Origin of Life
Origin of Life
life
         life, living matter and, as such, matter that shows
                                                                            TABLE OF CONTENTS
         certain attributes that include responsiveness,
         growth, metabolism, energy transformation, and                       Introduction
         reproduction. Although a noun, as with other                         Definitions of life
         defined entities, the word life might be better cast                 Life on Earth
         as a verb to reflect its essential status as a process.              The origin of life
         Life comprises individuals, living beings, assignable
Streptococcus pyogenes
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               Mangroves (Rhizophora apiculata) at                                                     o
                low tide on the coast of Thailand.                                                     m
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         non of life can be approached in several ways: life as it is known and studied on
         planet Earth; life imaginable in principle; and life, by hypothesis, that might exist
         elsewhere in the universe (see extraterrestrial life). As far as is known, life exists
         only on Earth. Most life-forms reside in a thin sphere that extends about 23 km
         (14 miles) from 3 km (2 miles) beneath the bottom of the ocean to the top of
         the troposphere (lower atmosphere); the relative thickness is comparable to a
         coat of paint on a rubber ball. An estimated 10–30 million distinguishable
         species currently inhabit this sphere of life, or biosphere.
         Definitions of life
                                                     Much is known about life from points of view
                                                     reflected in the various biological, or “life,”
                                                     sciences. These include anatomy (the study of
                                                     form at the visible level), ultrastructure (the
                                                     study of form at the microscopic level),
                                                     physiology (the study of function), molecular
                             reed frog               biology and biochemistry (the study of form
                   Reed frog perched on a lily.      and function at chemical levels), ecology (the
                                                     study of the relations of organisms with their
         environments), taxonomy (the naming, identifying, and classifying of organisms),
         ethology (the study of animal behaviour), and sociobiology (the study of social
         behaviour). Specific sciences that participate in the study of life focus more
         narrowly on certain taxa or levels of observation—e.g., botany (the study of
         plants), lichenology (the study of lichens, leafy or crusty individuals composed of
         permanent associations between algae or photosynthetic bacteria and fungi),
         herpetology (the study of amphibians and reptiles), microbiology (the study of
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         bacteria, yeast, and other unicellular fungi, archaea, protists, viruses), zoology
         (the study of marine and land animals), and cytology (the study of cells).
         Although the scientists, technicians, and others who participate in studies of life
         easily distinguish living matter from inert or dead matter, none can give a
         completely inclusive, concise definition of life itself. Part of the problem is that
         the core properties of life—growth, change, reproduction, active resistance to
         external perturbation, and evolution—involve transformation or the capacity for
         transformation. Living processes are thus antithetical to a desire for tidy
         classification or final definition. To take one example, the number of chemical
         elements involved with life has increased with time; an exhaustive list of the
         material constituents of life would therefore be premature. Nonetheless, most
         scientists implicitly use one or more of the metabolic, physiological, biochemical,
         genetic, thermodynamic, and autopoietic definitions given below.
Metabolic
         Metabolic definitions are popular with biochemists and some biologists. Living
         systems are objects with definite boundaries, continually exchanging some
         materials with their surroundings but without altering their general properties,
         at least over some period of time. However, there are exceptions. There are
         frozen seeds and spores that remain, so far as is known, perfectly dormant. At
         low temperatures they lack metabolic activity for hundreds, perhaps thousands,
         of years but revive perfectly well upon being subjected to more clement
         conditions. A candle flame has a well-defined shape with a fixed boundary and
         is maintained by “metabolizing” its organic waxes and the surrounding
         molecular oxygen to produce carbon dioxide and water. Similar reactions,
         incidentally, occur in animals and plants. Flames also have a well-known capacity
         for growth. These facts underscore the inadequacy of this metabolic definition,
         even as they suggest the indispensable role of energy transformation to living
         systems. (See metabolism.)
Physiological
         Physiological definitions of life are popular. Life is defined as any system capable
         of performing functions such as eating, metabolizing, excreting, breathing,
         moving, growing, reproducing, and responding to external stimuli. But many
         such properties are either present in machines that nobody is willing to call alive
         or absent from organisms, such as the dormant hard-covered seed of a tree,
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Genetic
         All organisms on Earth, from the tiniest cell to the loftiest trees, display
         extraordinary powers. They effortlessly perform complex transformations of
         organic molecules, exhibit elaborate behaviour patterns, and indefinitely
         construct from raw materials in the environment more or less identical copies of
         themselves. How could systems of such staggering complexity and such
         stunning beauty ever arise? A main part of the answer, for which today there is
         excellent scientific evidence, was carefully chronicled by the English naturalist
         Charles Darwin in the years before the publication in 1859 of his epoch-making
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         organization (or decrease the net entropy) of the system. Thus, the universe
         taken as a whole is steadily moving toward a state of complete randomness,
         lacking any order, pattern, or beauty. This fate was popularized in the 19th
         century as the “heat death” of the universe.
         Living organisms are manifestly organized and at first sight seem to represent a
         contradiction to the second law of thermodynamics. Indeed, living systems
         might then be defined as localized regions where there is a continuous
         maintenance or increase in organization. Living systems, however, do not really
         contradict the second law. They increase their organization in regions of energy
         flow, and, indeed, their cycling of materials and their tendency to grow can be
         understood only in the context of a more general definition of the second law
         that applies to open as well as closed and isolated systems. In nature (except at
         cosmic scales, where gravity becomes a crucial factor), energy moves from being
         concentrated to being spread out; spontaneously occurring complex systems do
         not violate the second law but help energy spread out, thus producing entropy
         and reducing gradients.
         reduction between the energy of the hot Sun and the cooler space around it.
         Although life has not fully reduced the solar gradient, incorporation of carbon
         dioxide into chemoautotrophs and production of clouds by plants help keep
         Earth’s surface cooler than it would otherwise be, thereby helping to degrade
         the solar energy gradient.
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               impact on the composition and         life on Earth has arisen through replication,
               temperature of the atmosphere.
                                                     with thermodynamically favoured pathways
         being used by energy-transforming organisms.
         Autopoietic
         One of the difficulties in defining life is that the only example is life found on the
         third planet from the Sun. On Earth all life’s autopoietic systems require a supply
         of water in its liquid state for self-maintenance of their parts. Taken together, all
         transformations that underlie autopoiesis require six elements: carbon, nitrogen,
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The biosphere
                                Earth
                                                    biosphere, by definition the place where all
                                                    Earth’s life dwells, is a delight with its green,
                        The planet Earth.
                                                    wet contrast. Austrian geologist Eduard Suess
         invented the term biosphere to match the other envelopes of the planet: the
         atmosphere of gas; the hydrosphere of oceans, lakes, rivers, springs and other
         waters; and the lithosphere, or the solid rock surface of the outer portion of
         Earth. Yet it was the great Russian crystallographer and mineralogist Vladimir I.
         Vernadsky who brought the term into common parlance with his book of the
         same name. In The Biosphere (1926) Vernadsky outlines his view of life as a
         major geological force. Living matter, Vernadsky contends, erodes, levels,
         transports, and chemically transforms surface rocks, minerals, and other features
         of Earth. If the biosphere is the place where life is found, the biota (or the
         biomass as a whole) is the sum of all living forms: flora, fauna, and microbiota.
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         During the second half of the 20th century, study of the deep sea, the upper
         atmosphere, the Antarctic dry deserts, newly opened caves, sulfurous tunnels,
         and granitic rocks showed that Earth’s surface is vigorously inhabited in places
         that were unknown to Vernadsky and his colleagues. Vernadsky’s international
         school of thought ushered in the field of “biogeochemistry,” and chemists and
         geologists were recruited to consider life as a planetary phenomenon. But not
         until giant, mouthless, red-gilled tube worms were videographed in the late
         1970s and ’80s did the extent and the weirdness of Earth’s biota begin to be
         fathomed. Entire large ecosystems were recognized on the ocean’s bottom that
         live not by the usual plant photosynthesis but rather by chemolithoautotrophy,
         a kind of metabolism in which organisms make food from carbon dioxide using
         energy from the oxidation of sulfide, methane, or other inorganic compounds.
         These discoveries have led to a deeper understanding of life’s varied modes of
         nutrition and sources of energy. Bacterial symbionts living in the tissues of some
         polychaete worms (alvinellids) or pogonophora (such as Riftia pacytila) provide
         the animals with their total nutritional needs. The submarine ecosystems
         supported by bacteria thrive along the worldwide rift zones that extend along
         the borders of huge continental plates at the Mid-Atlantic Ridge, on the East
         Pacific Rise, at 21° north of the Equator off the coast of Baja California, Mex., and
         at a dozen other newly studied sites. By the beginning of the 21st century it had
         become abundantly clear that many life-forms and ecosystems remained
         unknown or under-studied. Those in the Siberian tundra, in the thickly forested
         portions of the Amazon River valley and its tributaries, at the tops of remote
         mountains and inside granitic rocks in temperate zones, and in the centre of
         Africa remain as inaccessible to most naturalists as they have been throughout
         history. The easily accessed woodlands and fields of well-lit land surfaces are
         another story.
         Vernadsky anticipated new discoveries of life inside hot springs and granitic
         rock. Although he qualified this statement by asserting that it would not hold for
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         Thus far, we have seen that the biosphere, by structure, composition, and physical
         makeup, is completely enclosed by the domain of life, which has so adapted itself to
         biospheric conditions that there is no place [on Earth] in which it is unable to manifest
         itself in one way or another.
         Although much is not known about life in the depths of the rocks and the sea,
         determination of the total range and mass (biomass) of the biota, the sum of all
         life in the biosphere, is a reasonable scientific goal.
         Chemistry of life
            fluid. The nuclear envelope, a double   Britannica. Although some feel debased by
            membrane surrounding the nucleus,
                contains pores that control the     the implication that people are “nothing
            movement of substances into and out     more” than a frenetic collection of interacting
              of the nucleoplasm. Chromatin, a
           combination of DNA and proteins that
                                                    molecules, others are thrilled with the power
              coil into chromosomes, makes up       of science to reveal the inner workings of the
            much of the nucleoplasm. The dense
                                                    chemistry of life. The spectacular success of
               nucleolus is the site of ribosome
                          production.               biochemistry and molecular biology in the
                                                    20th century suggests that laws of biology are
         derived from the interaction of atoms, thermodynamic principles, and life’s
         chemistry, which has persisted with faithful continuity since its origin some 3.7
         billion to 3.5 billion years ago.
         are mediated by enzymes called DNA polymerases. With the aid of enzymes,
         DNA can be produced in the laboratory.
         The cell, whether bacterial or nucleated, is the minimal unit of life. Many of the
         fundamental properties of cells are a function of their nucleic acids, their
         proteins, and the interactions among these molecules bounded by active
         membranes. Within the nuclear regions of cells is a mélange of twisted and
         interwoven fine threads, the chromosomes. Chromosomes by weight are
         composed of 50–60 percent protein and 40–50 percent DNA. During cell
         division, in all cells but those of bacteria (and some ancestral protists), the
         chromosomes display an elegantly choreographed movement, separating so
         that each offspring of the original cell receives an equal complement of
         chromosomal material. This pattern of segregation corresponds in all details to
         the theoretically predicted pattern of segregation of the genetic material
         implied by the fundamental genetic laws (see heredity). The chromosome
         combination of the DNA and the proteins (histone or protamine) is called
         nucleoprotein. The DNA stripped of its protein is known to carry genetic
         information and to determine details of proteins produced in the cytoplasm of
         cells; the proteins in nucleoprotein regulate the shape, behaviour, and activities
         of the chromosomes themselves.
         The other major nucleic acid is ribonucleic acid (RNA). Its five-carbon sugar is
         slightly different from that of DNA. Thymine, one of the four bases that make up
         DNA, is replaced in RNA by the base uracil. RNA appears in a single-stranded
         form rather than a double. Proteins (including all enzymes), DNA, and RNA have
         a curiously interconnected relation that appears ubiquitous in all organisms on
         Earth today. RNA, which can replicate itself as well as code for protein, may be
         older than DNA in the history of life.
         Chemistry in common
         The genetic code was first broken in the 1960s. Three consecutive nucleotides
         (base-sugar-phosphate rungs) are the code for one amino acid of a protein
         molecule. By controlling the synthesis of enzymes, DNA controls the functioning
         of the cell. Of the four different bases taken three at a time, there are 43, or 64,
         possible combinations. The meaning of each of these combinations, or codons,
         is known. Most of them represent one of the 20 particular amino acids found in
         protein. A few of them represent punctuation marks—for example, instructions
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         to start or stop protein synthesis. Some of the code is called degenerate. This
         term refers to the fact that more than one nucleotide triplet may specify a given
         amino acid. This nucleic acid–protein interaction underlies living processes in all
         organisms on Earth today. Not only are these processes the same in all cells of
         all organisms, but even the particular “dictionary” that is used for the
         transcription of DNA information into protein information is essentially the
         same. Moreover, this code has various chemical advantages over other
         conceivable codes. The complexity, ubiquity, and advantages argue that the
         present interactions among proteins and nucleic acids are themselves the
         product of a long evolutionary history. They must interact as a single
         reproductive, autopoietic system that has not failed since its origin. The
         complexity reflects time during which natural selection could accrue variations;
         the ubiquity reflects a reproductive diaspora from a common genetic source;
         and the advantages, such as the limited number of codons, may reflect an
         elegance born of use. DNA’s “staircase” structure allows for easy increases in
         length. At the time of the origin of life, this complex replication and transcription
         apparatus could not have been in operation. A fundamental problem in the
         origin of life is the question of the origin and early evolution of the genetic
         code.
                     Hemoglobin tetramer
                                                    identical to one of the building blocks of the
                                                    nucleic acids (both DNA and RNA) is
            Two αβ dimers combine to form the
           complete hemoglobin molecule. Each       employed. Metabolically ubiquitous molecules
            heme group contains a central iron
                                                    —flavin adenine dinucleotide (FAD) and
             atom, which is available to bind a
           molecule of oxygen. The α1β2 region is   coenzyme A—include subunits similar to the
                 the area where the α1 subunit      nucleotide phosphates. Nitrogen-rich ring
                   interacts with the β2 subunit.   compounds, called porphyrins, represent
                                                    another category of molecules; they are
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         smaller than proteins and nucleic acids and common in cells. Porphyrins are the
         chemical bases of the heme in hemoglobin, which carries oxygen molecules
         through the bloodstream of animals and the nodules of leguminous plants.
         Chlorophyll, the fundamental molecule mediating light absorption during
         photosynthesis in plants and bacteria, is also a porphyrin. In all organisms on
         Earth, many biological molecules have the same “handedness” (these molecules
         can have both “left-” and “right-handed” forms that are mirror images of each
         other; see below The earliest living systems). Of the billions of possible organic
         compounds, fewer than 1,500 are employed by contemporary life on Earth, and
         these are constructed from fewer than 50 simple molecular building blocks.
         Chemical bonds that make up the compounds of living organisms have a certain
         probability of spontaneous breakage. Accordingly, mechanisms exist that repair
         this damage or replace the broken molecules. Furthermore, the meticulous
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         control that cells exercise over their internal activities requires the continued
         synthesis of new molecules. Processes of synthesis and breakdown of the
         molecular components of cells are collectively termed metabolism. For synthesis
         to keep ahead of the thermodynamic tendencies toward breakdown, energy
         must be continuously supplied to the living system.
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             Pathway of carbon dioxide fixation     rich organic molecules as sugars, amino acids,
            and reduction in photosynthesis, the
           Calvin cycle. The diagram represents     and nucleotides. The oxygen becomes the gas
            one complete turn of the cycle, with    O2, which is released as waste back into the
           the net production of one molecule of
           glyceraldehyde-3-phosphate (Gal3P).      atmosphere. Animals, which are strictly
             This three-carbon sugar phosphate      heterotrophs, cannot live on carbon dioxide,
           usually is converted to either sucrose
                          or starch.                sunlight, and water with a few salts like plants
                                                    do. They must breathe in the atmospheric
         oxygen. Animals combine oxygen chemically with hydrogen atoms that they
         remove from their food—that is, from organic materials such as sugar, protein,
         and amino acids. Animals release water as a waste product from the oxygen
         respiration. Animals, like all heterotrophs, use organic materials as their sole
         source of carbon. This conversion of carbon provides an example of an aspect of
         an ecological cycle in which a required element flows through different types of
         organisms as it changes its oxidation state from CO2 to (CH2O)n and back to
         CO2.
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         must cycle. A search for such transformations provides one method of detecting
         extraterrestrial life.
                 The three processes of ATP          carbon sugar and three phosphates. As far as
              production include glycolysis, the
           tricarboxylic acid cycle, and oxidative   is known, such molecules are the general and
            phosphorylation. In eukaryotic cells     unique energy currency of living systems on
            the latter two processes occur within
              mitochondria. Electrons that are
                                                     Earth.
           passed through the electron transport
           chain ultimately generate free energy     No metabolic process occurs in a single step.
                    capable of driving the           The ordinary six-carbon sugar, glucose, does
                  phosphorylation of ADP.
                                                     not oxidize to carbon dioxide and water in
         living cells in the same way that glucose in air burns. Any release of energy by
         burning would be too sudden and too concentrated in a small volume to
         happen safely inside the tiny cell. Instead, glucose is broken down at ambient
         (i.e., relatively cool) temperatures by a series of successive and coordinated
         steps. Each step is mediated by a particular and specific enzyme. In most cells
         that metabolize glucose, the sugar first breaks down in a set of steps that occur
         in the absence of oxygen. The total number of such steps in plants, animals,
         fungi, and protists (see below Hypotheses of origins) is about 11. Other
         organisms, primarily bacteria and obscure protists and fungi, are anaerobes:
         they do not utilize molecular oxygen in their metabolism. In anaerobes, glucose
         metabolism stops at compounds such as ethanol or lactic acid. Aerobic
         organisms, including all animals, carry the oxidation of glucose farther. They
         rapidly use anaerobic glucose breakdown products such as lactic acid, ethanol,
         or acetate with Krebs-cycle intermediates in the mitochondria. Aerobic oxidation
         of glucose requires an additional 60 enzyme-catalyzed steps. The anaerobic
         breakdown of glucose uses enzymes suspended freely in solution in the cells.
         The aerobic steps occur on enzymes localized in mitochondria, the “power
         packs” of cells where oxygen gas is used to make the energy compound ATP.
         The complete aerobic breakdown of sugar to carbon dioxide and water is about
         10 times more efficient than the anaerobic in that 10 times as many ATP
         molecules are produced. (See metabolism.)
         Energy made available to cells in the form of ATP is used in a variety of ways—
         for example, for motility. When an amoeba extends pseudopods or when a
         person walks, ATP molecules are tapped for their energy-rich phosphate bonds.
         ATP molecules are used for the synthesis of proteins that all cells require in their
         growth and division, amino acids, and five-carbon sugars of nucleic acids. Each
         synthetic process is controlled and enzymatically mediated. Each starts from an
         organic building-block compound available to the cell as food. The amino acid
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         L-leucine, for example, is produced from pyruvic acid, which is itself the product
         of the anaerobic breakdown of glucose. Synthesis of L-leucine from pyruvic acid
         involves eight enzyme-mediated steps with an addition of acetic acid and water.
         These exquisitely interlocked and controlled metabolic steps are not performed
         in a diffuse manner helter-skelter in the cell. Rather, a marvelously architectured
         cellular interior displays specialized regions visible at the electron-microscopic
         level. Particular chemical reactions are performed in association with specific
         structures. In aerobic eukaryotes the mitochondrion with its intricate cristate
         membrane (the folds in the membrane are called cristae) provides the site of
         pyruvate, acetate, and lactate metabolism. These molecules are transformed and
         passed on from one enzyme to another as through a conveyor belt in a factory.
         Similarly, in those eukaryotes capable of oxygenic photosynthesis (algae, plants),
         photosynthesis occurs only in an organelle (a cell part) called a chloroplast.
         Chlorophyll, carotenoids, and other pigments that absorb visible light, as well as
         the detailed enzymatic apparatus for the photosynthetic process, reside there.
         All life is composed of cells of one of two types: prokaryotes (those that lack a
         nucleus) or eukaryotes (those with a nucleus). Even in one-celled organisms this
         distinction is very clear.
         All bacteria are prokaryotic, even though many, probably most, are multicelled
         in nature. The only other single-celled organisms that exist are fungi (one-celled
         fungi are called yeasts). All nucleated organisms (cells with nuclei and
         chromosomes in their cells) that are not animals, fungi, or plants are Protista.
         This huge group includes the unicellular or few-celled protists and their
         multicellular descendants. The large kingdom of Protista has 250,000 estimated
         species alive today. Some are very large, such as red algae and the kelp
         Macrocystis. One-celled protists include the familiar amoebas, paramecia, and
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                divides into two, freeing sister   all absent in prokaryotes. Prokaryotic cells,
                chromatids from each other.D.
               Anaphase. Sister chromatids are     which include all the cyanobacteria (formerly
                  drawn to opposite ends as        called blue-green algae), are bacteria in every
           centromeric microtubules shorten and
            polar microtubules lengthen, causing
                                                   way. Division is nonmitotic in all prokaryotes.
              the poles to move farther apart.E.   Bacteria lack nucleoprotein and a nuclear
              Telophase. Chromosomes uncoil,
                                                   membrane, and, when chromosome stain is
               microtubules disappear, and the
            nuclear membrane re-forms around       applied, only fuzz or nothing is seen. Whereas
             each set of daughter chromosomes.
                                                   all eukaryotic cells have more than one
             The cytoplasm begins to pinch in to
                  create two daughter cells.       chromosome and sometimes over a thousand,
                                                   the genes of prokaryotic cells are organized
         into a single “chromoneme” or “genophore.” (The term bacterial chromosome,
         while still in use, is, technically speaking, inaccurate.) The genes may or may not
         be concentrated enough to be seen, but in any case bacterial DNA floats freely
         in the cytoplasm. Prokaryote cell organization is less complex than that of
         eukaryotes. The basic question of the evolution of prokaryotes into eukaryotes
         —often rated the second major evolutionary mystery, after the origin of life—is
         thought to involve a complex series of partnerships in which distinct strains of
         bacteria entered each others’ bodies, merged symbiotically, and traded genes.
         Multicellularity
         extend their pseudopods, and, as individuals again, they migrate to feed. The life
         history repeats with swarms of migrating amoebas, slugs, stalks, and finally
         clusters of amoeba cysts on top as wet, food-rich conditions are followed by
         dryness and scarcity.
         Modern biology, following the lead of the German biologist Ernst Haeckel and
         the American biologists Herbert F. Copeland and Robert H. Whittaker, has now
         thoroughly abandoned the two-kingdom plant-versus-animal dichotomy.
         Haeckel proposed three kingdoms when he established “Protista” for
         microorganisms. Copeland classified the microorganisms into the Monerans
         (prokaryotes) and the Protoctista (which included fungi with the rest of the
         eukaryotic microorganisms). His four-kingdom scheme (Monera, Protoctista,
         Animalia, and Plantae) had the advantage of clearly separating microbes with
         nuclei (Protoctista) from those without (Monera: the prokaryotes—that is, the
         bacteria and archaea) and of distinguishing the two embryo-forming groups—
         plants and animals—from the rest of life. Whittaker, on ecological grounds,
         raised the fungi to kingdom status. The modified Whittaker five-kingdom
         classification system is perhaps the most comprehensible and biologically based
         way to unambiguously organize information about all groups of living beings.
         American microbiologist Carl Woese has offered still another classification
         scheme, in which all organisms are placed in either the Archaea (prokaryotes
         that include some salt lovers, acid lovers, and methane producers), the Bacteria
         (all other prokaryotes, including obligate anaerobic bacteria as well as
         photosynthetic and chemoautotrophic bacteria), or the Eukarya (all eukaryote
         forms of life). Woese’s scheme is based on molecular biological criteria that
         focus on the RNA sequence of morphological factors to classify new or disputed
         organisms. Although Woese’s three-domain system is very popular, a potential
         problem with it is that RNA, one characteristic among thousands, does not
         consistently correlate with many others.
         Microbes (or microbiota) are simply all those organisms too small to be
         visualized without some sort of microscopy. Bacteria, the smaller fungi, and the
         smaller protists are undoubtedly microbes. Some scientists classify tiny animals,
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         worms, and rotifers as microbes as well. Like weed, a plant not wanted in a
         garden, microbe is often a more useful term than one with a precise scientific
         meaning.
         Sex
         The world of microbes, in any case, is more vast, complex, diverse, and
         widespread than the visible ordinary world of plants and animals. For example,
         microbes have sexual lives that are different from those of the animal and plant
         kingdoms. In all organisms composed of prokaryotic cells, DNA that is not
         complexed with protein (“naked,” or chromonemal, DNA) transfers from a
         source (such as a plasmid, a virus, a second cell, or even DNA molecules
         suspended in a solution) to a live prokaryotic cell. The recipient cell at the end of
         the sex act contains some quantity of its own DNA and integrates some from
         the donor. All prokaryotes can reproduce in the absence of any sex act.
         In eukaryotes the sexual act requires the opening of membranes and the fusion
         of entire cells or at least of cell nuclei. The contribution from genes to the
         recombinant offspring is approximately 50 percent from each parent. From two
         to a dozen or so genders (in some species of paramecia) are present in any
         given sexual group. Although any given sex act requires at least two individuals,
         mating tends to be by pairs. Gender is understood to be those traits that
         predispose any organism to enter the sex act with any other. In multigender
         species only two genders or mating types enter a sex act at any one time. The
         rule is that in multigender species a mating requires any gender other than
         one’s own. Individual cells or multicellular organisms of complementary
         genders, in principle, produce fertile offspring. The universal rule is that no
         offspring result from matings of individuals of the same gender. In protists and
         fungi, uniparental reproduction (i.e., reproduction of a single parent) can occur
         in the absence of any sexual act, but two-parent sex may prevail seasonally or
         under other given environmental conditions in many inclusive taxa (such as
         families, classes, or phyla). Members of all species of the plant and animal
         kingdoms develop from embryos that form from a sexual act between the
         parents, and therefore two-parent (biparental) sex is the rule. Biparental
         sexuality of plants and animals has likely preceded its loss in all cases where a
         plant or animal species has reverted to uniparental reproduction, as in rotifers,
         whiptail lizards, and hundreds of plants that reproduce by runners rather than
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         by seed. This suggestion is based on the fact that, at the cell level, aspects of
         meiosis (required for two-parent sex) continue to occur..
         Ploidy, the concept of the number of complete sets of genes organized into
         chromosomes, is inapplicable to prokaryotes. Ploidy in protists, depending on
         species, varies so greatly and regularly that it is obvious that sexual cycles
         evolved in this diverse group of eukaryotes. Fungal cell nuclei are haploid (one
         set of chromosomes) or dikaryotic (two distinct nuclei from two different
         parents, each with one set of chromosomes sharing the same cell). Plant cell
         nuclei have two sets of chromosomes (diploid, in the sporophyte generation) or
         one (haploid, in the gametophyte generation). Animal cell nuclei, except in the
         gametes (sperm and egg), tend to have two sets of chromosomes (they are
         diploid).
         Viruses
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Limits to life
         Life has been detected in the stratosphere and in the ocean’s major depths.
         Mud-loving photosynthetic bacteria live in pools at Yellowstone National Park at
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         Bacteria and fungal spores have been discovered near the base of the
         stratosphere by balloon searches. Organisms sought at much higher altitudes
         (up to 30,000 metres [100,000 feet]) have been detected; they are few in number
         and are all propagules. Birds have been observed to fly at maximum altitudes of
         8,200 metres (27,000 feet), and on Mount Everest jumping spiders have been
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         found at 6,700 metres (22,000 feet). At the opposite extreme, ciliates, pout fish,
         crabs, and clams have been recovered from ocean depths where pressures are
         hundreds of times those found at sea level. At these depths no light penetrates,
         and the organisms, some of which are quite large with bioluminescent organs
         that glow in the dark, feed on particles of organic matter raining down from the
         upper reaches of the oceans. Others sustain themselves by their
         chemoautotrophic bacterial associations.
         Radiation and nutrient deprivation
Sizes of organisms
         New work on genome sequences, the total amount and quality of all of the
         genes that make up a live being, permits more accurate assessment of the
         material basis of the theoretically smallest and simplest extant free-living
         organisms. The complete DNA sequences of a few extremely small free-living
         organisms are now known—e.g., Mycoplasma genitalium with its 480 genes. All
         the molecules necessary for metabolism must be present. The smallest free-
         living cells include the pleuropneumonia-like organisms (PPLOs). Whereas an
         amoeba has a mass of 5 × 10−7 gram (2 × 10−8 ounce), a PPLO, which cannot
         be seen without a high-powered electron microscope, weighs 5 × 10−16 gram (2
         × 10−15 ounce) and is only about 100 nanometres across. PPLOs grow very
         slowly. Other, even smaller organisms that grow even more slowly would be
         extremely difficult to detect. An organism the size of a PPLO that has room for
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         only about a hundred enzymes depends entirely upon the animal tissue in which
         it lives. A much smaller organism would have room for many fewer enzymes. Its
         ability to accomplish the functions required for autopoiesis in living systems
         would be severely compromised. Were there, however, an environment in which
         all the necessary organic building blocks and such energy sources as ATP were
         provided “free,” then there might be a functioning organism substantially
         smaller than a PPLO. The inside of cells provides just such an environment,
         which explains why infectious agents, such as prions, plasmids, and viruses, may
         be substantially smaller than PPLOs. But it must be emphasized that viruses and
         their kin are not, even in principle, autopoietic.
         Metabolites and water
         Water, which is crucial for life, is the major molecule in all organisms. Unless a
         massive mineral skeleton is present, the dry matter of most organisms is about
         one-half carbon by weight. This reflects the fact that all organic molecules are
         composed of carbon bound at least to hydrogen. Metabolism uses a wide
         variety of other chemical elements. Amino acids are made of nitrogen and sulfur
         in addition to carbon, hydrogen, and oxygen. Nucleic acids are made of
         phosphorus in addition to hydrogen, nitrogen, oxygen, and carbon. Sodium,
         potassium, and calcium are used to maintain electrolyte balance and to signal
         cells. Silicon is used as a structural material in the diatom shell, the radiolarian
         and heliozoan spicule, and the chrysophyte exoskeleton. Iron plays a
         fundamental role in the transport of molecular oxygen as part of the
         hemoglobin molecule. In some ascidians (sea squirts), however, vanadium
         replaces iron. Ascidian blood also contains unusually large amounts of niobium,
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         Some species of animals enjoy highly specialized and exotic organs for the
         detection or transmission of sound. Dolphins and whales use their blowholes
         rather than their mouths to utter their sounds.
         Besides the familiar senses of sight, hearing, smell, taste, and touch, organisms
         have a wide variety of other senses (see above Sensory capabilities and
         awareness). People have inertial orientation systems and accelerometers in the
         cochlear canal of the ear. The water scorpion (Nepa) has a fathometer sensitive
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Convergence
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         Life ultimately is a material process that arose from a nonliving material system
         spontaneously—and at least once in the remote past. How life originated is
         discussed below. Yet no evidence for spontaneous generation now can be cited.
         Spontaneous generation, also called abiogenesis, the hypothetical process by
         which living organisms develop from nonliving matter, must be rejected.
         According to this theory, pieces of cheese and bread wrapped in rags and left in
         a dark corner were thought to produce mice, because after several weeks mice
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         By the 18th century it had become obvious that plants and animals could not be
         produced by nonliving material. The origin of microorganisms such as yeast and
         bacteria, however, was not fully determined until French chemist Louis Pasteur
         proved in the 19th century that microorganisms reproduce, that all organisms
         come from preexisting organisms, and that all cells come from preexisting cells.
         Then what evidence is there for the earliest life on Earth?
         Geologic record
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         Chemical analyses on organic matter extracted from the oldest sediments show
         what sorts of organic molecules are preserved in the rock record. Porphyrins
         have been identified in the oldest sediments, as have the isoprenoid derivatives
         pristane and phytane, breakdown products of cell lipids. Indications that these
         organic molecules dating from 3.1 billion to 2 billion years ago are of biological
         origin include the fact that their long-chain hydrocarbons show a preference for
         a straight-chain geometry. Chemical and physical processes alone tend to
         produce a much larger proportion of branched-chain and cyclic hydrocarbon
         molecular geometries than those found in ancient sediments. Nonbiological
         processes tend to form equal amounts of long-chain carbon compounds with
         odd and even numbers of carbon atoms. But products of undoubted biological
         origin, including the oldest sediments, show a distinct preference for odd
         numbers of carbon atoms per molecule. Another chemical sign of life is an
         enrichment in the carbon isotope C12, which is difficult to account for by
         nonbiological processes and which has been documented in some of the oldest
         sediments. This evidence suggests that bacterial photosynthesis or
         methanogenesis, processes that concentrate C12 preferentially to C13, were
         present in the early Archean Eon.
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         The earliest fossils are all of aquatic forms. Not until about two billion years ago
         are cyanobacterial filaments seen that colonized wet soil. By the dawn of the
         Phanerozoic Eon, life had insinuated itself between the Sun and Earth, both on
         land and in the waters of the world. For example, the major groups of marine
         animals such as mollusks and arthropods appeared for the first time about 541
         million years ago at the base of the Cambrian Period of the Phanerozoic Eon.
         Plants and fungi appeared together in the exceptionally well-preserved Rhynie
         Chert of Scotland, dated about 408 million–360 million years ago in the
         Devonian Period. Solar energy was diverted to life’s own uses. The biota
         contrived more and more ways of exploiting more and more environments.
         Many lineages became extinct. Others persisted and changed. The biosphere’s
         height and depth increased, as did, by implication, the density of living matter.
         The proliferation and extinctions of a growing array of life-forms left indelible
         marks in the sedimentary rocks of the biosphere (see evolution: The concept of
         natural selection).
         The origin of life
         Hypotheses of origins
         Perhaps the most fundamental and at the same time the least understood
         biological problem is the origin of life. It is central to many scientific and
         philosophical problems and to any consideration of extraterrestrial life. Most of
         the hypotheses of the origin of life will fall into one of four categories:
             1. The origin of life is a result of a supernatural event—that is, one irretrievably beyond
                the descriptive powers of physics, chemistry, and other science.
             2. Life, particularly simple forms, spontaneously and readily arises from nonliving matter
                in short periods of time, today as in the past.
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             3. Life is coeternal with matter and has no beginning; life arrived on Earth at the time of
                Earth’s origin or shortly thereafter.
             4. Life arose on the early Earth by a series of progressive chemical reactions. Such
                reactions may have been likely or may have required one or more highly improbable
                chemical events.
                                                      Hypothesis 1, the traditional contention of
                                                      theology and some philosophy, is in its most
                                                      general form not inconsistent with
                                                      contemporary scientific knowledge, although
               Michelangelo: The Creation of          scientific knowledge is inconsistent with a
                         Adam                         literal interpretation of the biblical accounts
            The Creation of Adam, detail of the       given in chapters 1 and 2 of Genesis and in
           ceiling fresco by Michelangelo, 1508–
                                                      other religious writings. Hypothesis 2 (not of
           12; in the Sistine Chapel, Vatican City.
                                                      course inconsistent with 1) was the prevailing
         opinion for centuries. A typical 17th-century view follows:
         [May one] doubt whether, in cheese and timber, worms are generated, or, if beetles and
         wasps, in cow’s dung, or if butterflies, locusts, shellfish, snails, eels, and suchlike be
         procreated of putrefied matter, which is apt to receive the form of that creature to which it
         is by the formative power disposed. To question this is to question reason, sense, and
         experience. If he doubts of this, let him go to Egypt, and there he will find the fields
         swarming with mice begot of the mud of the Nylus [Nile], to the great calamity of the
         inhabitants.
         It was not until the Renaissance, with its burgeoning interest in anatomy, that
         such spontaneous generation of animals from putrefying matter was deemed
         impossible. During the mid-17th century the British physiologist William Harvey,
         in the course of his studies on the reproduction and development of the king’s
         deer, discovered that every animal comes from an egg. An Italian biologist,
         Francesco Redi, established in the latter part of the 17th century that the
         maggots in meat came from flies’ eggs, deposited on the meat. In the 18th
         century an Italian priest, Lazzaro Spallanzani, showed that fertilization of eggs by
         sperm was necessary for the reproduction of mammals. Yet the idea of
         spontaneous generation died hard. Even though it was clear that large animals
         developed from fertile eggs, there was still hope that smaller beings,
         microorganisms, spontaneously generated from debris. Many felt it was obvious
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         Toward the end of the 19th century, hypothesis 3 gained currency. Swedish
         chemist Svante A. Arrhenius suggested that life on Earth arose from
         “panspermia,” microscopic spores that wafted through space from planet to
         planet or solar system to solar system by radiation pressure. This idea, of course,
         avoids rather than solves the problem of the origin of life. It seems extremely
         unlikely that any live organism could be transported to Earth over interplanetary
         or, worse yet, interstellar distances without being killed by the combined effects
         of cold, desiccation in a vacuum, and radiation.
         Although English naturalist Charles Darwin did not commit himself on the origin
         of life, others subscribed to hypothesis 4 more resolutely. The famous British
         biologist T.H. Huxley in his book Protoplasm: The Physical Basis of Life (1869) and
         the British physicist John Tyndall in his “Belfast Address” of 1874 both asserted
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         that life could be generated from inorganic chemicals. However, they had
         extremely vague ideas about how this might be accomplished. The very phrase
         “organic molecule” implied, especially then, a class of chemicals uniquely of
         biological origin. Despite the fact that urea and other organic (carbon-
         hydrogen) molecules had been routinely produced from inorganic chemicals
         since 1828, the term organic meant “from life” to many scientists and still does.
         In the following discussion the word organic implies no necessary biological
         origin. The origin-of-life problem largely reduces to determination of an organic,
         nonbiological source of certain processes such as the identity maintained by
         metabolism, growth, and reproduction (i.e., autopoiesis).
         Darwin’s attitude was: “It is mere rubbish thinking at present of the origin of life;
         one might as well think of the origin of matter.” The two problems are in fact
         curiously connected. Indeed, modern astrophysicists do think about the origin
         of matter. The evidence is convincing that thermonuclear reactions, either in
         stellar interiors or in supernova explosions, generate all the chemical elements
         of the periodic table more massive than hydrogen and helium. Supernova
         explosions and stellar winds then distribute the elements into the interstellar
         medium, from which subsequent generations of stars and planets form. These
         thermonuclear processes are frequent and well-documented. Some
         thermonuclear reactions are more probable than others. These facts lead to the
         idea that a certain cosmic distribution of the major elements occurs throughout
         the universe. Some atoms of biological interest, their relative numerical
         abundances in the universe as a whole, on Earth, and in living organisms are
         listed in the table. Even though elemental composition varies from star to star,
         from place to place on Earth, and from organism to organism, these
         comparisons are instructive: the composition of life is intermediate between the
         average composition of the universe and the average composition of Earth.
         Ninety-nine percent of the mass both of the universe and of life is made of six
         atoms: hydrogen (H), helium (He), carbon (C), nitrogen (N), oxygen (O), and
         neon (Ne). Might not life on Earth have arisen when Earth’s chemical
         composition was closer to the average cosmic composition and before
         subsequent events changed Earth’s gross chemical composition?
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          hydrogen           87            16                 3
          helium             12            0*                 0
          carbon             0.03          21                 0.1
          nitrogen           0.008         3                  0.0001
          oxygen             0.06          59                 49
          neon               0.02          0                  0
          sodium             0.0001        0.01               0.7
          magnesium 0.0003                 0.04               8
          aluminum           0.0002        0.001              2
          silicon            0.003         0.1                14
          sulfur             0.002         0.02               0.7
          phosphorus 0.00003 0.03                             0.07
          potassium          0.000007 0.1                     0.1
          argon              0.0004        0                  0
          calcium            0.0001        0.1                2
          iron               0.002         0.005              18
          *0 percent here stands for any quantity less than 10–6 percent.
                                                    The Jovian planets (Jupiter, Saturn, Uranus,
                                                    and Neptune) are much closer to cosmic
                                                    composition than is Earth. They are largely
                                                    gaseous, with atmospheres composed
                                                    principally of hydrogen and helium. Methane,
                                                    ammonia, neon, and water have been
                                                    detected in smaller quantities. This
                                                    circumstance very strongly suggests that the
                                                    massive Jovian planets formed from material
                                                    of typical cosmic composition. Because they
            photo of Jupiter taken by Voyager
                            1                       are so far from the Sun, their upper
               Photograph of Jupiter taken by       atmospheres are very cold. Atoms in the
             Voyager 1 on February 1, 1979, at a    upper atmospheres of the massive, cold
           range of 32.7 million km (20.3 million
             miles). Prominent are the planet's
                                                    Jovian planets cannot now escape from their
            pastel-shaded cloud bands and Great     gravitational fields, and escape was probably
                  Red Spot (lower centre).
                                                    difficult even during planetary formation.
         Earth and the other planets of the inner solar system, however, are much less
         massive, and most have hotter upper atmospheres. Hydrogen and helium
         escape from Earth today; it may well have been possible for much heavier gases
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         to have escaped during Earth’s formation. Very early in Earth’s history, there was
         a much larger abundance of hydrogen, which has subsequently been lost to
         space. Most likely the atoms carbon, nitrogen, and oxygen were present on the
         early Earth, not in the forms of CO2 (carbon dioxide), N2, and O2 as they are
         today but rather as their fully saturated hydrides: methane, ammonia, and water.
         The presence of large quantities of reduced (hydrogen-rich) minerals, such as
         uraninite and pyrite, that were exposed to the ancient atmosphere in sediments
         formed over two billion years ago implies that atmospheric conditions then
         were considerably less oxidizing than they are today.
         In the 1920s British geneticist J.B.S. Haldane and Russian biochemist Aleksandr
         Oparin recognized that the nonbiological production of organic molecules in
         the present oxygen-rich atmosphere of Earth is highly unlikely but that, if Earth
         once had more hydrogen-rich conditions, the abiogenic production of organic
         molecules would have been much more likely. If large quantities of organic
         matter were somehow synthesized on early Earth, they would not necessarily
         have left much of a trace today. In the present atmosphere—with 21 percent of
         oxygen produced by cyanobacterial, algal, and plant photosynthesis—organic
         molecules would tend, over geological time, to be broken down and oxidized to
         carbon dioxide, nitrogen, and water. As Darwin recognized, the earliest
         organisms would have tended to consume any organic matter spontaneously
         produced prior to the origin of life.
         The first experimental simulation of early Earth conditions was carried out in
         1953 by a graduate student, Stanley L. Miller, under the guidance of his
         professor at the University of Chicago, chemist Harold C. Urey. A mixture of
         methane, ammonia, water vapour, and hydrogen was circulated through a liquid
         solution and continuously sparked by a corona discharge mounted higher in the
         apparatus. The discharge was thought to represent lightning flashes. After
         several days of exposure to sparking, the solution changed colour. Several
         amino and hydroxy acids, familiar chemicals in contemporary Earth life, were
         produced by this simple procedure. The experiment is simple enough that the
         amino acids can readily be detected by paper chromatography by high school
         students. Ultraviolet light or heat was substituted as an energy source in
         subsequent experiments. The initial abundances of gases were altered. In many
         other experiments like this, amino acids were formed in large quantities. On the
         early Earth much more energy was available in ultraviolet light than from
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         The early ocean and lakes themselves may have been a dilute solution of
         organic molecules. If all the surface carbon on Earth were present as organic
         molecules, or if many known ultraviolet synthetic reactions that produce organic
         molecules were permitted to continue for a billion years with their products
         dissolved in the oceans, a 1 percent solution of organic molecules would result.
         Haldane suggested that the origin of life occurred in a “hot dilute soup.”
         Concentration through either evaporation or freezing of pools, adsorption on
         clay interfaces, or the generation of colloidal enclosures called coacervates may
         have served to bring the organic molecules in question in contact with each
         other.
         The essential building blocks for life (the monomers) were probably produced in
         relatively abundant concentrations, given conditions on the early Earth.
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         Although relevant, this is more akin to the origin of food than to the origin of
         life. If life is defined as a self-maintaining, self-producing, and mutable
         molecular system that derives energy and supplies from the environment, then
         food is certainly required for life. Polynucleotides (polymers of RNA and DNA)
         can be produced in laboratory experiments from nucleotide phosphates in the
         presence of enzymes of biological origin (polymerases) and a preexisting
         “primer” nucleic acid molecule. If the primer is absent, polynucleotides are still
         formed, but they lack specific genetic information. Once such a polynucleotide
         forms, it can act as a primer for subsequent syntheses.
         Many separate and rather diverse instances of the origin of living cells may have
         occurred in the Archean Earth, but obviously only one prevailed. Interactions
         eventually eliminated all but our lineage. From the common composition,
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         metabolism, chemical behaviour, and other properties of life, it seems clear that
         every organism on Earth today is a member of the same lineage.
         The earliest living systems
         Most organic molecules made by living systems inside cells display the same
         optical activity: when exposed to a beam of plane-polarized light, they rotate
         the plane of the beam. Amino acids rotate light to the left, whereas sugars,
         called dextrorotatory, rotate it to the right. Organic molecules produced
         artificially lack optical activity because both “left-handed” and “right-handed”
         molecules are present in equal quantity. Molecules of the same optical activity
         can be assembled in complementary ways like the stacking of right-handed
         gloves. The same monomers can be used to produce longer chain molecules
         that are three-dimensional mirror images of each other; mixtures of monomers
         of different handedness cannot. Cumulative symmetry is responsible for optical
         activity. At the time of the origin of life, organic molecules, corresponding both
         to left- and right-handed forms, were no doubt formed as they are in laboratory
         simulation experiments today: both types were produced. But the first living
         systems must have employed one type of component, for the same reason that
         carpenters cannot use random mixtures of screws with left- and right-handed
         threads in the same project with the same tools. Whether left- or right-handed
         activity was adopted was probably a matter of chance, but, once a particular
         asymmetry was established, it maintained itself. Optical activity accordingly is
         likely to be a feature of life on any planet. The chances may be equal of finding a
         given organic molecule or its mirror image in extraterrestrial life-forms if, as
         Morowitz suspects, the incorporation of nitrogen into the first living system
         involved glutamine, the simplest of the required amino acid precursors with
         optical activity.
         The first living cells probably resided in a molecular Garden of Eden, where the
         prebiological origin of food had guaranteed monomers that were available. The
         cells, the first single-celled organisms, would have increased rapidly. But such an
         increase was eventually limited by the supply of molecular building blocks.
         Those organisms with an ability to synthesize scarce monomers, say A, from
         more abundant ones, say B, would have persisted. The secondary source of
         supply, B, would in time also become depleted. Those organisms that could
         produce B from a third monomer, C, would have preferentially persisted. The
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            CITATION INFORMATION
            ARTICLE TITLE: life
            WEBSITE NAME: Encyclopaedia Britannica
            PUBLISHER: Encyclopaedia Britannica, Inc.
            DATE PUBLISHED: 14 June 2025
            URL: https://www.britannica.comhttps://www.britannica.com/science/life
            ACCESS DATE: August 11, 2025
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