Archive for the ‘ATP’ Category
abiogenesis is heavy, man

So, once more into the breach, let’s try and have fun with abiogenesis. It supposedly starts with organic compounds, generally considered as carbon-based, though I’ve heard tell of the possibility of silicon-based life – presumably you want to start with an element that combines readily with others, and those elements, but carbon in particular, fit the bill. Hydrocarbons, the simplest of which is methane (CH4), are an obvious example. However, as far as I’m aware, we haven’t been able to bridge the gap between non-life and life, inanimate and animate, chemistry and biology, in any clear-cut way in our laboratories and experiments. Membranes, self-replications, chains, autocatalysis are all more or less required, but nobody seems to have any clear idea of how and when it all started here. There may have been a few starts that then ended, until one didn’t. Here’s a bit from Wikipedia:
Life functions through the chemistry of carbon and water, and builds on four chemical families: lipids for cell membranes, carbohydrates for chemical energy storage and structural composition, amino acids for protein metabolism, and the nucleic acids DNA and RNA for heredity. A theory of abiogenesis must explain the origins and interactions of these classes of molecules.
Sounds like hard work, especially the genetic stuff. So I’ll start with amino acids, since I don’t have a clue… We get them from food, essentially, but what is food but living stuff, organic stuff, and so goes the circle. But let’s keep going. They were first discovered/identified in the early 1800s, the first being asparagine, from asparagus, in 1806. Apparently our bodies need twenty types of these carbon-based molecules, strings of which, or chains of which, form proteins. Of those twenty, eleven can be made by our bodies, and are labeled non-essential, while the other nine, the essential ones, must be obtained by food. All in all they’re important for brain chemistry, hormone production, and for maintenance and repair of muscle, skin and organ tissues.
But how did amino acids come to be? And what’s the difference between L and D types of amino acids? Apparently they’re like the mirror image of each other which makes me think of chirality which I barely understand. Britannica starts one of its articles with this:
The question of why organisms on Earth consist of L-amino acids instead of D-amino acids is still an unresolved riddle. Some scientists have long suggested that a substantial fraction of the organic compounds that were the precursors to amino acids—and perhaps some amino acids themselves—on early Earth may have been derived from comet and meteorite impacts. One such organic-rich meteorite impact occurred on September 28, 1969, over Murchison, Victoria, Australia.
… which is interesting but doesn’t help much, though it’s certainly a cause for wonder. Anyway, the video referenced below tells me that of the 20 amino acids that build proteins in our body, 19 are chiral. Then one particular amino acid, alanine, is focussed on, as it’s one of the simplest enantiomers – pairs of molecules that are mirror images of each other, and so un-super-imposable.
So this molecular biology is about life-sustaining molecules but not quite organisms, and nobody knows precisely how complex molecules become organisms – otherwise we’d be having fun creating new life forms, and only gods are allowed to have that kind of fun.
So we haven’t made life yet, but we’re getting there?
I’ve heard of course of an RNA world that might have preceded the DNA one, so let’s go there for a while. Nucleotides, nucleic acids, nucleosides, nucleobases and such all have to be understood and connected together to make sense of it all. So from here on in it will be attempted definition after attempted definition, with further attempts to connect them all together.
So what about prebiotic synthesis? Or, to quote another video referenced below, ‘location… where can we find the satisfactory chemistry required to make bioactive molecules? And what were these first biomolecules? We must surely need water and carbon – that’s what life as we know it requires, at a minimum. Then there’s nitrogen, key to building proteins (amino acids being nitrogen-based), and RNA and DNA for ‘information’. And phosphorous, essential for building many biomolecules, ATP for cellular energy, and phospholipids for cell membranes. Also referenced are amphiphiles (never heard of them) for forming primitive cells. They’re made from phospholipids so I’m not sure of the difference, just as I’m not sure of the difference between lipids and fatty acids – and did somebody mention tryptophan…? You need largely to be there in the labs being educated by the experts, and observing and experimenting.
The discovery in quite recent times of hydrothermal deep ocean vents and the chemo-synthesised, sunlight-free ecosystems they support, has added fuel, such as hydrogen sulphide, to the quest for the earliest life forms. But, to quote Phy the Neutrophil:
In an alkaline vent environment, the conditions for chemistry heavily disfavour the formation of cells. While hydrothermal vents do have the chemistry to make long-chain fatty acids, the harsh salty environment of the ocean is going to make it very difficult for these proto-membranes to form.
Mr Phy likes the Darwinian idea of a warm little pond, but also recognises that this too has its problems. In any case, some kind of cell or capsule formation, however or wherever it may have evolved, would be a major advance. Creating an enclosed micro-environment is likely to speed up the process of effective chemical development, and Mr Phy goes into much detail on this, and its alternatives, but of course I’m not strong on biochemistry, so proton gradients haven’t triggered my neurons.
But I must soldier on. AI has this to say on proton energetics:
All life uses proton gradients across membranes to drive energy production via ATP synthase. Because building proton pumps requires pre-existing energy, scientists propose that life began in alkaline hydrothermal vents, where natural geological pH gradients across inorganic pores provided the first proton-motive force before biological pumps evolved.
Adenosine triphosphate (ATP) , which I know is associated with mitochondria in humans, and is always called the ‘energy molecule’, or the energy storage molecule, as Wikipedia puts it, relies on this ATP synthase enzyme, which catalyses ATP using ADP (adenosine diphosphate) and inorganic phosphate. It gets very complicated with protons being pushed along an electrochemical gradient so that ATP can be stored by cells for future use.
Of course the evolution of ATP synthase, like so much in the make-up of the earliest life forms, is obscurely ancient, but well worth exploring as it appears to be central to all life. Wikipedia goes into hellish detail about it all, which is impressive and exhausting. I’m not sure if I can go on…
References
https://en.wikipedia.org/wiki/D-Amino_acid
https://www.britannica.com/science/amino-acid/Amino-acids-and-the-origin-of-life-on-Earth
Abiogenesis – LUCA, gradients, amino acids, chemical evolution, ATP and the RNA world

Jacinta: So now we’re thinking of the Earth 4 billion years BP, with an atmosphere we’re not quite sure of, and we want to explore the what and when of the first life forms. Haven’t we talked about this before?
Canto: Yeah we talked about the RNA world and viroids and abiogenesis, the gap between chemistry and biology, inter alia. This time we’re going to look more closely at the hunt for the earliest living things, and the environments they might’ve lived in.
Jacinta: And it started with one, it must have. LUA, or LUCA, the last universal common ancestor. Or the first, after a number of not-quite LUCAs, failed or only partially successful attempts. And finding LUCA would be much tougher than finding a viroid in a haystack, because you’re searching through an immensity of space and time.
Canto: But we’re much closer to finding it than in the past because we know so much more about what is common to all life forms.
Jacinta: Yes so are we looking definitely at the first DNA-based life form or are we probing the RNA world again?
Canto: I think we’ll set aside the world of viroids and viruses for now, because we want to look at the ancestor of all independently-existing life forms, and they’re all DNA-based. And we also know that LUCA used ATP. So now I’m going to quote from an essay by Michael Le Page in the volume of the New Scientist Collection called ‘Origin, Evolution, Extinction’:
How did LUCA make its ATP? Anyone designing life from scratch would probably make ATP using chemical reactions inside the cell. But that’s not how it is done. Instead energy from food or sunlight is used to power a protein ‘pump’ that shunts hydrogen ions – protons – out of the cell. This creates a difference in proton concentration, or a gradient, across the cell membrane. Protons then flow back into the cell through another protein embedded in the membrane, which uses the energy to produce ATP.
Jacinta: You understand that?
Canto: Sort of.
Jacinta: ‘Energy from food or sunlight is used..’ that’s a bit of a leap. What food? The food we eat is organic, made from living or formerly living stuff, but LUCA is the first living thing, its food must be purely chemical, not biological.
Canto: Of course, not a problem. I believe the microbes at hydrothermal vents live largely on hydrogen sulphide, and of course sunlight is energy for photosynthesising oganisms such as cyanobacteria.
Jacinta: Okay, so your simplest living organisms, or the simplest ones we know, get their energy by chemosynthesis, or photosynthesis. Its energy, or fuel, not food.
Canto: Semantics.
Jacinta: But there are other problems with this quote re abiogenesis. For example, it’s talking about pre-existent cells and cell membranes. So assuming that cells had to precede ATP.
Canto: No, he’s telling us how cells make ATP today. So we have to find, or synthesise, all the essential ingredients that make up the most basic life forms that we know – cell membranes, proteins, ATP and the like. And people are working towards this.
Jacinta: Yes and first of all they created these ‘building blocks of life’, as they always like to call them, amino acids, in the Miller-Urey experiments, since replicated many times over, but what exactly are nucleic acids? Are they the same things as nucleic acids?
Canto: Amino acids are about the simplest forms of organic compounds. It’s probably better to call them the building blocks of proteins. There are many different kinds, but generally each contain amine and carboxyl groups, that’s -NH2 and -COOH, together with a side chain, called an R group, which determines the type of amino acid. There’s a whole complicated lot of them and you could easily spend a whole lifetime fruitfully studying them. They’re important in cell structure and transport, all sorts of things. We’ve not only been able to create amino acids, but to combine them together into longer peptide chains. And we’ve also found large quantities of amino acids in meteorites such as the Murchison – as well as simple sugars and nitrogenous bases. In fact I think we’re gradually firming up the life-came from-space hypothesis.
Jacinta: But amino acids and proteins aren’t living entities, no matter how significant they are to living entities. We’ve never found living entities in space or beyond Earth. Your quote above suggests some of what we need. A boundary between outside and inside, a lipid or phospho-lipid boundary as I’ve heard it called, which must be semi-permeable to allow chemicals in on a very selective basis, as food or fuel.
Canto: I believe fatty acids formed the first membranes, not phospho-lipids. That’s important because we’ve found that fatty acids, which are made up of carbon, hydrogen and oxygen atoms joined together in a regular way, aren’t just built inside cells. There’s a very interesting video called What is Chemical Evolution?, produced by the Center for Chemical Evolution in the USA, that tells about this. Experimenters have heated up carbon monoxide and hydrogen along with many minerals common in the Earth’s crust and produced various carbon compounds including fatty acids. Obviously this could have and can still happen naturally on Earth, for example in the hot regions maybe below or certainly within the crust. It’s been found that large concentrations of fatty acids aggregate in warm water, creating a stable, ball-like configuration. This has to do with the attraction between the oxygen-carrying heads of fatty acids and the water molecules, and the repulsion of the carbon-carrying tails. The tails are forced together into a ball due to this repulsion, as the video shows.

fatty acids, with hydrophobic and hydrophilic ends, aggregating in solution
Jacinta: Yes it’s an intriguing video, and I’m almost feeling converted, especially as it goes further than aggregation due to these essentially electrical forces, but tries to find ways in which chemical structures evolve, so it tries to create a bridge between one type of evolution and another – the natural-selection type of evolution that operates upon reproducing organisms via mutation and selection, and the type of evolution that builds more complex and varied chemical structures from simpler compounds.
Canto: Yes but it’s not just the video that’s doing it, it’s the whole discipline or sub-branch of science called chemical evolution.
Jacinta: That’s right, it’s opening a window into that grey area between life and non-life and showing there’s a kind of space in our knowledge there that it would be exciting to try and fill, through observation and experimentation and testable hypotheses and the like. So the video, or the discipline, suggests that in chemical evolution, the highly complex process of reproduction through mitosis in eukaryotic cells or binary fission in prokaryotes is replaced by repetitive production, a simpler process that only takes place under certain limited conditions.
Canto: So under the right conditions the balls of fatty acids grow in number and themselves accumulate to form skins, and further forces – I think they’re hydrostatic forces – can cause the edges of these skins to fuse together to create ‘containers’, like vesicles inside cells.
Jacinta: So we’re talking about the creation of membranes, impermeable or semi-permeable, that can provide a safe haven for, whatever…
Canto: Yes, and at the end of the video, other self-assembling systems, such as proto-RNA, are intriguingly mentioned, so we might want to find out what’s known about that.
Jacinta: I think we’ll be doing a lot of reading and posting on this subject. I find it really fascinating. These limited conditions I mentioned – limited on today’s Earth surface, but not so much four billion years ago, include a reducing atmosphere lacking in free oxygen, and high temperatures, as well as a gradient – both a temperature gradient and a sort of molecular or chemical gradient, from more reducing to more oxidising you might say. These conditions exist today at hydrothermal vents, where archaebacteria are found, so researchers are naturally very interested in such environments, and in trying to replicate or simulate them.
Canto: And they’re interested in the boundary between chemical and biological evolution, and reproduction. There are so many interesting lines of inquiry, with RNA, with cell membranes….
Jacinta: Researchers are particularly interested in alkaline thermal vents, where alkaline fluids well up from beneath the sea floor at high temperatures. When this fluid hits the ocean water, minerals precipitate out and gradually create porous chimneys up to 60 metres high. They would’ve been rich in iron and sulphide, good for catalysing complex organic reactions, according to Le Page. The temperature gradients created would’ve favoured organic compounds and would’ve likely encouraged the building of complexity, so they may have been the sites in which the RNA world began, if it ever did.

a hydrothermal vent off the coast of New Zealand. Image from NOAA
Canto: So I think we should pursue this further. There are a lot of researchers homing in on this area, so I suspect further progress will be made soon.
Jacinta: Yes, we need to explore the exploitation of proton gradients, the development of proton pumps and the production of ATP, leaky membranes and a whole lot of other fun stuff.
Canto: I think we need to get our heads around ATP and its production too, because that looks pretty damn complex.
Jacinta: Next time maybe.
