Anton und ich bringen soeben CTD-Cast Nummer 45 an das Tageslicht. Während wir gerade wieder einmal mit viel Enthusiasmus frisch gezapfte Flaschen durchschütteln, meine ich, ein nett gemeintes, aber deutliches Kopfschütteln bei Jamileh erkennen zu können, als sie uns ein Guten Morgen zulächelt. Das denken sich hier scheinbar alle: Bereits 45 CTD-Einsätze? Und viele davon an ein- und derselben Stelle? Warum das Ganze? Wir müssten das Wasser doch kennen, sobald wir es einmal „vermessen“ haben, oder? Naja, irgendwie schon.
„Unsere“ CTD, von den Biologen bevorzugt auch „Wasserschöpfer“ genannt, wird seitlich aus dem Hangar herausgefahren, herabgelassen und misst in der Basisversion quasi kontinuierlich (mit 24 Hz) Leitfähigkeit (Salzgehalt), Temperatur und Druck (Tiefe) (Conductivity, Temperature, Depth), idealerweise hinunter bis zum Meeresboden. Darüber hinaus werden Sauerstoffgehalt und Fluoreszenz gemessen, was eine Abschätzung der biologischen Produktivität ermöglicht (siehe Blogeinträge zu „Mikrokreaturen“ von Nicole und Manfred). Als praktische Zugabe können mithilfe der 24 Niskin-Flaschen Wasserproben in verschiedenen Tiefen genommen werden (Manfred ist da nebenbei bemerkt mit Abstand unser bester Kunde).
Für Ozeanographen sind aber vor allem die kontinuierlichen Messungen von Temperatur und Salzgehalt von entscheidender Bedeutung, da wir daraus z.B. ableiten können, wie stabil das Wasser geschichtet ist oder woher Wassermassen und geostrophische Strömungen kommen. Dies sind wichtige Informationen, die Rahmenbedingungen darstellen, die das lokale Ökosystem stark beeinflussen. Um eine möglichst hohe Genauigkeit der physikalischen Messungen zu erreichen, nehme ich auch selbst Wasserproben, allerdings „nur“ zur späteren Kalibrierung der verschiedenen Sensoren und nicht zur Analyse der darin enthaltenen kuriosen Lebewesen.

Die meisten Einsätze wurden bisher in Küstennähe in einer Tiefe von 1500 Metern gefahren. Die folgende Abbildung zeigt eines unserer wertvollen Tiefseeprofile bis in eine Tiefe von fast 3300 Metern. Hier bilden die obersten 100m die so genannte „Deckschicht“ (Mixed Layer), in welcher alle gemessenen Größen durch den Wind gut durchmischt sind. . Wir beobachten, dass die Tiefe der Deckschicht variiert, aber grundsätzlich – wie für die Wintermonate in diesen Breiten typisch – relativ mächtig ist. An unserer ersten Station betrug die Deckschichttiefe sogar ca. 200 Meter!

Temperatur (rot), Salz (blau), Sauerstoff (gelb) als auch Chlorophyll (grün) zeichnen praktisch vertikale Linien in das Diagramm. Interessanterweise bildet sich genau an bzw. unter der Deckschicht häufig ein Maximum an Chlorophyll, welches als Indikator für das Vorkommen von Phytoplankton dient (siehe wieder Nicoles und Manfreds Blog-Eintrag). Obwohl Phytoplankton grundsätzlich autotroph, also auf Sonnenlicht angewiesen ist, kann es in dieser recht Tiefen Schicht mit sehr wenig Sonnenlicht überleben. Ein Grund dafür ist der erhöhte Nährstoffgehalt in tieferen Schichten.
Darüber hinaus bildet die Pyknokline direkt unterhalb der Deckschicht eine starke physikalische Barriere für vertikale Vermischung und kann Organismen, die selbst nicht aktiv schwimmen können, praktisch „einsperren“. Die Pyknokline ist die Schicht, in der die Dichte des Wassers mit der Tiefe (hier aufgrund des Temperaturgradienten) sehr schnell zunimmt. Diese Schichten beherbergen eine hohe Spannbreite an Temperatur- und Salzgehalten und werden auch Zentralwasser genannt.
Um Wassermassen zu identifizieren, werden Temperaturen und Salzgehalte in einem sogenannten „T-S Diagramm“ (wie in Abbildung 4) gegeneinander aufgetragen. In unserem Beispiel sieht man gut, dass das Wasser rund um Madeira zu einem großen Teil aus Nordatlantischem Zentralwasser (Eastern North Atlantic Central Water) besteht. Dieses dominiert die Pyknokline im großen Nordatlantischen Wirbel und ist deutlich salzhaltiger als im Südatlantik (vgl. Eastern South Atlantic Central Water). In unserem Profil Nummer 41 (Abbildung 3) fällt aber noch etwas anderes ins Auge. Auf etwa 1100 Metern Tiefe zeigt sich eine Nase mit noch einmal deutlich erhöhtem Salzgehalt, die nicht so recht zum linear verlaufenden Zentralwasser zu passen scheint. Hier macht sich der Einfluss des Mittelmeerwassers (MW) bemerkbar, welches aufgrund der überwiegend starken Verdunstung bei gleichzeitig wenig Niederschlag im Mittelmeerraum besonders hohe Salzgehalte mit sich bringt. Aufgrund dieses hohen Salzgehaltes manifestiert es sich trotz der warmen Temperaturen in größeren Tiefen um typischerweise 1100-1200 Meter. Wir sehen im T-S Diagramm aber auch, dass das Mittelmeerwasser im Süden von Madeira bereits etwas durchmischter, also weniger warm und salzhaltig als direkt am Ausgang des Mittelmeeres ist. Noch tiefer, was wir insbesondere bei unseren ausgedehnteren CTD-Stationen bis auf 3000 Meter und mehr gut beobachten können, findet sich das berühmte Nordatlantische Tiefenwasser (North Atlantic Deep Water). Dieses wird unter anderem durch Tiefenkonvektion im Nordatlantik gebildet und spielt eine zentrale Rolle für die globale thermohaline Zirkulation, und die gesamte Klimadynamik. Es ist für Tiefenwasser relativ „jung“ und damit reich an Sauerstoff (wir sagen gerne „gut ventiliert“) und bildet einen Kontrast zum Sauerstoffminimum, welches wir hier um Madeira auf etwa 800-900 Metern beobachten. Diese Minimumzone entsteht durch Respiration des abgesunkenen organischen Materials, z.B. von dem sonnenlichtabhängigen Phytoplankton in den obersten ~150 Metern. Im Vergleich mit den großen bekannten Sauerstoffminimumzonen im subtropischen Ost-Atlantik und -Pazifik, ist jedoch noch vergleichsweise reichlich Sauerstoff vorhanden.

Nun kennen wir das Profil einer CTD-Station etwas genauer. Im Grunde ist dieses sogar ziemlich repräsentativ für die übrigen 44. Die Frage, warum Anton und ich wie die Wahnsinnigen weiter „CTDs fahren“, bleibt also noch unbeantwortet. Wenn wir jedoch genauer hinschauen, sehen wir, dass die Temperatur- und Salzprofile nicht komplett „glatt“ verlaufen. Tatsächlich entdecken wir kleine wellenförmige Abweichungen. Messungenauigkeiten? Nein. Es sind interne Wellen, die die Profile lebendig machen. Interne Wellen können in jedem stratifizierten Medium auftreten, also Fluide, in denen die Dichte nicht konstant ist. Es gibt zwei rückstellende Kräfte, die auf interne Wellen im Ozean wirken: Gravitation und die Corioliskraft. Hauptantriebe für interne Wellen sind die Gezeiten (wie Ebbe und Flut), dicht gefolgt von Wind. Wir wissen, dass interne Wellen eine entscheidende Rolle für den Energietransport im Ozean spielen. Wie gewöhnliche Oberflächenwellen, können auch interne Wellen brechen. Wenn sie das tun, findet Vermischung statt. Das wiederum kann Nährstoffe transportieren und dadurch die biologische Produktivität beeinflussen. Die Wechselwirkung von internen Wellen mit Topographie (d.h. Inseln wie Madeira) und Strömungen ist sehr komplex und noch nicht vollumfänglich verstanden. Durch eine hohe Anzahl an Stationen zu verschiedenen Zeiten (und Gezeitenstadien) erhalten wir eine bessere räumliche und zeitliche Auflösung des internen Wellenfeldes und können die Prozesse besser verstehen. Deswegen sind wir z.B. Fans von sogenannten „Jo-Jo-CTDs“. Wie bei einem echten Jo-Jo fahren wir die CTD an ein- und derselben Stelle mehrfach direkt hintereinander auf- und ab.

In der obigen Abbildung haben wir sechs direkt aufeinander folgende Profile eines „Jo-Jos“ übereinander geplottet. Man erkennt, dass die Profile auf manchen Tiefen mehr voneinander abweichen, und auf anderen wieder nicht (Knotenpunkte). Den imposantesten Einfluss nehmen interne Wellen auf die Deckschichttiefe, diese kann alleine dadurch innerhalb von Minuten um mehrere zehn Meter variieren.
Besonderer Nervenkitzel kommt auf, wenn zur „Eddy-Jagd“ aufgerufen wird. Das klingt jetzt martialischer, als es gemeint ist. Eddies sind ozeanische Wirbel, die rund um Madeira einen Durchmesser von ca. 50 Kilometern erreichen, mit der Topographie (Inseln) sowie internen Wellen interagieren und bekanntermaßen die Biodiversität beeinflussen können. Sie entstehen über einen Zeitraum von Tagen / Wochen und sind leider kaum vorhersagbar. Daher checken wir täglich Satelliten- und Modelldaten für die Region, um ein mögliches Feature zu identifizieren, und falls möglich, in situ mit dem Schiff zu beproben. Starke Eddies können ein Signal in der Meereshöhe, den Oberflächentemperaturen und im Chlorophyll erzeugen.
Unsere Kollegen vom Ozeanographischen Institut Madeira unterstützen uns vor Ort mit regionalen Satelliten- und Modelldaten (siehe https://oomdata.arditi.pt/msm126/ ). Es ist insgesamt beeindruckend, wie gut die Zusammenarbeit an Bord und darüber hinaus funktioniert! In der Nacht vom 13. auf den 14. Februar fand bereits eine „Eddy-Jagd“ statt. Allerdings war das Satellitensignal schwach und dementsprechend konnten wir vor Ort mit unserem schiffseigenen ADCP (das Ozeanströmungen bis in knapp 1000 Meter Tiefe misst) keinen starken, kohärenten Wirbel nachweisen.(Randbemerkung: Es wurde dabei aber ein anderes spannendendes feature (mutmaßlich eine kräftige interne Welle) in der Deckschicht ausgemacht, welches wir nun analysieren.)

In einem der nächsten Blogeinträge wollen wir euch beweisen, dass unsere lieb gewonnene CTD dank raffinierter Tunings, unter anderem mit hochauflösenden Kamerasystemen, rein „objektiv“ etwas ganz Besonderes ist. Dann klären wir auf, warum auch Anton, obwohl er kein physikalischer Ozeanograph ist, gerne „Jo-Jos“ fährt, und es gibt endlich wieder Fotos von Wassertierchen!
Viele Grüße von Bord der MARIA S. MERIAN,
Marco Schulz und Anton Theileis
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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