Research Explainer: How giant clams record their diet in their shells

Two giant clams near Eilat in the Northern Red Sea. To the left is the small giant clam, Tridacna maxima, and to the right is a mature individual of the rare endemic giant clam Tridacna squamosina, only found in the Northern Red Sea.

You are what you eat, and clams are too. We’re made of atoms, which come in “flavors” called isotopes, relating back to the mass of the atoms themselves (how many protons and neutrons they have). Nitrogen, for example, comes in two stable (non-radioactive) forms called nitrogen-14 and nitrogen-15. Much like scientists can track the composition of a person’s diet from the isotopes of their hair, researchers have used the isotopes of clams to figure out their diet.

Nitrogen isotopes provide us with a useful and detailed record of food webs. Plants and algae tend to have more of the light isotope of nitrogen in their tissues than the animals that eat them (primary consumers), and the animals that eat those animals have even higher nitrogen isotope values. We can measure the amount of “heavy” atoms of nitrogen with a unit called δ¹⁵N (“delta 15 N”). A carnivore at the top of the food chain will have a very high δ¹⁵N, while plants will be the lowest. Clams, typically being filter feeders, will usually have an intermediate value, since they’re eating a lot of phytoplankton (tiny microscopic floating algae) and zooplankton (animal plankton that eat other plankton).

But I study a special kind of clam, the giant clams, which have a cheat code enabling them to become giant: they have algae *inside* of their bodies. The algae make food using photosynthesis and share it with their hosts! In exchange, the clams provide the algae with a stable environment free of predators, plenty of fertilizer in the form of their own waste, and even channel extra light to help the symbionts grow faster. This partnership is called photosymbiosis, and is pretty rare in clams, though it is common in other animals like the corals that build the reefs where giant clams are found! Previous researchers have shown that giant clams have very low nitrogen isotopic values in their tissue, like a plant, because they get most of their nutrition from the algae, rather than filter feeding.

I am a sclerochronologist. That means I study the hard parts of animals, in this case the shells of bivalves. Like the rings of tree, bivalves make growth lines in their shells which can serve as a diary of their lives. Some of my past work has looked at using chemistry of the growth lines of giant clams to measure the temperatures they grow at, compare the growth of ancient and modern clams, and even look at how much the clams grow in a day! Today though, I’m talking about my most recent paper, which looks at how we can use the shells of giant clams as a food diary.

But when they’re babies, the symbiosis in giant clams is not yet fully developed. During this early period of their lives, giant clams actually get more of their nutrition from filter-feeding like a “normal” non-photosymbiotic clam, until they’ve had a chance to grow in surface area and become a living solar panel. Like all bivalves, the shells of giant clams are made of calcium carbonate, bound together by a protein scaffold we call the shell organic matrix. Proteins are made of amino acids, which contain nitrogen! If we can get the nitrogen out of the shell from the early part of the clam’s life, and compare it to the nitrogen at the end of the clam’s life, it might record the clam’s transition from filter feeding to its mature plant-like lifestyle! If our hypothesis holds, we should record a decrease through its life in the shell δ¹⁵N values.

A model I made of the clams’ nitrogen intake, with the left plot how they switch from filter feeding to getting most of their nitrogen from dissolved sources around 5-6 years of age. Because the nitrogen isotopes of those two sources are different, that manifests in the expected values from the clam’s body (the right plot)!
A map made by my talented partner, Dana Shultz!

So I gathered a team of talented collaborators and set out to test that hypothesis, using giant clam shells that I was able to get on loan from the Hebrew University of Jerusalem Museum. These shells had been confiscated from poachers at the Egypt-Israel border. While I would have rather known these clams were still alive in the waters of the Northern Red Sea, being able to use them for research to understand the biology of their species was the next best thing! I had originally planned on pursuing a postdoc undertaking this project with Rowan Martindale, a professor at UT Austin who has studied the nitrogen isotopes of photosymbiotic corals, but when I started up at Biosphere 2, we ended up continuing with the project anyway as a collaboration! We measured the nitrogen isotopes of the shell material in the lab of Christopher Junium, a professor at Syracuse University, who has developed an exquisitely sensitive method to measure the nitrogen from shell material by essentially burning the shell powder and then scrubbing out unwanted material to isolate the nitrogen, to measure the isotopes in a machine called a mass spectrometer. Katelyn Gray is a specialist in isotopes of biominerals and assisted with drilling out powder from the shells with a Dremel. Shibajyoti Das, now at NOAA, is a specialist in measuring the shell nitrogen isotopes of other bivalves and he was master at doing much of the mass spectrometer work, and assisting in interpretation. Adina Paytan is a professor at UC Santa Cruz. She first provided the funding and support for me to go to the Gulf of Aqaba and collect these shells as part of an NSF-funded student research expedition! She also provided environmental data which helped us to interpret what the clams were actually eating!

A figure showing the four shells we sampled from, with the sampling areas in each hinge area showing colored and matching with the corresponding isotope plot to the right (colored points). 3 of the 4 shells show declines in isotope values with age. Shaded ribbon behind the data shows the model output.

So what did our crack team of scientists find out? We found that three of the four tested giant clams did indeed measure a decline in nitrogen isotopes over the course of their lives. Their earliest growth lines in the hinge areas of their shells record elevated δ¹⁵N values similar to other filter-feeders from the region. But as they aged, their later growth lines show much lower δ¹⁵N values, more like photosymbiotic corals and plants from the region. So clams indeed recorded the transition in nutrition as they became solar-powered! This degree and directionality of change in nitrogen isotopes was much greater than has been observed in any other clams measured in this way, which made sense considering their unique physiology. The clams have another area of the shell, the outer shell layer, which is closer to the symbionts than the hinge area. In this outer shell area, we did not observe much of a consistent trend in nitrogen isotopes. It’s likely that the outer layer is highly influenced by the photosymbionts even at the earliest stages of life.

Growth lines in the hinge area of two of the shells lit from behind, with the drilled areas for this study visible as well. The outer shell layer is the opaque and was also sampled for this study.

There was one clam that differed from the others in showing low δ¹⁵N values through life in its hinge shell layer. To help explain these differences, I created an independent model of the clams’ internal chemistry based on their growth rate, which slows as they age, and also is faster in the summer. When the clams are young filter feeders, they get most of their nitrogen from plankton, debris and other material floating in the water column making up floating material we call Particulate Organic Matter (POM). Meanwhile, when they are in their photosynthetic life stage, they get most of their nitrogen from nitrate, which is essentially Miracle Gro for the symbionts. The model showed that the clams should record a flip from filter feeding to photosynthesis around 4-5 years of age, which was confirmed by three of the shells! But what about the one that didn’t show this trend? My colleague Adina had fortunately measured the isotopes of POM and nitrate in different seasons in the Gulf of Aqaba. We found that in summer, as expected, POM δ¹⁵N is lower than nitrate. In the winter, meanwhile, that relationship is flipped! So if a clam grew more in winter, it would not record the same transition as was seen by the other clams. We think the clam that was the exception to the rule might have been more of a winter grower.

The chaotic nutrient environment of the Northern Red Sea, showing how in different seasons, dissolved nitrate has higher or lower δ¹⁵N values than the Particulate Organic Matter that the clams filter-feed on.

But long story short, we were able to demonstrate for the first time that giant clams show nitrogen isotopic values in their shells in line with expectations from their diet. Other clams have been measured this way, but the fact that we were able to conduct these analyses at all is a testament to the sensitivity of the elemental analyzer in Chris’s lab. Giant clams have *very* low concentrations of organic matter in their shells, so the forward march of technology was a major factor enabling this study to be possible.

Why does it matter that we can measure the transition of the clams from filter-feeding to photosymbiotic in their shell records? Well, giant clams are not the only bivalves which have photosymbionts. There are other clams in the fossil record which have been proposed to have had symbioses with algae, but until now we’ve never had a definitive geochemical way to measure this in fossils. We hope that this approach can be applied to the organic material in fossil shells, which is often well preserved, to see if huge clams in the Cretaceous and Jurassic had a similar way of life to the modern giant clams! If we can demonstrate that was the case, we can see how such species responded to past intervals of climate change, which will help us understand how giant clams will fare in the warming, acidifying ocean of the present.

These results also help explain the lives of giant clams themselves. We hope this kind of data can be used to measure the symbiotic development of giant clams in different places, with different types of food and nitrogen available, where we’d have the potential to measure pollution. Interestingly, the time that the model shows the clams transitioning to photosynthetic maturity is right around the time that they reach reproductive maturity (5-10 years of age). We’d like to investigate whether the time of clam maturity is controlled by the development of their symbiosis, which itself might relate to nutrients in the clams’ environment. If clams can grow faster, then they can mature faster, and potentially reproduce sooner in life. Will giant clams be able to thrive in the presence of increased nitrate, which is a common pollutant in coral reef environments? Like all worthwhile research projects, we have dozens of new questions to pursue as a result of this work, so stay tuned for the next installment in this journey of clam knowledge!

The boring giant clam is anything but.

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Tridacna crocea, bored into a coral head on a reef in Palau

There are many types of giant clam. Not all of them are giant; the boring giant clam, Tridacna crocea, only grows to 10 cm long or so. The boring giant clam is not so named because it’s dull; its main skill is its ability to bore into the coral of its coral reef home and live with its entire shell and body embedded in the living coral. They sit there with their colorful mantle edge exposed from a thin opening in the coral, harvesting energy from sunlight like the other giant clams. When disturbed by the shadow of a human or other such predator, they retract their mantle and close their shell, encased by an additional wall of coral skeleton. It’s a clever defensive strategy, and they are some of the most numerous giant clams in many reefs in the Eastern and Southern Equatorial Pacific.

But it’s always been a mystery of how they bore away at the coral so efficiently, and how they continue to enlarge their home as they grow their shell. There are other bivalves that are efficient borers, including the pholad clams (“piddocks”) which use sharp teeth on their hinge to carve their way into solid rock, and the shipworms, which have abandoned their protective shell and instead use their two valves as teeth to burrow into wood. Both of these methods of boring are pretty straightforward.

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Piddocks in next to holes that they made in solid rock. Source: Aphotomarine

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Shipworm embedded in wood. Source: Michigan Science Art via Animal Diversity Web

But the boring giant clam has no such adaptation. It does not have large teeth on its hinge to carve at the coral. Such abrasion of the coral would also not explain how they widen the opening of their cubby-holes to allow their shell to grow wider. This mystery has long confounded giant clam researchers. I myself have wondered about it, and was surprised to find there was no good answer in the literature about it. But now, a team of scientists may have cracked the problem once and for all.

At the back of T. crocea‘s shell at the hinge, there is a large “byssal opening” with a fleshy foot which they can extend out of the opening to attach themselves to surfaces. Giant clams that don’t embed in coral (“epifaunal,” resting on the surface of the coral rather than “infaunal,” buried in the coral) lack this opening. The researchers suspected that the foot was the drilling instrument the clam used to create its home.

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Byssal opening of T. crocea with the foot retracted. Source: NickB on Southwest Florida Marine Aquarium Society

How could a soft fleshy foot drill into the solid calcium carbonate (CaCO3) skeleton of corals? I can confirm from experience that my own foot makes for a very ineffective drilling instrument in such a setting. But T. crocea has a secret weapon: the power of acid-base chemistry. CaCO3 can be dissolved by acids. You may well have taken advantage of this chemistry to settle your acid stomach by taking a Tums, which is made of CaCO3 and reacts with the excessive hydrochloric acid in your stomach, leaving your tummy with a more neutral pH. pH is a scale used to measure acidity, with low numbers indicating very acidic solutions like lemon juice, and high pH indicating a basic solution like bleach.

Scientists are well aware of the hazards corals face from decreasing pH (increasing acidity) in the oceans. All the CO2 we are emitting, in addition to being a greenhouse gas, dissolves in the ocean as carbonic acid and gets to work reacting and dissolving away the skeletons of corals and any other “calcifying” organisms that make shells. It makes it harder for corals to form their skeletons and is already worsening die-offs of corals in some areas. The researchers suspected that the clams use this phenomena to their advantage at a small scale, lowering the pH with their foot somehow to dissolve away the coral to make their borehole.

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Using a wedge to keep open a Tridacna shell in my Red Sea work. We took a small blood sample with permission of local authorities. This caused no lasting effects to the clams.

But they needed to prove it, and that was a challenge. Giant clams can be unwilling research participants. I myself have observed this in trying to take samples of their body fluid for my own research. When they sense the presence of a predator, they immediately clam up in their protective shell. I used a small wedge to keep their shells open to allow me to take a sample of their body fluid, but the researchers working on T. crocea needed to convince the clam to place its foot on a piece of pH-sensitive foil, keep it there and do whatever acid-secreting magic allows it to burrow into coral. They would then be able to measure whether it indeed is making the water around its foot more acidic, and by how much.

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Diagram from Hill et al., 2018 showing their experimental design.

In what I can only assume was an extended process of trial and error and negotiation with a somewhat unwilling research subject, the researchers found exactly the right angle needed to convince the clam that it was safe enough to try making a coral home. But it was not in coral, instead sitting in an aquarium, on top of a special type of foil that changes color when exposed to changing pH, like a piece of high-tech litmus paper. The researchers discovered that their suspicions were correct: the clams do make the area around their feet significantly more acidic than the surrounding seawater, as much as two to four pH units lower. Where seawater is around a pH of around 8, the clams were regularly reducing pH to as low as 6 (about the level of milk) and sometimes as low as 4.6 (about the pH of acid rain). Small differences in pH can make a big difference in the power of an acid because each pH unit corresponds to 10x more protons (hydrogen ions, H+) in the water. The protons are the agent that dissolves CaCO3. Each proton can take out one molecule of coral skeleton. The clams are dissolving away coral skeleton to make holes with only their feet!

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Footage of the pH- sensitive foil, with darker areas corresponding to lower pH. The areas of low pH (high acidity) correspond exactly to the “footprint” of the clam!

But what in T. crocea‘s foot allows them to make acid? I know that my foot does not do this, though that would be a very entertaining and obscure superpower. The researchers found the enzymes called vacuolar-type H+-ATPase (VHA) present in great quantities in the outermost cells of the clam’s feet. These enzymes are found throughout the tree of life and are proton pumps that can quickly reduce pH through active effort. Other prior researchers like the influential Sir Maurice Yonge, a legendary British marine biologist who worked extensively with giant clams, had suspected that the clams had used acid but had never been able to detect a change in pH in the seawater around the clams’ feet through more conventional methods. It was only because of new technologies like the pH paper that this research team was able to finally solve this issue. And now, I suspect other groups will want to re-investigate the importance of VHA in their study organisms. Many branches of the tree of life may be utilizing acid-base chemistry to their advantage in ways we never had previously imagined.

You are Isotopes (Part III)

This is the third part of a series about isotopes and why they’re useful and interesting to scientists.

Isotopes are the flavors of elements. And because our universe is made up of atoms of elements, every object can be thought of as a delicious smoothie of flavors. Scientists like me are trying to reverse engineer those mixtures and pick out individual tastes, in order to answer questions about our world.

For example, I work with giant clams. These guys build enormous shells made of a mineral called calcium carbonate: CaCO3. That means that every molecule in a clam’s shell contains a calcium atom, a carbon and three oxygens. But as you might know from reading the previous entries in this series, not all of those atoms are the same. They are a mixture of different flavors. We have some carbon-12 and 13 in there (so named for their atomic weights), and some oxygen-16, 17 and 18. Here I’m focusing on the stable isotopes, which are not radioactive and are called “stable” because they’re not going to self-destruct. There are radioactive isotopes in there too, but I don’t use those nearly as often in my work.

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Officer, this is a pile of giant clam powder, I swear!

I am measuring stable isotopes of carbon and oxygen in my shell samples. To do this, I take a sample of powder, grind it up, weigh it, and put it into tiny little cups. We only need a very small sample: about 50 micrograms of shell material. A typical pill of tylenol contains over 300 mg of active ingredient, so about 6,000 of my samples will fit in a single tylenol regular strength pill, if you suddenly decided you needed a giant clam prescription.

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Simplified representation of what’s happening in a mass spec. Source

This tiny sample is one of thirty that I can measure at a time. Those samples are reacted with acid and the CO2 gas that is released as a result of the reaction can be processed by a machine called a mass spectrometer. The mass spec, which is in the Stable Isotope Laboratory in my building, ionizes the molecules in that gas (gives them a bit of electric charge) and then those ions are flung through an electromagnetic field. That beam of charged gas is flung around a curve. That curve is where the magic of making a mass spectrum happens.

Think of the atoms in the CO2 gas from my sample as a bunch of racecars exiting the straightaway and starting around the curve on the racetrack. Only these racecars vary in weights. And the race organizers have greased the track at the curve so that they fling into the sides of the track when they try to turn. As the racecars fling into the sides of the track, they will separate according to their mass. The lighter cars will be able to make it further around the curve before they meet their demise because they have less inertia forcing them forward, whereas the SUVs in the race will barrel forward straight into the sides of the track. At the end, you have a spectrum of racecars poking out of the walls of the track, with SUVs first, then the coupes, then the compact cars and then the motorcycles, which almost made it around the bend, but not quite. Atoms in the mass spectrometer act the same way, and we measure how many collisions happen along each point of the bend in order to not only “weigh” the sample of gas, but also figure out how many molecules of each weight there are!

It turns out that it is quite difficult to measure the exact number of atoms of a particular isotope in gas, however. It is much more economical and feasible for the purposes of most researchers to simply compare our mass spectrum to the results from a standard. Much like there is a literal standard kilogram and standard meter in a lab somewhere in France which is used to keep track of how much mass is actually in a kilogram, there is a standard used by all researchers like me to describe our samples of carbonate.

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A collection of belemnite fossils from the Pee Dee formation, similar to the one used for the PDB standard. Source

The most common standard used is from a belemnite fossil from the Pee Dee formation in North Carolina. Belemnites are extinct squid-like creatures that formed an internal shell, and one of those internal shells was fossilized, unearthed by a researcher and ground up to become the reference for all other researchers following. Samples of the carbonate in its fossil had more carbon-13’s per unit mass than most other fossil specimens known.  Almost everything you measure will be “lighter” in terms of carbon, because carbon-12 is naturally so common on our planet.

Scientists needed a convenient way to put a number on this, so a simple formula was developed which would allow us to quickly communicate to each other how isotopically “heavy” or “light” a particular sample is in comparison to the Pee Dee Belemnite. The formula isn’t that important for our purposes but the units of its output are in parts per thousand, or “per mil” for short (same idea of how we shorten parts per hundred to “percent”).

The symbol for per mil is a percent sign with an extra little loop at the end: ‰. To make the shorthand complete, we also need to note that this is how much the carbon-13 to carbon-12 isotope ratio of a sample differs from the Pee Dee Belemnite. We do so, we use the Greek delta symbol (δ), commonly used in science and math to represent “difference or change from.” So a sample that has a carbon-13 to carbon-12 ratio which is 20 parts per thousand less than that of the Pee Dee Belemnite is written -20 ‰ δ13CPDB. There are other samples that can be used as well, including Standard Mean Ocean water (SMOW), and the Vienna Pee Dee Belemnite (VPDB). It’s important to note which you are using so that people know the scale of your measurement!

Phew, hopefully that didn’t confuse the hell out of you! Next time, I’ll talk about how different δ13C (and for oxygen isotopes, δ18O) can tell us different details about the life of an organism. Here’s a cute gif of a scallop as a chaser after all that science you read.

You are isotopes (Part II)

This is the second part in a series how isotopes work and how they are scientifically fascinating. Part I here

It turns out a horse is not just a horse, of course. The horse is a collection of atoms, and each of those atoms has a particular isotopic “flavor”, and the collection of isotope types in the horse tells a story.  At the end of the day, scientists are simply interested in reading and telling stories about our world. The tail….er, tale of the horse is written by myriad interacting processes in the universe which influence the horse’s stable isotope ratios.

As I mentioned last time, carbon-12 is much, much more common than carbon-13 is on our planet, due to nuclear fusion of helium-4 in the sun. there are nearly 99 carbon-12’s on earth for every carbon-13. But that’s the base ratio if you took our whole planet, put it in a blender and mixed it all up. If you measured a particular object, such as a horse, it likely does not follow that measure exactly. It has become differentiated from the global average by numerous factors which have altered the isotope ratio.

In isotopic chemistry, fractionation is our name for any process which creates a preference for a certain isotope. If chemical reactions had no bias toward any particular isotope, that 99 to 1 ratio of carbon-12 to carbon-13 would be present in literally everything including you and me. But it turns out that the biochemical dice are loaded- to make the ratio even more biased!

The enormous Rubisco enzyme. No one said photosynthesis was simple. Source: Wikipedia

Photosynthesis is the process by which plants take carbon dioxide gas in the atmosphere and “fix” it to make sugars, which they then use for food. The core enzyme responsible for this carbon fixation is called Rubisco (short for Ribulose-1,5-bisphosphate carboxylase/oxygenase). This enormous molecule is likely the most abundant enzyme on earth. And it turns out that it has a favorite flavor when it comes to the carbon it fixes into sugar.

In fact, the entire plant is discriminating against carbon-13 in several of the processes of photosynthesis. Carbon dioxide molecules diffuse more quickly into the plant’s leaves if they include the lighter carbon-12 rather than carbon-13. “Light” CO2 also dissolves more easily in the plant’s fluids. But the biggest fractionation happens when the Rubisco molecule gets hold of CO2 and breaks it. At each of these steps, the light carbon-12 is more likely to be used by the plant than its heavier siblings. There are various thermodynamic reasons for why this is the case, but the plant is essentially a sieve removing more of those heavy carbons at every step. At the end of the process, the plant is left isotopically “lighter” than the CO2 gas surrounding it that it breathes in.

Because you are what you eat, this means that you are suspiciously carbon-light, and there’s nothing you can do about it. Should have thought of that before you decided to be dependent on plants as the factory for your carbon-based molecules. Next time, we’ll talk about how we measure this, and the kinds of science that can happen once you have a nice consistent measurement to use to compare isotopic ratios between samples.

You are isotopes (Part I)

As you may well know, every element is defined by its number of protons contained the nuclei of its atoms. Hydrogen has one. Carbon has six. This is non-negotiable. But every element can be found in multiple “flavors” known as isotopes. This flavor depends on the isotope’s atomic mass, which is determined by the number of neutrons present in the nucleus of that atom. Neutrons are kind of like atomic ballast. Unlike protons, which have a positive charge, they are neutral, but they do have a mass. Different isotopes have different numbers of neutrons, determining their atomic mass but preserving its particular elemental identity (which would only change if you changed the number of protons present).

Let’s focus on carbon, an element which I think about daily, though every element has isotopes and I could pick many other examples. Hope you’re OK with that, but if not it’s my blog so deal with it. So carbon has been found or created in up to 15 flavors. A whopping 98.9% of all the carbon on Earth occurs as carbon-12 (written as 12C), which has six protons and six neutrons, adding up to an atomic mass of about 12 atomic mass units (amu). It’s the most common because it’s the product of three helium-4 isotopes fusing together, each weighing 4 amu + 4 amu + 4 amu adding to make a single carbon-12. This is a very common reaction in stars, and because you are stardust, it is also the most common flavor of carbon in you.

But we make other flavors by adding neutrons. You can make carbon-13 with six protons and seven neutrons. This is a rare flavor, accounting for almost all of the remaining 1.1% of carbon found on earth. It is also the only other stable form of carbon. I note that it’s stable because all the other 13 known flavors of carbon are unstable, and many are only known from the laboratory because they are too short-lived to be found in the environment.

It turns out that if an element’s atomic nucleus is too light, or too heavy, that element will become radioactive and decay with time, continuously firing off pieces of itself out of frustration. Carbon-14 is the most famous and common of these radioactive isotopes of carbon, and it still only makes up 1 in every million million atoms of carbon on earth. Carbon-14 fires off particles and decays into nitrogen-14 because it is more stable orientation for the protons and neutrons to be in, for physics reasons I won’t get into here.

Carbon-14 does this in a very predictable, methodical pattern. It’s difficult to predict when an individual carbon-14 atom will do this, but if you take any object you have just created, like a piece of pottery, for example, you can be pretty much certain that in 5,730 years, only 1/2 of the carbon-14’s will still be present. The rest decided they’d rather be nitrogen-14. This is non-negotiable and you’d best learn to accept it. But it means that we can sniff out the age of a lot of interesting mysterious objects if we know the amount of carbon-14 present in the environment (which we often do) and measure the amount present in the object today. You have some restrictions. For example, for objects that are too old, too little of the carbon-14 would be left for you to measure accurately.

Carbon-14 dating, often just called radiocarbon dating, is very useful in figuring out the ages of stuff, but I’m mostly interested in the stable isotopes of carbon. Next week I’ll talk about why that is, and what kind of questions I can answer by looking at amounts of different stable carbon isotopes in a sample. See you then!