Thursday, 9. September 2010
In 1943, Lourens G.M. Baas-Becking, Dutch microbiologist, coined the phrase “Everything is everywhere, the environment selects”. This was used to describe the ability of microbes to travel everywhere, and flourish in suitable environments, provided they are able to adapt the necessary mechanisms to survive these new habitats. However, this accepted idea did not adequately prepare scientists for the remarkable discovery made nearly forty years later, causing scientists to remodel accepted dogmas and theories.
A temperature anomaly recorded in the Pacific Ocean showed higher than expected temperatures, triggering geologists to launch an exploration project in 1977 (28). This led to the accidental discovery of the first hydrothermal vent, and its unique community of organisms seeming to disregard scientific expectations. Due to seafloor spreading, there are some areas of the ocean floor that are very close to the hot magma beneath the earth’s crust. This heat is transferred to ocean water seeping down into cracks, super-heating the fluid, and allowing it to accumulate minerals. This fluid is then funneled back up through the crust to meet the ocean. When this super-heated fluid meets the near-freezing ocean water, the minerals will precipitate out of the fluid, providing a mineral-rich environment, but also one that has extremes of cold water and hot water (sometimes nearing 400°C).
These extreme temperatures aren’t the only factors that would be thought to hinder biological growth. Hydrothermal vents are found around 2.5km below the ocean’s surface, where pressures can reach over 250atm. Even the longest reaching wavelengths given off by the sun cannot reach these depths, and any dying or decaying organisms or organic matter falling through the water from upper depths would have already been consumed. These harsh conditions have been thought to make the ocean floor uninhabitable.
However, keeping with Baas-Becking’s theory, we can find microorganisms at these sites – quite a large amount, in fact. Many species of bacteria grow in these environments, in thick mats visible to the naked eye. The bacteria at hydrothermal vents are so prolific, they are able to sustain the growth of many multicellular species, including a species of worm that can grow over six feet long. One organism responsible for sustaining this ecosystem is a prokaryote less than one micrometer in diameter, the archaeabacteria Methanococcus jannaschii.
This organism was first collected during a 1982 Alvin submersible dive led by Holger Jannasch (11). The first specimens were retrieved near a white smoker – a vent where the water coming up is relatively cool (200 – 300°C), and the majority of the minerals precipitating are Zinc, giving the water a whitish appearance. Quite apart from not being able to survive in this habitat, with a few adaptations, M. jannaschii has been able to thrive and take advantage of resources available to it. The mineral-rich environment makes this a prime place for chemoautotrophs, and M. jannaschii is one such organism, harnessing chemical energy to fix carbon dioxide into methane as follows:
4H2 + CO2 à CH4 + 2H2O
This carbon fixation is most likely accomplished by the employment of a RubisCO–like enzyme. This enzyme has similar binding sites to normal RubisCO and catalyzes the same essential Carbon fixation, but differences in the actual amino acid sequence and specific functionality require further analysis to determine whether it can truly be considered a form of RubisCO. This enzyme is heat-stable, able to function at temperatures up to 85°C, however, displays some of the lowest activity recorded when exposed to oxygen, forcing M. jannaschii to live as a strict anaerobe (20). Another factor forcing M. jannaschii to live as a strict anaerobe it its ability to fix nitrogen, and the enzyme accomplishing this is also sensitive to oxygen.
Methanogenesis ability and round shape are two primary factors in determining genus, and its current taxonomic breakdown is Superkingdom Archaea, Phylum Euryarchaeota, Family Methanococcales, Genus Methanococcus. However, it can more recently be found referred to as Methanocaldococcus jannaschii, in the Family Methanocaldococcaceae. The Methanocaldococcaceae are separated from the Methancoccales by their heat tolerance, the latter holding the mesophilic organisms, and Methanocaldococcaceae containing the thermophiles and hyperthermophiles (23). Able to survive in temperatures between 60°C and 90°C, M. jannaschii has an optimum temperature of 85°C, which requires the possession of several adaptations, but an ability to function in these high temperatures provides these microbes with an advantage besides a lack of much competition.
Due to the lack of ready-made nutrients, M. jannaschii must have pathways to make everything it needs, from lipids to proteins to nucleic acids. On the surface, the synthesis of all amino acids involve endergonic reactions. However, in these hot environments, M. jannaschii does not lose any energy when synthesizing most amino acids. In fact, the synthesis of Methionine from H2, NH3, CO2, and H2S results in an energy profit of 175kJ/mol. An exergonic reaction is evidenced in the production of at least ten other amino acids as well, resulting in an energy profit for most proteins (1).
This is one of the advantages to living in an extremely hot environment, however, M. jannaschii must also develop adaptations to protect its life functions against the extreme heat and pressure. Problems facing all thermophiles and hyperthermophiles include having to prevent membrane hyperfluidity, keeping macromolecules from denaturing, and obtaining usable water. M. jannaschii can control membrane fluidity in a variety of ways – like many archaea, membrane lipids are almost completely saturated, preventing too much movement. In addition to this, tetraether linkages may be formed, resulting in a lipid monolayer, providing a more rigid membrane structure. A novel way of decreasing membrane fluidity, so far only seen in M. jannaschii and Methanococcus igneus, is to join the ends of the two fatty acid chains, forming a macrocyclic lipid(6).
Proteins seen in M. jannaschii are heat-stabilized due to changes in non-essential amino acid sequences. Contrasted with homologous proteins in their mesophilic counterparts, proteins in these microbes are likely to be smaller, decreasing the amount of wobbling and flexibility, as well as maintaining secondary and tertiary structures by increasing the amount of polar and charged amino acids, as well as disulfide bonds. To prevent nucleic acids from denaturing, one might expect an increase in the number of hydrogen bonds normally seen in mesophilic archaea, meaning a higher G-C content. This is not the case, however, there are other methods hyperthermophiles can use to prevent denaturation. On notable characteristic that may be used to protect DNA is the presence of a reverse gyrase, which can work to reseal denatured DNA. In addition to this, DNA in archaea is usually found associated with histones, which are usually absent in true bacteria, but present in eukaryotic cells.
The presence of histones is a major factor in the classification of prokaryotic organisms, which, until recently, were all lumped into the Kingdom Monera. Some biologists believed that it would be better to have two groups to separate true bacteria from archaeabacteria, but it wasn’t until the first archaea’s genome was sequenced that strong evidence supported this case. M. jannaschii is probably most famous for being the first archaea to have its genome sequence, and only the fourth organism to be sequenced (2, 11).
Prior to this organism, two bacteria – Haemophilus influenza and Mycoplasma genitalium – had their complete genomes sequenced, as well as the eukaryote Saccharomyces cerevisiae. The genomic material in M. jannaschii is found in three pieces, a larger chromosome containing most of the genetic information, with additional information being contained on two smaller extrachromosomal elements (ECEs). At 1.66 Mb, the size of M. jannaschii’s genome was found to be one of the smallest in nature, excluding viruses and strict symbionts. In this there are 1738 genes, 44 of which are on the larger ECE, and 12 on the smaller ECE. It was thought that the archaea would be very similar to bacteria, but on closer inspection, only 11% and 17% of the genes were homologous to genes found in H. influenza and M. genitalium, respectively. This lent much evidence that archaea should not be grouped with bacteria, and while gene homologues were found in eukarya, 56% of its genome was completely new, giving strong proof to Carl Woese’s hypothesis that archaea are a distinct group, similar to both bacteria and eukarya, but not enough to be considered either (2,11).
The split between bacteria and eukarya does not seem random, either, as most genes found in M. jannaschii that share a homology with bacteria are involved in metabolism and structural characteristics. For example, MJ0577, an ATP-binding protein found in the archaeon shares much of its sequence with YnaF, a protein found in E. coli (15). Other similarities between bacteria and archaea are mechanosensitive ion channels (Msc), with MscMJ (MJ0170) showing striking homology with YggB, an E. coli Msc, enough so that when inserted into E. coli, normal Msc activity is observed (7). The genes shared with eukarya seem to be involved in transcription and translation. For example, the introns included in tRNA in bacteria are small and self-splicing, while eukaryotes require the use of a separate endonuclease to cleave these introns. It was found that M. jannaschii and other archaea also utilize a separate endonuclease to cleave these fragments (3).
The most interesting thing found in the study of M. jannaschii’s genome is what it lacks. Not only does it thrive in areas thought to be uninhabitable, it can also live without molecules thought to be necessary for survival. In other organisms, three DNA polymerases are needed, even in the simplest of bacteria, but only one can be found in M. jannaschii (11). The question next is why more of these cannot be found. Do they simply not exist, or are the unidentified genes coding for unknown molecules doing the same function? One of the many things lacking in M. jannaschii was a cysteinyl-tRNA synthetase, necessary for translation, but translation, and activity resembling that of cysteinyl-tRNA synthetase were observed. Further investigation showed that a single enzyme was responsible for the function of two aminoacyl-tRNA’s – prolyl-tRNA synthetase is able to not only make prolyl-tRNA, but cysteinyl-tRNA as well. Interestingly enough, the sequence of prolyl-tRNA synthetase in M. jannaschii does not differ much from other prolyl-tRNA synthetases, which makes it hard to track phylogenetically (17). This could be indicative of the high rate of mutations expected to be seen during life’s origins – few enzymes working to create many proteins could increase variety. Or over the course of several billions years has this organism lost an enzyme, and adapted an old one to continue surviving?
This could be one of the reasons why M. jannaschii’s genome is so small – it’s able to utilize a single enzyme for multiple reactions, where other organisms need to synthesize unique enzymes for each reaction. This is seen again in efforts to reduce mutations in the genome. CTP deaminases can deaminate cytosine to uracil, which when incorporated into DNA can lead to incorrect base pairing in replication, and mutation. To prevent the incorporation of uracil into DNA, organisms possess UTPases which convert UTP to UMP. Once again a “two for one” enzyme has been discovered – DCD-DUT is a single enzyme that performs both of these functions (4). The comparative instability of cytosine in high temperature environments may be one of the reasons for this – having an enzyme which makes the deaminated CTP “safe” in the immediate vicinity would help to reduce the amount of UTP incorporated into the DNA (4, 10). At these high temperatures, rapid molecular movement and interactions like these could be disastrous if there wasn’t a mechanism to control it.
Another reason why its genome is so small could be due to the sizes of the proteins it needs to create in extreme temperatures. By eliminating nonessential amino acid sequences from proteins, they are made more compact, and not easily moved. This would help to maintain stability within this organism. Evidence to support could be demonstrated in the sequencing of the psychrophile Colwellia psychroerthraea, whose genome is over twice the size of M. jannaschii’s at 5.3Mb (24). Most thermophiles have small genomes, and once more psychrophiles have their genomes sequenced, it could be looked at to determine if they have more genes, or are simply making larger proteins, or if simply the size of the main chromosome can lend some stability to the nucleic acid.
The isolation and culture of M. jannaschii was not a simple task to accomplish. It’s well-suited for its environment of over 200atm, and attempts to remove it from its environment resulted in cells rupturing as they were brought to the surface. This was thought to be due to the high vacuole content, as it’s producing a gaseous product from gaseous substrates. Further investigation showed that the amount of time given to decompression can affect the amount of cells that lyse, and unlike some other deep-sea barophiles, like MT-41, if the cells are decompressed slowly, they are capable of growing normally at 1atm (14). Another obstacle in the harvesting and culturing of these bacteria was the energy requirement. In environments lacking H2, the cultures cannot survive, and cocultures with organisms, such as Thermotoga martina, which produce molecular hydrogen, allows M. jannaschii to thrive without adding external H2 or CO2. This also provides an energy source for the heterotrophic organism, creating a healthy consortium. Using this technique, cocultures have been very successful, allowing T. maritima to thrive wherein previous, isolated cultures, it was inhibited by its own H2 production, and as long as the two organisms were touching, M. jannaschii could utilize that H2, removing it from the environment (12). These experiments and techniques performed with M. jannaschii lends some insight on how microbial communities really function around hydrothermal vents, and provides new ideas on how to culture “unculturable” microbes obtained from these sites. In the environment, probing for signature enzymes, such as methyl reductase or nitrogenase, could identify M. jannaschii. Of course, these enzymes are only indicative of most methanogens, and more testing would be needed to make sure it was M. jannaschii. If one just wants to study it in the lab, a culture of it can be obtained from Braunschweig, Germany’s Deutsche Sammlung von Mikroorganismen(12).
These organisms are cultured and studied for a variety of reasons, spanning several disciplines. As previously mentioned, understanding their genetic code may help to trace back the origins of life, and identify the common ancestor of all domains. Further studies may help to clarify whether eubacteria and archaea came together to form eukaryotes, or if archaea split into these two groups. Phylogenetically, the sequencing of this organism has provided a lot of insight to questions, and has spurred even more to be asked. The ability of M. jannaschii to live in these harsh conditions, deprived of sunlight and oxygen, making its own macromolecules has made scientists reevaluate the origin of life. Perhaps here in these dark depths M. jannaschii, and other archaea like it, took the relatively simple inorganic molecules found there, and began synthesizing them into more complex organic molecules, enriching the seas and allowing other organisms to take advantage of this and flourish. Nutrients would have been provided not only for other prokaryotes, but for eukaryotes and multicellular organisms as well. Sheets of M. jannaschii and other archaea found at these hydrothermal vents can be used as a source of nutrition for various organisms, such as shrimp and crabs only found at these vent sites. This has made scientists wonder – if these archaea are responsible for the beginnings of life under the ocean here, why not elsewhere? While Mars is closer, and easier to explore, the recent discovery of these hydrothermal vents perhaps being the origin of life here on Earth has caused people to turn to another celestial body in the search of extraterrestrial life. While not the largest or most impressive body in the heavens, Jupiter’s moon, Europa, is distinct in that underneath an icy exterior is a vast ocean, larger in volume than all our oceans put together. Its ocean contains enough salt and minerals it can conduct electricity, and has liquid water. Perhaps at the bottom of this vast ocean is Europa’s own hydrothermal vents, bustling with bacterial activity, and maybe even life that’s evolved from bacteria. NASA has already developed a project to study Europa, along with two other of Jupiter’s moons, for the possibility of life (22).
But there are other reasons for studying M. jannaschii, reasons closer to home. For a while now, thermophiles have been studied in the effort of developing heat-stable enzymes used for industrial and agricultural means. By using a thermostable form of amylase derived from M. jannaschii, new ways of processing starch have been developed which require much less energy than previously used (9). But not only has M. jannaschii been studied to reduce the amount of energy used, but it can also be utilized to create energy. Projects to study this organism, along with other methanogens have been approved by the United States Department of Energy. The methane these organisms produce is a large constituent of natural gas, and the alcohol methanol can be used in gasoline, which makes most of American’s energy usage (25). By studying methods of culturing these methane-producers, and refining the methane so it can be used as a fuel-source, an unlimited supply of fuel could be created. Unfortunately, using methane as a fuel is not that easy, requiring higher than normal temperatures to keep it going, as well as producing byproducts that can lead to acid rain, and so studies of using different kinds of catalysts for combustion of the fuel are being pursued (5,8,21). Another advantage of using methanogens like M. jannaschii to produce methane is the requirement of CO2, one of the more prevalent greenhouse gases. Intelligent utilization of this organism could potentially provide a clean fuel source, as well as reversing the affects of not-so clean fuel sources used in the past.
This is truly an interesting organism, to be the basis of study for so many branches of biology. Using it for industry, whether agricultural or as an energy source, its products have many uses. But far from just what it can be used for, the simple fact of its existence is groundbreaking. It has made us question the boundaries of life, and what’s necessary for an organism to survive, which has made most people believe that life outside the Earth is not just a piece of science-fiction anymore. Further investigation has been given to other environments on our own Earth we previously thought uninhabitable to see if life exists there.
One of the most significant discoveries, regarding M. jannaschii, is its symbiosis with other organisms, and methods of getting to the surface. This organism has been around for millions of years, dwelling in relatively obscurity at the bottom of the sea. This also seems to be the case with the giant lizard, Gojira tokyalis (30). When Gojira tokyalis awoke from its slumber, and headed towards land, doubtless it was covered with this bacteria.
Recently, it has been theorized that this archaeabacterium is also responsible for the destruction Gojira tokyalis was able to bring to the fair city of Tokyo. By producing methane gas, this organism was lending fuel to the fire – literally. The pyrorespiration, once thought to be simply another of G. tokyalis’s unique traits (29), may not be its own at all. Much like angler fish, who harbor bioluminescing bacteria, which are kept in a special organ which is used to lure prey, this giant lizard may be doing the same thing (31).
Preliminary investigations have lent supporting evidence to this theory. Rather than a parasitic symbiosis, this looks to be more of a mutualistic one, with both organisms benefiting. Through careful investigation, it has been found there’s a higher M. jannaschii cell density around the nostrils and mouth of this great beast – which would provide the archaeon with the carbon dioxide needed for methanogenesis. Extra methane would be released, and, if ignited, would allow Gojira to pyro-respire in the outflow, thus allowing the lizard a novel attacking ability to use against its prey.
Of course, this begs the question of how this gas is ignited. Once again, furthur investigation must be done, but some of the following possibilities have been theorized. Most likely it is not from the archaeon at all, but an ability of Gojira, which may include specialized teeth or organs in its mouth capable of ignition. Others believe that it is not an innate ability of the great beast, but rather, an influence of its diet. G. tokyalis has never been witnessed pyro-respiring, except for in the middle of an attack on Tokyo. This high automobile/train diet may cause excess bits of metal to become lodged in its teeth, and, when struck together, may cause sparks, and ignition of the methane (32).
Further studies must be done of course to determine the full extent of this symbiosis. To what lengths does it extend? It’s proved that the methanogen can life freely, but what about the beast? During its long sleeps at the bottom of the ocean, is the extra methane produced by M. jannaschii sustaining G. tokyalis? Or does its food come from other energy stores? More research must be done on this topic before it can be decided.
In summary, Methonococcus jannaschii, the deep sea thermophilic archaeon, is a novel organism, not in just its ability to synthesize enzymes and products used for technology, but also all the questions it allows us to ask, and study. How did life as we know it, including our own existence, evolve? What conditions are “too harsh” to sustain life? Are conditions on other planets able to sustain life, and, if so, do they? All these questions stem from, and could be answered by, a tiny microbe, invisible to the naked eye.
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