of the school tasks above, if the growth of cyanobacteria had not been limited by any factor, the cyanobacteria would have quickly produced an amount of oxygen sufficient to oxidize all available oxidizable substances on Earth.

A better-substantiated hypothesis is that the growth rate of cyanobacteria was limited by a phosphorus deficiency (Kipp, Stueken, 2017). Here, we have a very important factor for the closure of material flows - stoichiometric constraints. According to this hypothesis, phosphorus determines marine biological productivity on a geological time scale. The emergence of aerobic photosynthesis triggered rapid absorption of carbon dioxide and, hence, rapid biomass production. Due to the low oxygen concentration, the demineralization rate was insignificant, and deposition of dead biomass and the phosphorus contained therein occurred. However, despite the consistency and validity of the hypothesis, some ambiguities remain. For example, if the proposed scenario were true, after the appearance of cyanobacteria and the onset of photosynthesis, the phosphorus concentration should have dropped dramatically to almost zero, but no evidence of this drop has been presented.

Another explanation is that with the emergence of oxygenic photosynthesis, the need to develop protection against oxygen and its reactive species arose. In other words, the time interval between the appearance of cyanobacteria and the Great Oxidation event might have been associated with the need to create a system of protection against their own product. Each of the reasons listed above (and unknown ones as well) might have contributed to the delay.

As long as the transition processes associated with the global change in conditions on early Earth occurred, the level of closure of matter flows was close to zero. During the Great Oxidation, the biosphere was generated. The global change in atmospheric gas composition simultaneously influenced all organisms in contact with the atmosphere, and instead of separate and virtually noninteracting chemoautotrophic oases, an integrated ecological system developed. Of the four energy epochs of life on Earth mentioned above, the formation of the biosphere corresponds to the end of the second and beginning of the third energy epochs - the transition to oxidative phosphorylation.

During the Great Oxidation and the drop in carbon dioxide concentration from ~7000 ppm to ~250 ppm (at the end of the Paleozoic, the concentration increased approximately tenfold), approximately 20000 GtC of organic residues was deposited. At the same time, the oxygen concentration in the atmosphere reached ~2% of the current atmospheric concentration; in other words, it rose slightly above the Pasteur point, where oxidative phosphorylation became energetically favorable.

Bacterial mats as local ecosystems - an “unconsolidated” biosphere

Then, for 1.5 billion years, the oxygen concentration in Earth's atmosphere did not change, suggesting that the rate of photosynthesis and the mineralization of organic matter conducted by decomposers were precisely balanced. Since the atmospheric o?q^gen concentration was only slightly above Pasteur's point and there was no increased organic matter deposition, the elevated oxygen conccntrationwas presumably created in the bull? of bacterial mats, ensuring rapid decomposition of dead biomass and a supply of mineral nutrients to phototrop hs. This significantly accelerated cyclic pro ce sscs. while minerals could still be assimilated from the environment. The spccific growth rate of bacterial communities with a locally elevated oxygen concentration became higher, and they consumed external resourc es quicke r, gaini ng a competitive advantage (Ab ed, 2010; Mo rris et al., 2008). The bacterial communities? that enabled more rapid material cyclingwon.

Bacterial mats and the Vernadsky-Darwin paradox

Consider the possibility (conditions) of resolving the Vmrn^ky-Darwin paradox inside closed bacterial systems. Todo this, we construct a model of such a system, taking into account the stoichiometric proportions of the two nutrients (for example, nitrogen and phosphorus) in the biomass of autotrophic and heterotrophic bacteria.

Inequality relations usually occur in nature. Thus, a simple model suggests the hypothesis that in closed systems, the trophic level should always consist of several types. In this model, the number of different heterotrophs should be no fewer than the number of nutrients.

In the model of a bacterial mat, the Vernadsky-Darwin paradox can be resolved in another way - the system must contain two autotrophs and one heterotroph capable of selecting the prey, i.e., a predator (Saltykov et al., 2012). Therefore, we move to the fourth energy epoch of the development of life on Earth (Judson, 2017) - consumption of living flesh, or predation.

It is important that complex food networks with many types of consumers were absent on Earth until approximately 550 million years ago, when the first animals that eat animals appeared. It seems that their appearance led to the rapid diversification of animal life. In geological terms, the thriving of animals had at least four major impacts on the biosphere.

First, the evolution of predators quickly led to the development of armor - scales, thorns, and shells made of materials such as calcite and silica. This development ultimately led to extremely large deposits of materials such as radiolarian chert, limestone, shell rock and chalk as well as changes in ocean chemistry.

Second, animals produce feces, which has a significant effect on the way nutrients are distributed globally. For example, sperm whale feces transports iron from the deep sea to the upper layer of the ocean, and the feces of birds such as cormorants caries nutrients from the ocean to dry land, sometimes in substantial quantities.

The third geological impact of animals is associated with their ability to dig in. Simple horizontal holes appear in the fossil record approximately 555 Ma. Widespread digging creates the mixing of sediments, known as bioturbation: it redistributes nutrients and sifts, irrigates and aerates sediments and soil.

Finally, the fourth major impact of flesheating forms arises from bioturbation, feces and the evolution of armor: the reorganization of Earth's biogeochemical cycles (Canfield et al., 2006; Boyle et al., 2014; Logan et al., 1995).

The Carboniferous period - the transition to the modern state of the biosphere

The increase in the number of available energy sources led to the creation of a much more complex biosphere, in which the interactions between the components became very close. The last severe imbalance in matter flow occurred during the Carboniferous period, which ended 300 million years ago. The atmospheric oxygen concentration at that time reached 35%, which is attributed to the appearance of lignin in land vegetation, which sharply lowered the decomposition rate of dead organic matter and contributed to the absorption of fallen plants by swamps and the subsequent formation of coal deposits.

The biosphere finally matured and became highly closed and systemic, in every sense, only 300 million years ago. The great diversity of organisms and the ramification of the food network of the biosphere facilitated the closure of matter flows and prevented the formation of so-called dead-locks, i.e., substances that are not consumed by other organisms. The fine adjustment of the food network could have occurred through adaptive metabolism, as discussed in a study by Saltykov et al. (2012), finally solving the Vernadsky-Darwin paradox.

Conclusion

When we consider the biosphere as a system of interacting components - populations and local ecosystems - we should recognize that the origin of life on ancient Earth did not mean the origin of the biosphere. The biosphere was born during the stage of photosynthesis emergence, when living beings began to have a global impact on each other. A full-fledged “mature” biosphere - a system with intense interactions between components - did not form until 300 million years ago. At the same time, high closure of matter flows resulted from the formation of an extensive network of trophic interactions and metabolic flexibility of individuals.

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