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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.

2. Hier wird “gewinklert”: Per Titration wird der Sauerstoffgehalt von Wasserproben bestimmt. Die Ergebnisse werden verwendet, um die Messergebnisse der CTD-Sensoren zu kalibrieren, welche oftmals einen Offset haben. Foto: Marco Schulz

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!

Abb.3: Ein beispielhaftes CTD-Profil vom 23. Februar südlich von Madeira, bis etwa 3300 Meter Tiefe. Enthält Fluoreszenz (grün), Sauerstoff (gelb), Salzgehalt (blau) und Temperatur (rot)

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.

Abb. 4: Das Temperatur-Salzgehalt Diagramm zu Profil 41 (Abb. 3). Mit den Buchstaben sind die typischen Temperatur- und Salzwerte bekannter Wassermassen markiert (siehe Text).

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.

Abb. 5: Eine unserer “Jo-Jo CTD’s”. Wie Abbildung 3, allerdings sechs CTD-Profile übereinander geplottet.

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.)

Abb. 6: Eddy hunt! Der Plan zum „spontanen“ Vermessen des potentiellen Wirbels. Es bot sich ein schwaches Satellitensignal für eine negative Anomalie im Meeresspiegel (blaue Konturen). Die rote Linie gibt den geplanten Track und die lila Dreiecke die geplanten CTD-Stationen an.

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

Als Physikalischer Ozeanograph allein unter Biologen

Ocean Acidification

What is the High Seas Treaty and Why Does It Matter?

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You may have seen headlines recently about a new global treaty that went into effect just as news broke that the United States would be withdrawing from a number of other international agreements. It’s a confusing time in the world of environmental policy, and Ocean Conservancy is here to help make it clearer while, of course, continuing to protect our ocean.

What is the High Seas Treaty?

The “High Seas Treaty,” formally known as the Agreement on the Conservation and Sustainable Use of Marine Biological Diversity of Areas Beyond National Jurisdiction (BBNJ) Agreement, went into effect on January 17, 2026. We celebrated this win last fall, when the agreement reached the 60 ratifications required for its entry into force. (Since then, an additional 23 countries have joined!) It is the first comprehensive international legal framework dedicated to addressing the conservation and sustainable use of the high seas (the area of the ocean that lies 200 miles beyond the shorelines of individual countries).

To “ensure the conservation and sustainable use of marine biological diversity” of these areas, the BBNJ addresses four core pillars of ocean governance:

  1. Marine genetic resources: The high seas contain genetic resources (genes of plants, animals and microbes) of great value for pharmaceuticals, cosmetics and food production. The treaty will ensure benefits accrued from the development of these resources are shared equitably amongst nations.
  2. Area-based management tools such as the establishment of marine protected areas (MPAs) in international waters. Protecting important areas of the ocean is essential for healthy and resilient ecosystems and marine biodiversity.
  3. Environmental impact assessments (EIA) will allow us to better understand the potential impacts of proposed activities that may harm the ocean so that they can be managed appropriately.
  4. Capacity-building and the transfer of marine technology with particular emphasis on supporting developing states. This section of the treaty is designed to ensure all nations benefit from the conservation and sustainable use of marine biodiversity through, for example, the sharing of scientific information.

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Why is the High Seas Treaty Important?

The BBNJ agreement is legally binding for the countries that have ratified it and is the culmination of nearly two decades of negotiations. Its enactment is a historic milestone for global ocean governance and a significant advancement in the collective protection of marine ecosystems.

The high seas represent about two-thirds of the global ocean, and yet less than 10% of this area is currently protected. This has meant that the high seas have been vulnerable to unregulated or illegal fishing activities and unregulated waste disposal. Recognizing a major governance gap for nearly half of the planet, the agreement puts in place a legal framework to conserve biodiversity.

A map of the globe depicting the areas designated as high seas versus exclusively an economic zone. The high seas represent about two-thirds of the global ocean.

As it promotes strengthened international cooperation and accountability, the agreement will establish safeguards aimed at preventing and reversing ocean degradation and promoting ecosystem restoration. Furthermore, it will mobilize the international community to develop new legal, scientific, financial and compliance mechanisms, while reinforcing coordination among existing treaties, institutions and organizations to address long-standing governance gaps.

How is Ocean Conservancy Supporting the BBNJ Agreement?

Addressing the global biodiversity crisis is a key focal area for Ocean Conservancy, and the BBNJ agreement adds important new tools to the marine conservation toolbox and a global commitment to better protect the ocean.

Ocean Conservancy’s efforts to protect the “ocean twilight zone”—an area of the ocean 200-1000m (600-3000 ft) below the surface—is a good example of why the BBNJ agreement is so important. The ocean twilight zone (also known as the mesopelagic zone) harbors incredible marine biodiversity, regulates the climate and supports the health of ocean ecosystems. By some estimates, more than 90% of the fish biomass in the ocean resides in the ocean twilight zone, attracting the interest of those eager to develop new sources of protein for use in aquaculture feed and pet foods.

An illustration of the zones of the ocean floor, depicting depth in meters/feet on the left and the layers from light blue to dark blue and orange, listed as follows: Continental Shelf (Epipelagic Zone: The Sunlight Zone; Mesopelagic Zone: The Twilight Zone), Continental Slope (Bathypelagic Zone: The Midnight Zone); Continental Rise (Abyssopelagic Zone: The Abyss), Ocean Basin, Hadal Zone: The Trenches.

Done poorly, such development could have major ramifications for the health of our planet, jeopardizing the critical role these species play in regulating the planet’s climate and sustaining commercially and ecologically significant marine species. Species such as tunas (the world’s most valuable fishery), swordfish, salmon, sharks and whales depend upon mesopelagic species as a source of food. Mesopelagic organisms would also be vulnerable to other proposed activities including deep-sea mining.

A significant portion of the ocean twilight zone is in the high seas, and science and policy experts have identified key gaps in ocean governance that make this area particularly vulnerable to future exploitation. The BBNJ agreement’s provisions to assess the impacts of new activities on the high seas before exploitation begins (via EIAs) as well as the ability to proactively protect this area can help ensure the important services the ocean twilight zone provides to our planet continue well into the future.

What’s Next?

Notably, the United States has not ratified the treaty, and, in fact, just a few days before it went into effect, the United States announced its withdrawal from several important international forums, including many focused on the environment. While we at Ocean Conservancy were disappointed by this announcement, there is no doubt that the work will continue.

With the agreement now in force, the first Conference of the Parties (COP1), also referred to as the BBNJ COP, will convene within the next year and will play a critical role in finalizing implementation, compliance and operational details under the agreement. Ocean Conservancy will work with partners to ensure implementation of the agreement is up to the challenge of the global biodiversity crisis.

The post What is the High Seas Treaty and Why Does It Matter? appeared first on Ocean Conservancy.

https://oceanconservancy.org/blog/2026/02/25/high-seas-treaty/

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Ocean Acidification

Hälsningar från Åland och Husö biological station

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On Åland, the seasons change quickly and vividly. In summer, the nights never really grow dark as the sun hovers just below the horizon. Only a few months later, autumn creeps in and softly cloaks the island in darkness again. The rhythm of the seasons is mirrored by the biological station itself; researchers, professors, and students arrive and depart, bringing with them microscopes, incubators, mesocosms, and field gear to study the local flora and fauna peaking in the mid of summer.

This year’s GAME project is the final chapter of a series of studies on light pollution. Together, we, Pauline & Linus, are studying the effects of artificial light at night (ALAN) on epiphytic filamentous algae. Like the GAME site in Japan, Akkeshi, the biological station Husö here on Åland experiences very little light pollution, making it an ideal place to investigate this subject.

We started our journey at the end of April 2025, just as the islands were waking up from winter. The trees were still bare, the mornings frosty, and the streets quiet. Pauline, a Marine Biology Master’s student from the University of Algarve in Portugal, arrived first and was welcomed by Tony Cederberg, the station manager. Spending the first night alone on the station was unique before the bustle of the project began.

Linus, a Marine Biology Master’s student at Åbo Akademi University in Finland, joined the next day. Husö is the university’s field station and therefore Linus has been here for courses already. However, he was excited to spend a longer stretch at the station and to make the place feel like a second home.

Linus & Pauline on Husö (left) and our home for the summer season on Husö, Nya Villan (right). (c) Pauline Wasle.

Our first days were spent digging through cupboards and sheds, reusing old materials and tools from previous years, and preparing the frames used by GAME 2023. We chose Hamnsundet as our experimental site, (i.e. the same site that was used for GAME 2023), which is located at the northeast of Åland on the outer archipelago roughly 40 km from Husö. We got permission to deploy the experiments by the local coast guard station, which was perfect. The location is sheltered from strong winds, has electricity access, can be reached by car, and provides the salinity conditions needed for our macroalga, Fucus vesiculosus, to survive.

Sanding PVC plates and cleaning the frames from two years ago. (c) left Linus Holmlund and (c) right Pauline Wasle.

To assess the conditions at the experimental site, we deployed a first set of settlement panels in late April. At first, colonization was slow; only a faint biofilm appeared within two weeks. With the water temperature being still around 7 °C, we decided to give nature more time. Meanwhile, we collected Fucus individuals and practiced the cleaning and the standardizing of the algal thalli for the experiment. Scraping epiphytes off each thallus piece was fiddly, and agreeing on one method was crucial to make sure our results would be comparable to those of other GAME teams.

PVC settlement panel with a faint biofilm, two weeks after deployment. (c) Pauline Wasle.

By early May, building the light setup was a project in itself. Sawing, drilling, testing LEDs, and learning how to secure a 5-meter wooden beam over the water. Our first version bent and twisted until the light pointed sideways instead of straight down onto the algae. Only after buying thicker beams and rebuilding the structure, we finally got a stable and functional setup that could withstand heavy rain and wind. The day we deployed our first experiment at Hamnsundet was cold and rainy but also very rewarding!

Testing a possible experimental setup in the lab ((c) left Pauline Wasle) and the final setup in the field ((c) right Walter Thörnwall).
Finally in the water: Our experimental setup including 4 frames with algal substrates and PVC strips. Two wooden beams were equipped with lighting systems. (c) Tim Wasle.

Outside of work, we made the most of the island life. We explored Åland by bike, kayak, rowboat, and hiking, visited Ramsholmen National Park during the ramson/ wild garlic bloom, and hiked in Geta with its impressive rock formations and went out boating and fishing in the archipelago. At the station on Husö, cooking became a social event: baking sourdough bread, turning rhubarb from the garden into pies, grilling and making all kind of mushroom dishes. These breaks, in the kitchen and in nature, helped us recharge for the long lab sessions to come.

Rock formations in Geta, a famous bouldering spot on Åland. (c) Pauline Wasle.

Every two weeks, it was time to collect and process samples. Snorkeling to the frames, cutting the Fucus and the PVC plates from the lines, and transferring each piece into a freezer bag became our routine. Sampling one experiment took us 4 days and processing all the replicates in the lab easily filled an entire week. The filtering and scraping process was even more time-consuming than we had imagined. It turned out that epiphyte soup is quite thick and clogs filters fastly. This was frustrating at times, since it slowed us down massively.

Over the months, the general community in the water changed drastically. In June, water was still at 10 °C, Fucus carried only a thin layer of diatoms and some very persistent and hard too scrape brown algae (Elachista). In July, everything suddenly exploded: green algae, brown algae, diatoms, cyanobacteria, and tiny zooplankton clogged our filters. With a doubled filtering setup and 6 filtering units, we hoped to compensate for the additional growth.

However, what we had planned as “moderate lab days” turned into marathon sessions. In August, at nearly 20 °C, the Fucus was looking surprisingly clean, but on the PVC a clear winner had emerged. The panels were overrun with the green alga Ulva and looked like the lawn at an abandoned house. Here it was not enough to simply filter the solution, but bigger pieces had to be dried separately. In September, we concluded the last experiment with the help of Sarah from the Cape Verde team, as it was not possible for her to continue on São Vicente, the Cape Verdean island that was most affected by a tropical storm. Our final experiment brought yet another change into community now dominated by brown algae and diatoms. Thankfully our new recruit, sunny autumn weather, and mushroom picking on the side made the last push enjoyable.

Fucus vesiculosus from experiment 3 (top left), Fucus vesiculosus from experiment 4 (top right), PVC from experiment 1 (bottom left) and PVC from experiment 3 (bottom right). (c) Linus Holmlund.

By the end of summer, we had accomplished four full experiments. The days were sometimes exhausting but also incredibly rewarding. We learned not only about the ecological effects of artificial light at night, but also about the very practical side of marine research; planning, troubleshooting, and the patience it takes when filtering a few samples can occupy half a day.

Mushrooms for dinner found right at our experimental site in Hamnsundet. (c) Pauline Wasle.

Hälsningar från Åland och Husö biological station

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Ocean Acidification

What is Coral Bleaching and Why is it Bad News for Coral Reefs?

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Coral reefs are beautiful, vibrant ecosystems and a cornerstone of a healthy ocean. Often called the “rainforests of the sea,” they support an extraordinary diversity of marine life from fish and crustaceans to mollusks, sea turtles and more. Although reefs cover less than 1% of the ocean floor, they provide critical habitat for roughly 25% of all ocean species.

Coral reefs are also essential to human wellbeing. These structures reduce the force of waves before they reach shore, providing communities with vital protection from extreme weather such as hurricanes and cyclones. It is estimated that reefs safeguard hundreds of millions of people in more than 100 countries. 

What is coral bleaching?

A key component of coral reefs are coral polyps—tiny soft bodied animals related to jellyfish and anemones. What we think of as coral reefs are actually colonies of hundreds to thousands of individual polyps. In hard corals, these tiny animals produce a rigid skeleton made of calcium carbonate (CaCO3). The calcium carbonate provides a hard outer structure that protects the soft parts of the coral. These hard corals are the primary building blocks of coral reefs, unlike their soft coral relatives that don’t secrete any calcium carbonate.

Coral reefs get their bright colors from tiny algae called zooxanthellae. The coral polyps themselves are transparent, and they depend on zooxanthellae for food. In return, the coral polyp provides the zooxanethellae with shelter and protection, a symbiotic relationship that keeps the greater reefs healthy and thriving.

When corals experience stress, like pollution and ocean warming, they can expel their zooxanthellae. Without the zooxanthellae, corals lose their color and turn white, a process known as coral bleaching. If bleaching continues for too long, the coral reef can starve and die.


Ocean warming and coral bleaching

Human-driven stressors, especially ocean warming, threaten the long-term survival of coral reefs. An alarming 77% of the world’s reef areas are already affected by bleaching-level heat stress.

The Great Barrier Reef is a stark example of the catastrophic impacts of coral bleaching. The Great Barrier Reef is made up of 3,000 reefs and is home to thousands of species of marine life. In 2025, the Great Barrier Reef experienced its sixth mass bleaching since 2016. It should also be noted that coral bleaching events are a new thing because of ocean warming, with the first documented in 1998.

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The planet is changing rapidly, and the stakes have never been higher. The ocean has absorbed roughly 90% of the excess heat caused by anthropogenic greenhouse gas emissions, and the consequences, including coral die-offs, are already visible. With just 2℃ of planetary warming, global coral reef losses are estimated to be up to 99% — and without significant change, the world is on track for 2.8°C of warming by century’s end.

To stop coral bleaching, we need to address the climate crisis head on. A recent study from Scripps Institution of Oceanography was the first of its kind to include damage to ocean ecosystems into the economic cost of climate change – resulting in nearly a doubling in the social cost of carbon. This is the first time the ocean was considered in terms of economic harm caused by greenhouse gas emissions, despite the widespread degradation to ocean ecosystems like coral reefs and the millions of people impacted globally.

This is why Ocean Conservancy advocates for phasing out harmful offshore oil and gas and transitioning to clean ocean energy. In this endeavor, Ocean Conservancy also leads international efforts to eliminate emissions from the global shipping industry—responsible for roughly 1 billion tons of carbon dioxide every year.

But we cannot do this work without your help. We need leaders at every level to recognize that the ocean must be part of the solution to the climate crisis. Reach out to your elected officials and demand ocean-climate action now.

The post What is Coral Bleaching and Why is it Bad News for Coral Reefs? appeared first on Ocean Conservancy.

What is Coral Bleaching and Why is it Bad News for Coral Reefs?

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