Geht man auf eine Wanderung in den Bergen, so schaut man sich meistens als ersten Schritt eine Karte an. Genauso ist es auch auf dem Ozean wichtig eine Karte zu haben. Nicht nur eine Karte, in der die Küsten und Inseln verzeichnet sind, sondern vor allem eine detaillierte Karte der Topografie des Meeresbodens. Während Mitte des 19. Jahrhunderts bis Anfang des 20. Jahrhunderts Tiefenmessung noch mit einem Gewicht am Ende eines langen Seils durchgeführt wurde, wird heute in den meisten Fällen das vom Kieler Dr. Alexander Behm 1913 patentierte Echolot genutzt.
Die beste und auch wissenschaftlich anerkannte bathymetrische Daten-Zusammenstellung erstellt GEBCO (englisch: General Bathymetric Chart of the Oceans). Der Datensatz basiert auf zusammengetragenen Daten aus Schiffs-Tiefenmessungen und wurde erstmals vor 120 Jahren der Öffentlichkeit vorgestellt. Heutzutage besteht dieser Datensatz weitestgehend aus so genannter prädizierter Bathymetrie. Das bedeutet, dass Satellitenmessungen gemacht werden, die im Anschluss mit von Schiffen gemessener Bathymetrie verifiziert und ergänzt werden können. Die Satelliten können über verschiedene physikalische Zusammenhänge aus der gemessenen Meeresspiegelhöhe ableiten, ob sich unter Wasser ein Seamount befindet. Dieses Verfahren ermöglicht zwar den gesamten Ozean abzubilden, ist aber sehr ungenau. Seamounts mit einer Größe unter 2 km können zum Beispiel nicht gemessen werden. Der GEBCO Datensatz wird mittlerweile jedes Jahr erneuert. Der einzige Nachteil ist, dass es ihn an detaillierten Metadaten mangelt. Metadaten sind Hintergrundinformationen, die zum Beispiel angeben, von welchem Institut oder auf welchem Schiff die zur Verfügung gestellten Daten gemessen wurden.
Da der Datensatz in großen Teilen auf Schiffsmessungen basiert, ist er stark abhängig von Schiffsrouten, zwischen denen sich teilweise sehr große Lücken befinden. Es sind erst circa 20% des Meeresbodens auf diese Weise vermessen (Mayer et. al 2018). Auf dieser Reise wollen wir einige dieser Lücken kartieren. Genauer gesagt, wollen wir sogenannte Seamounts kartieren.
Seamounts sind unter Wasser liegende Berge meist vulkanischen Ursprungs. Sie sind typischerweise kegelförmig, haben oft Krater, lineare Kämme oder flache Gipfel. Die Form ist häufig abhängig von der Entstehung des Seamounts. Geformt werden sie an Orten, an denen es tektonische Aktivitäten gibt, so zum Beispiel in der Nähe von ozeanischen Rücken, Inselbögen oder an Stellen, wo unter der tektonischen Platte heißes Material aus dem Erdmantel aufsteigt. Seamounts, die in der Nähe von Plattengrenzen entstehen, also dort, wo die Lithosphäre (die Erdkruste und der äußerste Teil des Erdmantels) noch frisch entstanden und dünn ist, sind meistens eher klein. Klein heißt in diesem Fall weniger als 2.5 km Höhe. Größere Seamounts mit 3-10 km Höhe entstehen häufig an Stellen, wo die Lithosphäre schon älter und dicker ist. Obwohl nicht genau bekannt ist, wie viele Seamounts es gibt, ist eines sicher: es sind sehr viele!
Aufgrund ihres vulkanischen Ursprungs sind Seamounts aus geologischer Sicht sehr interessant, da sie einen Einblick in die Zusammensetzung und die Temperatur des Erdmantels geben können. Auch für ozeanographische Betrachtungen sind Seamounts wichtig, da die Bathymetrie Einfluss auf Strömungen und Vermischungsprozesse hat. So können Seamounts als Barrieren fungieren, die verhindern, dass kaltes Tiefenwasser sich mit dem warmen Oberflächenwasser mischen kann. Zu guter Letzt sind sie auch Mittelpunkt eines diversen Ökosystems. Das liegt daran, dass nährstoffreiches Tiefenwasser an ihnen aufsteigt (diesen Prozess nennt man Upwelling) und somit die perfekte Grundlage für Fische und eine vielfältige Flora und Fauna bildet.
Jetzt wissen wir also, warum wir uns für Seamounts interessieren sollten, dass es unglaublich viele von ihnen gibt und, dass viele noch nicht kartiert sind.

Auf unserer geplanten Reiseroute kommen wir an einigen Stellen vorbei, wo Seamounts vermutet werden. Durch nur leichte Kursänderung ist es möglich über einige dieser Seamounts hinweg zu fahren und sie so mit dem Schiffsecholot zu vermessen. Dabei wird ein akustisches Signal zum Meeresboden gesendet, das am Boden reflektiert und dann bei Rückkehr zum Schiff wieder empfangen wird. So kann man durch die gemessene Zeit zwischen Senden und Empfangen den Abstand zwischen Schiff und Meeresboden messen. Dieses Prinzip wird auch hier auf der Maria S. Merian genutzt, mit dem Unterschied, dass nicht nur ein Signal, sondern ein ganzer Fächer von Signalen ausgesendet wird. Damit kann ein Streifen mit einer Breite sechs Mal so groß wie die Wassertiefe vermessen werden. In unserem derzeitigen Messgebiet beträgt die Wassertiefe 2500-3000 m was einem kartierten Streifen von 15 bis 18 km Breite entspricht.
Wir befinden uns im Moment in der Nähe des Mittelozeanischen Rückens, also an einem Ort, wo neue Lithosphäre entsteht. Wie wir bereits gelernt haben, werden die hier zu findenden Seamounts eher kleiner sein. In diesem Gebiet ist auch die Anzahl und Dichte der vorhergesagten Seamounts deutlich größer. Unser erster „überfahrende“ kleine Seamount, noch weit entfernt von dem Mittelozeanischen Rückens, zeigte einen flachen Gipfel mit einer ungefähren Höhe von 450 m. Mit 7.5 km breite sowie 8 km Länge war er fast rund und äußerst sehenswert. In wie weit dieser Seamount in Zukunft weiter erforscht wird, wird sich zeigen.

Auf dieser Fahrt kümmert sich Daniel und Marianne vom „Unterwegs“-Forschungsdaten Projektes der Deutschen Allianz Meeresforschung (DAM) um alles, was mit den Seamounts und dem Fächerecholot zu tun hat. Häufig werden Fächerecholot Daten auch nebenbei erhoben, wenn der Schwerpunkt der Ausfahrt nicht in der Vermessung des Meeresbodens liegt. Im Rahmen des Projekts arbeiteten beide daran, dass diese Daten erhoben und nach der Forschungsfahrt für die Wissenschaft verfügbar gemacht werden. Beide arbeiten für PANGAEA einem Datenrepositorium für Erd- und Umweltdaten.
English version:
If you go on a hike in the mountains, you usually look at a map as the first step. It is also important to have a map being on the ocean. Not only a map listing the coasts and islands, but above all a detailed map of the topography of the seabed. During the middle of the 19th century to the beginning of the 20th century, depth measurement was still carried out with a weight at the end of a long rope, but today the echo sounder patented by Dr. Alexander Behm from Kiel in 1913 is used in most cases.
The most accurate and scientifically recognized bathymetric data collection is produced by GEBCO (General Bathymetric Chart of the Oceans). The dataset is based on collected data from vessel depth measurements and was first presented to the public 120 years ago. Today, this data set consists largely of so-called predicated bathymetry. This means that satellite measurements are made, which can then be verified and supplemented with bathymetry measured by ships. The satellites can derive from the measured sea level via various physical relationships whether a seamount is underwater. This method allows us to map the entire ocean, but it is very inaccurate. Seamounts less than 2 km in size, for example, cannot be measured. The GEBCO dataset is now renewed every year. The only drawback is that it lacks detailed metadata. Metadata are background information indicating, for example, by which institute or on which vessel the data provided were measured.
Since the data set is largely based on ship measurements, it is highly dependent on ship routes, some of which have very large gaps. Only about 20% of the seabed have been measured in this way (Mayer et. al 2018). On this journey we want to map some of these gaps. More specifically, we want to map so-called seamounts.
Seamounts are submerged mountains of volcanic origin. They are typically conical, often with craters, linear ridges or shallow peaks. The shape often depends on the origin of the seamount. They are formed in places where tectonic activity occurs, such as near oceanic ridges, arch islands, or at places where hot material rises from the Earth’s mantle beneath the tectonic plate. Seamounts that form near plate boundaries, i. e. where the lithosphere (the Earth’s crust and the outer part of the Earth’s mantle) is still fresh and thin, tend to be rather small. Small in this case means less than 2. 5 km altitude. Larger seamounts with a height of 3-10 km often form in places where the lithosphere is older and thicker. Although it is not known exactly how many seamounts there are, one thing is certain: there are many!
Due to their volcanic origin, seamounts are very interesting from a geological point of view, as they can provide insight into the composition and temperature of the Earth’s mantle. Seamounts are also important for oceanographic observations, as bathymetry influences currents and mixing processes. Seamounts can act as barriers that prevent cold deep water from mixing with warm surface water. Finally, they are also the centre of a diverse ecosystem. This is because nutrient-rich deep water rises at their flanks (a process called upwelling) and thus forms the perfect basis for fish and a diverse flora and fauna.
So now we know why we should be interested in seamounts, that there are many of them out there, and that a lot of them have not yet been mapped.

On our planned itinerary we pass some places where seamounts are suspected. By only slight course changes it is possible to drive over some of these seamounts and to measure them with the ship echo sounder. An acoustic signal is sent to the seabed, which is reflected on the ground and then received when returning to the ship. Thus, the measured time between sending and receiving can be used to measure the distance between the ship and the seabed. This principle is also used here on the Maria S. Merian, with the difference that not only one signal, but a whole range of signals is emitted. This allows a strip with a width of six times as large as the water depth to be measured. In our current measuring area the water depth is 2500-3000 m which corresponds to a mapped strip of 15 to 18 km wide.
We are at the moment near the Mid-Oceanic Ridge, a place where new lithosphere is forming. As we have already learned, the seamounts to be found here will tend to be smaller. In this area, the number and density of predicted seamounts is also significantly higher. Our first mapped small seamount, still far from the Mid-Oceanic Ridge, showed a shallow peak with an approximate height of 450 m. With 7. 5 km wide and 8 km long, it was almost round and extremely worth seeing.

On this trip, Daniel and Marianne from the “Underway” research data project of the German Marine Research Alliance (DAM) will take care of everything that has to do with the seamounts and the Multibeam Echo Sounder. Frequently, Multibeam data is collected even if the focus of the research is not in the measurement of the seabed. As part of the project, Daniel and Marianne worked to collect these data and make them available to scientists after the research trip. Both are part of PANGAEA, a data repository for earth and environmental data.
Quellen/Sources:
- Gevorgian, J., Sandwell, D. T., Yu, Y., Kim, S.-S., & Wessel, P. (2023). Global distribution and morphology of small seamounts. Earth and Space Science, 10, e2022EA002331. https://doi.org/10.1029/2022EA002331
- Mayer, L.; Jakobsson, M.; Allen, G.; Dorschel, B.; Falconer, R.; Ferrini, V.; Lamarche, G.; Snaith, H.; Weatherall, P. The Nippon Foundation—GEBCO Seabed 2030 Project: The Quest to See the World’s Oceans Completely Mapped by 2030. Geosciences 2018, 8, 63. https://doi.org/10.3390/geosciences8020063
- Damaske, D. (2013): Bathymetry and short term changes of submarine seafloor structures in the area of the former Larsen ice shelf, north west Weddel Sea, Master thesis, http://hdl.handle.net/10013/epic.67a7bbd6-5ada-4764-a961-519e334d5c56
- https://oceanexplorer.noaa.gov/facts/seamounts.html
Ocean Acidification
New Friends, New Addresses
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
Ocean Acidification
Color Traditions with Munsell Soil-Color Charts

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