Smallest Life as We Know It

Diverse uncultivated ultra-small bacterial cells in groundwater

Nature has taken the praise-worthy step of making content available to a wider readership, via active links to ReadCube versions of the papers in media partners, like “The Huffington Post” in this case.

This particular paper reports on the characterisation of ultra-small organisms, which otherwise have proven impossible to culture. To make them available for study, samples were put into a rapid cryogenic freezer “snap freezing” them for electron microscopy. The results are fascinating, as the organisms are abundant and close to the smallest theoretical size for viable lifeforms.

Ultra-small bacteria

A bare minimum for any living thing, based on DNA, is a cell-wall, a means of making proteins (i.e. a ribosome, which translates the DNA chain into amino-acid chains that then fold into proteins) and the raw materials to make them from. That minimum size is around 200 nanometres – 0.2 millionths of a metre. These new organisms are as follows in this table:

Table 1

They’re so small that the volume taken up by their intra-cellular space and their cell-walls are of comparable size. A cubic micrometre is a volume of just 1E-18 cubic metres, or a water mass of just 1E-15 kilograms. Thus the smallest cell in the table masses ~4E-18 kg – in atomic masses that’s 2.4 billion amu. As the average atomic mass of living things is ~8 amu, that means a cell composed of just ~300 million atoms. The cell walls look crinkled because we’re seeing their molecule structure up-close.

Table 2

Regular bacteria can contain thousands of ribosomes, but these newly characterised micro-bacteria contain ~30-50. This indicates that they reproduce very slowly. Their genomes are also very short. Escherichia coli, a common bacteria in the human enteric system, has over 4.6 million base-pairs in its genome (humans have 3.2 billion) – but these new species range in length from a million to just under 700,000.

Genome Data

Genomes under a million base-pairs usually mean the organisms are obligate “parasites”, living around or inside larger organisms to source genes and metabolites that they can’t make themselves. Larger genomes mean they’re able to make all the required proteins, although they may live very slowly since they have so few ribosomes.

A key question, in molecular biology and astrobiology alike, is how the simple biomolecules produced by chemistry [as reviewed in this recent blog-post] came together to produce the “simplest” organisms. If we imagine a ‘soup’ of simple biomolecules, massing ~300 amu each, then about 8 million of them are required to produce the smallest organism described above. Merely throwing them together will not produce a living organism – the probability is something like 10-8,000,000. This is the chief puzzle faced by “Origins of Life” researchers.

There have been many clever proposals, with simplified metabolic cycles controlled by ribozymes (RNA enzymes) using an RNA based genetic code being a contender for an even smaller, simpler life-form. From the other direction, we know that plausible chemistry can concentrate and link up monomers of RNA nucleotides, forming quite long oligomers of RNA. Surprisingly short sequences show ability to work as ribozymes, thus a ready pool of ribozymes could conceivably form. From such a pool, some self-replicating set could form, which evolution could amplify into ever greater degrees of complexity. Just which particular ribozymes started down that road in the case of terrestrial life we don’t yet know. We might never know, since we have no clear molecular fossils from so deep in our past. Or do we? There’s a hint of that RNA past in the structure of ribosomes themselves. As we learn more about those “molecular assemblers” that produce all living things from raw amino acids, we will gain more insights into the rise of Life from molecules.

A thing to remember is that living things, at a biomolecular level, are continually converting simple molecules into incredibly complex ones, via ‘simple’ chemistry all the time. And those complex molecules show a particular ‘intelligence’ of their own. A good example is protein folding – to work, proteins fold up into specific 3-D configurations. Just how they do so has puzzled physical biochemists for years. It can’t be via simply twisting around at random. To see why, consider a short protein just 300 amino acids long. If, in each connection between amino acids, there are just 2 possible positions they can take, then the total number of possible positions is (2)300 ~2E+90 – a ridiculously large number of options to search through one-by-one. Thus it is impossible to jiggle an amino acid string randomly into the correct configuration of a protein in the mere minutes that protein folding is observed to take. The process is non-random and the way the sequence folds up is driven by the electromagnetic properties of each amino acid, so that they’re driven to form a protein’s structure through their mutual attractions and repulsions. Proteins are also very resilient to random changes in the amino acid sequence – only very rarely do single amino acid mutations produce a totally malfunctioning protein. Fortunately for us, as we depend on properly functioning proteins!

Making the Stuff of Life in One Batch

Common origins of RNA, protein and lipid precursors in a cyanosulfidic protometabolism : Nature Chemistry : Nature Publishing Group.

Life is built on chemistry, but the chemistry required to jump from the basic amino acids and small organic molecules expected on the Early Earth to the components of Life-As-We-Know-It – lipids, proteins and nucleic acids – has been obscure, until now. The scenario outlined in Nature Chemistry [doi:10.1038/nchem.2202] also explains why the various chemical components of our kind of life are so very similar. Even though they perform quite different roles, the building blocks are similar, produced originally by very similar chemical processes.

Original caption: The degree to which the syntheses of ribonucleotides, amino acids and lipid precursors are interconnected is apparent in this ‘big picture’. The network does not produce a plethora of other compounds, however, which suggests that biology did not select all of its building blocks, but was simply presented with a specific set as a consequence of the (photo)chemistry of hydrogen cyanide (11) and hydrogen sulfide (12), and that set turned out to work. To facilitate the description of the chemistry in the text, the picture is divided into four parts:

(a) Reductive homologation of hydrogen cyanide (11) (bold green arrows) provides the C2 and C3 sugars — glycolaldehyde (1) and glyceraldehyde (4)—needed for subsequent ribonucleotide assembly (bold blue arrows), but also leads to precursors of Glycine, Alanine, Serine and Threonine.

(b) Reduction of dihydroxyacetone (17) (the more stable isomer of glyceraldehyde (4)) gives two major products, acetone (18) and glycerol (19). Reductive homologation of acetone (18) leads to precursors of Valine and Leucine, whereas phosphorylation of glycerol (19) leads to the lipid precursor glycerol-1-phosphate (21).

(c) Copper(I)-catalysed cross-coupling of hydrogen cyanide (11) and acetylene (32) gives acrylonitrile (33), reductive homologation of which gives precursors of Proline and Arginine.

(d) Copper(II)-driven oxidative cross-coupling of hydrogen cyanide (11) and acetylene (32) gives cyanoacetylene (6), which serves as a precursor to Asparagine, Aspartic acid, Glutamine and Glutamic acid. Pi, inorganic phosphate.

The key-point is the relatedness and the step-by-step creation of one component or another, by short chemical processes, from the basic materials. To have produced such serial chemistry would have required means of isolating the raw materials and products, then mixing them. The next image from the paper provides a hint of what would’ve been required, on some sun-drenched landscape, swept by occasional rains, in an atmosphere of (probably) H2, N2, CO2 and H2O…

Chemosynthesis Sequence
Original caption: A series of post-impact environmental events are shown along with the chemistry (boxed) proposed to occur as a consequence of these events.

(a) Dissolution of atmospherically produced hydrogen cyanide results in the conversion of vivianite (the anoxic corrosion product of the meteoritic inclusion schreibersite) into mixed ferrocyanide salts and phosphate salts, with counter cations being provided through neutralization and ion-exchange reactions with bedrock and other meteoritic oxides and salts.

(b) Partial evaporation results in the deposition of the least-soluble salts over a wide area, and further evaporation deposits the most-soluble salts in smaller, lower-lying areas.

(c) After complete evaporation, impact or geothermal heating results in thermal metamorphosis of the evaporite layer, and the generation of feedstock precursor salts (in bold).

(d) Rainfall on higher ground (left) leads to rivulets or streams that flow downhill, sequentially leaching feedstocks from the thermally metamorphosed evaporite layer.

Solar irradiation drives photoredox chemistry in the streams. Convergent synthesis can result when streams with different reaction histories merge (right), as illustrated here for the potential synthesis of arabinose aminooxazoline (5) at the confluence of two streams that contained glycolaldehyde (1), and leached different feedstocks before merging.