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I have had the privilege to sail twice on the JOIDES Resolution, with this being my second cruise, Expedition 402 Tyrrhenian Continent-Ocean Transition. The first time was with Expedition 393: South Atlantic Transect II. We aimed to study the age of the oceanic crust as we moved away from the mid-Atlantic ridge toward South America. You can see the expedition summary here.

Tessa Peixoto on steel beach in front of a sunrise during Expedition 393

At the time I had very little understanding of rocks and sediment besides what my oceanography class in college provided me. Most of my academic career was focused on the biology of organisms, so when I thought of rocks I thought of how they provided shelter and structure for the living things that I studied. For instance, rocks provided a hard surface for corals and algae to root themselves and sediment provided hiding spots for bottom dwelling fish. After a few days on Expedition 393, I learned that rocks and sediment can hold the history of our atmosphere, the history of our oceans, and the history of catastrophic events (big or small).

The rocks and sediment on both expeditions have been extraordinarily different. I cannot say that I have seen a similar core between the two, which makes sense because we are in drastically different areas. But again, I had the genuine thought, what could be different about the seafloor from one place to another.

Examples of some of the sediment cores from different oceans or seas across the globe. Each core was taken on different expeditions.

Each expedition has different goals, and different operation expectations, however the methods we use to drill, make thin sections, make p-wave velocity measurements, and more  tends to be relatively the same give or take some modifications. For example, thin sections can only be done by taking a small piece of hard rock, cut a thing slice from the top, then polish it down to the thickness of a hair strand. That process does not change because we found a rock in a different ocean. As someone who was returning to the JOIDES Resolution, I envisioned seeing similar gray rocks with some dark grays and browns, I envisioned seeing sediment that followed the color range of chocolates in a chocolatier shop. I figured I was going to be learning about the ocean floor from a different perspective guided by the different expedition objectives. Immediately, I was very wrong and it was thrilling. As Phillipe Pezard, our Downhole specialist, said on one of our first days: “I am a kid in a candy shop”. The ship is a candy shop and the scientists are the local kids who just got their weekly allowance.

Sediment in the Tyrrhenian Sea did not look the same as that of in the South Atlantic, nor did it seem to act the same way when we drilled into the seafloor in both locations.

Examples of some of the sediment from Tyrrhenian Seas cores.

As someone who does not immerse themselves in geology every day, I still was able to follow the science party as they explained their research goals and expectations from the scientific prospectus in the weeks leading up to expedition 402. Rationally it felt straightforward to understand that under different circumstances like temperature and pressure sediment and rocks react in certain ways. It felt straightforward to understand that these materials will undergo change, erosion, weathering, layering and more. But once I saw the actual cores a foot away from my face, it was a whole other beast. That is the value of field work and that is the value of this ship. You cannot learn more about this planet if you do not have access to it.

Tomoaki Morishita, petrologist, looking at hard rock samples during Exp 402.
EXP 402 petrologists and geologists discuss sampling on hard rock cores.                  

As I reflected on my two expedition experiences and saw the science crew experience a range of emotions as new cores were collected, I decided to go around and ask some people who have been on multiple expeditions for their perspectives.

“What has surprised you about the rocks and sediment you have seen across expeditions?”

Alejandro has sailed on 8 expeditions (or 6, he wasn’t entirely sure) and is sailing as the Physical Properties Lab Specialist. He is most surprised by the homogeneity (the sameness) and the gradual change in characteristics of the cores from the bigger oceans. When he was in the Pacific it took a few cores before you started to see a huge color change or texture change, while in the shallower basins the cores tend to be more heterogenous (varied) and have more rapid changes to their features. It always keeps him asking why.

Alejandro, physical properties marine technician.

Emily Estes has sailed on 4 expeditions with the JOIDES Resolution and is the current Expedition Project Manager. She is surprised that even when we have the prospectus identifying everything that we expect and understand to be in the area, we still find something different. Especially when the data in the prospectus is based on previous drilling sites in the area, one would think the core would bring few surprises. Though she does not think of these moments as bad surprises, but as opportunities to ask more questions. Most of her work and expeditions have been in larger oceanic basins where there are similar features throughout multiple cores before it starts to change, which is not the case for the shallower basins like the Tyrrhenian Sea.

Emily Estes excited about some data on Rig Watch, a system used to monitor the drilling performance.

Kevin Grigar has sailed on 24 expeditions and is the Operations Superintendent. Though his role is to check how well the cores are coming out to help determine with SIEM Offshore what could change about the drilling operations and procedures, he still gives the cores a look. What surprises him is the change in formations and color throughout the cores, sometimes within the same core and sometimes it is after a few ones. Either way he is amazed, and loves how pretty the changes can look.

Kevin Grigar in his office on the bridge deck.

James Kowalski has sailed on 3 expeditions and is sailing as the ship curator. He is surprised by the laminations (layering that happens in sedimentary rocks) and features that disappear quickly between cores. He finds that each core is so different and rarely sees similarity across expeditions. The variety is something that he enjoys and it keeps him on his toes.

James on the core catwalk preparing the measurements for the core to be sectioned off into 150cm pieces.

Hearing their responses made me think of the cycle of scientific thinking (https://www.youtube.com/watch?v=j12BBcKSgEQ)  and what one of our co-chiefs, Nevio Zitellini, said the other day “We start this expedition with a question, and we end this expedition with more questions.”

As we settle into week 3 of Expedition 402, I enter it even more consumed by two notions. First, that we still have so much to learn, and secondly, it seems that when I ask “how could rocks and sediment from one ocean to another be different” it is a question that scientists and the public, alike, share.

A rock is a rock is it not?

Ocean Acidification

New Friends, New Addresses

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The JOIDES Resolution (JR) was a renowned, international, scientific research ship. It was home to over 190 expeditions, each sailing for 60 days at a time without docking. Scientists and crew members from all over the world met to discover Earth’s secrets through studying ocean cores. Every two months the JR would get a new crew, sailing to an entirely new place. This once in a lifetime experience forms special and unforgettable social connections.

Since working on the JR I’ve kept those connections strong with snail mail. I have always been an avid penpal, so meeting new friends means new addresses to send my letters and postcards to. Experiences like sailing on the JOIDES Resolution or participating in programs like OCEAN CORE Academy is one of the ways I’ve met people from all over the world.

Now that the JR is retired, there is no more scientific research drilling being done through the International Ocean Discovery Program (IODP). But, there is still plenty to learn from ocean cores, and plenty of people to meet through programs like OCEAN CORE Academy (OCA). OCA is an annual summer opportunity from the U.S. Scientific Support Program (USSSP) that hosts undergraduates interested in geoscience related careers. Students can apply to this program for a chance to research and study data recovered from cores originally brought up by the JR, now located at the Gulf Coast Repository (GCR) in College Station, Texas. Students also practice forms of science communication with the guide of mentors. As a science communicator and fan of snail mail, I ran a craft night teaching students how to make and send science-themed postcards.

Fig. 1) students using watercolor to paint onto 4 by 6 inch board paper, a photo of a thin section slide is in the background. Photo by Dr. Leah Joseph.

For this project, we based the cover image of the postcards off of rock thin section slides. These slides are a slice of a hard rock or mineral that’s been glued to a microscope slide, sanded to 0.03 millimeter thickness, and polished. Thin section slides are used to identify grain size, shape, color, and other physical properties. This helps scientists understand the textural relationships between the rocks and determine the origin or evolution of the parent rock. Thin sections can also be helpful for identifying minerals using cross polarized light (XPL). XPL reduces light reflection and glare, commonly used for sunglasses and professional photography, but in a polarizing microscope, XPL is used to create a dark field causing certain minerals to appear brighter and more visible. Different colors are associated with different minerals, and as the stage of the microscope rotates, light passes through the slide in unique ways aiding scientists with identification. Identifying minerals can help scientists in understanding more about where the rocks came from and how old they are. These thin sections are not only informative, but are incredibly beautiful, making unique and stunning postcard covers.

     

Fig. 2) Examples of thin section slides under a XPL microscope, bronzitite (left) and gabbro (right). Sourced from here.

After the OCA students finished their paintings, my home-made “post card” stamps go on the back, a stamp gets added, and they’re ready to be mailed out. Although most OCA participants this year were U.S. based, they came from all over, ranging from Staten Island to San Francisco to Arizona to Connecticut. In addition to one mentor from New Zealand!  For many of these students this was their first time traveling on their own, and their first time forming long-distance connections. With these scientific postcards, OCA students can stay connected by reminding each other of the science they learned together. My experience on the JR taught me great things about geological research, but it also gave me life long connections that I cherish. Although the JR is gone, its legacy lives on in our memories and the ways we stay connected with friends. I’m grateful to know that even without an international ship, I’m still able to add friends to my address book.

     

Fig. 3) Examples of participant made postcards

Written by Kellan Moss

New Friends, New Addresses

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Ocean Acidification

Color Traditions with Munsell Soil-Color Charts

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Fig. 1) an open page of the Munsell Soil-Color Chart book

The Munsell Color Chart has been the national standard and official color system for soil research in the U.S. since the 1930s. For nearly 100 years, geologists and soil scientists have taken these color chip pages into the field to better understand the Earth they are studying, so it comes as no surprise that it is the standard for recording ocean cores brought up by the JOIDES Resolution.

Upon first glance, these charts may look like a page of free paint sample strips you can find at your local hardware store, but they are critical to classifying sediment and understanding the environments they came from and can cost several hundred dollars. The Munsell Color System is a method of numerically describing colors. It specifies colors based on hue, value, and chroma and measures them in a three dimensional space. Hue refers to the dominant color of the soil, value is the lightness of the color (scaled 0-10; 0 being black and 10 being white), and chroma is the intensity or saturation of the color.

Fig. 2) A 3D model representation of the Munsell Color System

There are five primary hues, red, yellow, green, blue, and purple, and five intermediate hues, which are a combination of primary hues such as yellow-red (YR) or green-yellow (GY). The hue of a color is represented as a ring and as the rings go up and down a vertical axis, the value of the color changes. As the color moves horizontally from the vertical axis, chroma or saturation becomes stronger or weaker. A color is specified by listing the three numbers or letters for hue, value, and chroma in that order. In the soil color chart, these number letter combinations correspond with a color. For instance, in figure 1, a 7.5YR 5/6 is also called “strong brown” (seen on the left page, bottom right). The names of colors used in weekly expedition reports are not arbitrary or subjective, they are specific and can be easily and accurately charted by anyone with a Munsell Chart reading the report.

Useful or Just Tradition?

The Munsell Color System has limitations. There are a distinct number of samples and the spacing between colors are large, making it difficult to measure thresholds. This inspired new color measuring methods to develop like CIELAB. Read more about CIELAB and what it means here (blog post “Color Science and Ocean Cores”). Changes to the Munsell system were made, doubling the number of hues in Munsell’s original book from 20 to 40, but CIELAB was already on its way to mainstream.

However, it’s still true that Munsell has been the soil color standard for nearly 100 years. That’s 100 years of geological and earth science research using this method of recording color. If scientists were to change to a system like CIELAB, it would mean having to constantly convert units when comparing previous research. Scientists compare and reference previous work all the time. Comparing sediment core colors from different sites can help support their own scientific findings. So switching to a different color recording method would mean converting all previous research. But is that a good enough reason to stick to tradition?

CIELAB creates a standard observer, which is an averaging of color matching that helps set a base value for recordings. This helps create the most accurate color reading on something such as an ocean core. Using color charts opens up the possibility for disagreements as no two human eyes see colors the same. And this really happens! In 2024 while aboard the JOIDES Resolution, EXP401 sedimentologists held long discussions about shades of grey they were recording differently.

Fig. 3) Photos of “The Great Grey Debate” on EXP401 by Dr. Patty Standring

Machines can record accurately and consistently, so why not switch to CIELAB? Well, expensive machines that use CIELAB, like the Section Half Multi-Sensor Logger (SHMSL) take anywhere from seven minutes to hours, recording only one core at a time. When on a two month cruise, pulling up hundreds of meters of core, time is crucial. Cores dry out and potentially change color as they dry, so it’s important to record fresh colors.

The color of a core can tell scientists so much information so quickly.

“Gradual color changes helped us to identify where we saw facies changes on a larger scale. There were very obvious cyclical color changes at Site U1385 that helped establish that the cores preserved a really good orbitally-driven sediment record. Color differences are also really useful when looking at different grain sizes that help identify turbidites and other sedimentary structures, and burrows from bioturbating organisms,” (Standring)

It’s important that scientists record these fresh colors as quickly and efficiently as possible. Although debates about the color grey can happen, these color discussions and international collaborations are what scientific research is all about. After 100 years, Munsell will stay the golden standard, not because it’s what we’ve always done, but because it’s still the best.

Written by Kellan Moss

Thank you to Dr. Patty Standring and Natacha Fabregas for help with this research

Sources:

Berns, R. S. (2016). Color science and the visual arts a guide for conservators, curators, and the curious. Los Angeles Getty Conservation Institute.

EXP 401 Sedimentologists: Dr. Patty Standring ad Natacha Fabregas

Featured Image: MerlinOne Archive

Fig. 1 Image: Here

Fig. 2 Image: Here

Fig. 3 Images: Dr. Patty Standring from EXP401

Color Traditions with Munsell Soil-Color Charts

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Ribbegople, Rippenqualle or Comb Jelly: Whatever You Call Mnemiopsis leidyi, You Should Be Concerned

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In early July at Kerteminde, most of the individuals I observed were longer than 10 cm, including one close to 15 cm. Their size, and their timing, deserve immediate attention.

⚠ One out of many large speciments I got from Kerteminde (Javidpour, July 2026)

It does not matter whether you call it ribbegople in Danish, Rippenqualle in German or comb jelly in English. The species is the same: Mnemiopsis leidyi. And what I have observed in Kerteminde this summer should concern us. During our current summer field course at the Marine Research Centre, I have repeatedly seen unusually large individuals of M. leidyi around the pier. Most of the animals I observed were longer than 10 cm, even bigger than the one I photographed.

Yes, yes, a pier observation is not a formal population survey….I know. We still need systematic sampling to determine the abundance, distribution and size structure of the population. Nevertheless, the observation is striking because both the size of the animals and the timing of their appearance are unusual, said by someone who is studying this species for the last 20 years.

This is happening earlier than expected

In previous years, the maximum population size of M. leidyi generally occurred several weeks later, mainly during August and early September. Our previous research, including work based on daily sampling, showed a clear seasonal development of the population. The timing varies among years and is influenced by environmental conditions, including winter temperature. Temperature is particularly important because it strongly affects the metabolism of M. leidyi. At warmer temperatures, individuals use their carbon reserves much faster and therefore require more food to maintain themselves and grow. This year, however, the pattern appears to be different. We are seeing very large individuals already in early July. We do not yet know whether this is a local aggregation, an unusually early bloom, transport from another area, particularly favourable feeding conditions or a combination of these factors. But it is a signal that deserves attention.

What does it take to grow by one centimetre?

It is tempting to ask how much energy an individual needs to add one centimetre to its body. The answer is not straightforward because one centimetre of length is not a fixed amount of biomass. Growing from 5 to 6 cm is not the same as growing from 14 to 15 cm…OK? However, we can make a rough carbon-budget calculation using a published relationship between the length and body-carbon content of M. leidyi:

Body carbon in milligrams = 0.0017 × body length in millimetres²·⁰¹³⁸

According to this relationship, an individual measuring 10 cm contains approximately 18.1 mg of carbon. At 11 cm, it contains about 21.9 mg. Adding this single centimetre therefore represents an increase of approximately 3.8 mg of body carbon. If we assume that the animal assimilates approximately 40% of the carbon it consumes, it would need to ingest at least ~10 mg of prey carbon to produce this additional tissue. Using an approximate value of 1 micrograms of carbon for a small copepod, this would correspond to more than 10,000 copepods.

For an already large individual growing from 14 to 15 cm, the estimated increase is approximately 5.3 mg of body carbon. At the same assimilation efficiency, that would require at least 13.3 mg of prey carbon: the equivalent of roughly 15,000 small copepods.

These calculations are only rough, conservative estimates. They are not complete energy budgets. They do not include the food needed for respiration, movement, reproduction, mucus production, excretion or unsuccessful feeding. The real prey requirement would therefore be considerably higher. The important point is that an individual measuring 15 cm represents a substantial transfer of material from the surrounding planktonic food web into gelatinous biomass. One additional centimetre is not “just” one centimetre.

Our students are tracing the food web

The timing of these observations coincides with our summer field course. The students are now collecting M. leidyi, fish, other gelatinous organisms and potential prey for stable-isotope analysis. By comparing carbon and nitrogen isotope values, we hope to obtain a rough picture of the relationships within the local food web. Carbon isotopes can help us trace the original sources of the material entering the food web, while nitrogen isotopes can provide information about relative trophic position.

This will not give us a direct photograph of one organism eating another. Stable-isotope values represent assimilated food over time, and their interpretation depends on appropriate baselines and turnover rates. Nevertheless, combined with information about size, abundance, prey availability and experimental feeding, they can help us understand where M. leidyi is obtaining its biomass and which organisms may be affected. …In simple terms, we are trying to determine who might be eating whom, and where this unusually large population fits into the food web.

Competition with fish is only part of the problem

The concern is not limited to competition for zooplankton. Mnemiopsis leidyi consumes copepods and other small planktonic animals that are also important food for pelagic fish. When the ctenophores are abundant, they can therefore compete directly with fish for prey. Our experiments have also demonstrated that M. leidyi can potentially feed directly on the early life stages of fish. In the study by my previous PhD student, the ctenophores captured and digested Baltic herring yolk-sac larvae. Predation was related to ctenophore size and was not simply eliminated when alternative copepod prey were available. This means that M. leidyi may/can affect fish populations in two ways: by consuming the food needed by fish and by consuming fish eggs or larvae directly.

A recent study by Lucila Sobrero and colleagues in Argentina, within the native range of M. leidyi, found a similar pattern. Their experiments showed size-dependent predation on fish eggs and larvae. Larger ctenophores consumed more eggs. Some eggs were later regurgitated, but many were no longer viable, while fish larvae were retained and digested. These findings are particularly relevant to what we are observing in Kerteminde. The size of an individual is not merely an interesting measurement. It can influence what that individual is capable of capturing and how strongly it affects the surrounding ecosystem. A population consisting of fewer but much larger individuals may still exert substantial pressure on zooplankton, fish eggs and fish larvae.

We need to investigate use, not only control

For several years, I have tried to obtain funding to investigate innovative approaches to this invasive species.

Once M. leidyi is well established, we may not be able to control its regional spread or completely prevent its blooms. But that does not mean that we have no options. We should investigate whether at least part of this recurring biomass can be collected and converted into something useful.

This is not a proposal for a miracle solution. Any utilisation strategy would have to be tested carefully. It must not encourage the further spread of the species, create damaging bycatch or provide an economic incentive to maintain an invasive population. We also need to understand the environmental costs of collection, transport and processing.

But these are exactly the questions that research funding should allow us to answer.

So far, my attempts to secure support for this work have been unsuccessful. Funding agencies do not seem to sense the urgency of studying approaches whose benefits may not be immediate or easily visible. and EPAs do not have any resource to invest in this part. The contrast with events on land is striking. This week, the oak processionary moth, the so-called “larva from hell”, has attracted considerable attention in Odense. Its microscopic hairs can cause rashes and allergic reactions, residents have reported serious discomfort, and a kindergarten has reportedly had to close temporarily. Those concerns are real and deserve a response.

But the case also illustrates how differently we react to environmental threats.

When the impact appears visibly on human skin, the urgency is immediately understood. When ecological damage develops below the surface of the sea, in the form of disappearing zooplankton, altered food webs, consumed fish eggs or reduced larval survival, it is much easier to overlook.

Marine ecosystem changes are often gradual, underwater and largely invisible to the public. By the time their consequences become obvious, the opportunity for early and relatively inexpensive action may already have passed.

Concern does not mean panic

One photograph and a series of observations from one pier do not prove that an ecological crisis is underway. I am not suggesting that they do. But science should not have to wait for undeniable damage before investigation becomes urgent.

The unusually large M. leidyi appearing in Kerteminde this July give us an opportunity to act early. We need systematic monitoring of their abundance and size distribution. We need to measure the available prey field. We need to determine their trophic position and investigate possible consequences for fish recruitment. And we need to explore whether biomass that we may be unable to prevent could be collected and used responsibly.

Whatever language we use and whatever name we give it, the message is the same:

We should measure early, investigate early and support innovative solutions while the warning is still only a warning, not after it has become a crisis.

Relevant publications

Javidpour, J. et al. (2009). “Seasonal changes and population dynamics of the ctenophore Mnemiopsis leidyi after its first year of invasion in the Kiel Fjord, Western Baltic Sea.” Biological Invasions.

Javidpour, J. et al. (2020). “Cannibalism makes invasive comb jelly, Mnemiopsis leidyi, resilient to unfavourable conditions.” Communications Biology.

Stoltenberg, I. et al. (2024). “Predation on Baltic Sea yolk-sac herring larvae (Clupea harengus) by the invasive ctenophore Mnemiopsis leidyi.” Fisheries Research.

Sobrero, L. et al. (2025). “Predatory impact on ichthyoplankton by Mnemiopsis leidyi is size-dependent: an experimental approach.” Marine Ecology Progress Series.

Ribbegople, Rippenqualle or Comb Jelly: Whatever You Call Mnemiopsis leidyi, You Should Be Concerned

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