Michael J. Stephen

Breath Taking


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burst into space and spread over the cosmos. Over time, various parts of the universe have expanded and cooled, with different solar systems springing up as stars exploded into violent supernovas and the leftover nebulae of gases condensed into solid matter.17

      Our own solar system formed about 4.5 billion years ago. The other planets near us are basically rocky masses, but Earth is obviously different. Pictured from outer space, it appears as the aptly named Blue Planet, a cool, serene mixture of deep aqua oceans and swirling white atmosphere. It stands in stark contrast to the harshness of neighboring Mars, the Red Planet, or our own moon, white and barren.

      But Earth came into being devoid of its beautiful oceans, lush green landscapes, and the give-and-take of evolution, life, and death. For the first four billion years of its existence, Earth fluctuated between extremes of heat and cold, its atmosphere a toxic mixture of nitrogen and carbon dioxide. And for the first two billion years of its existence, it had absolutely no oxygen in its atmosphere.

      Oxygen is so important because of its ability to generate energy efficiently. Organisms derive energy from molecules called adenosine triphosphate (ATP), which are formed through cellular respiration. Without oxygen, cells, through a process called anaerobic fermentation, can still produce ATP—but only a measly two units from each molecule of sugar. This is highly inefficient compared to metabolism with oxygen, through which cells can produce thirty-six ATP units from each sugar molecule. Equipped with these extra units of energy, organisms are able to grow bigger, run faster, and jump higher. Without oxygen, the only living mobile organisms would be anaerobes, tiny creatures that are no match for this world’s oxygen consumers.

      Figure 1: The Great Oxygenation Event: the natural history, over time, of atmospheric gases.

      A single question remained for a long time, however: Where had all this oxygen come from? Something substantial must have happened for a whole new gas to transform the planet in such a unique way. The story of how we began to understand where oxygen came from, and how it changed the world, is an extraordinary tale of hard work, keen observation, and luck (a combination that likely describes many, if not most, scientific discoveries). It’s also a story that simply is not well known—but should be.

      During his doctoral studies at Berkeley, Waterbury found his passion in cyanobacteria, microorganisms that were known to colonize fresh water. More commonly known as blue-green algae, these organisms have properties more like those of plants than of bacteria. Foremost among these unusual properties is the ability to photosynthesize—to turn carbon dioxide and water into oxygen and carbohydrates. But in the 1970s, cyanobacteria were mostly known to colonize only small freshwater areas and were thought to have had a limited role in the Earth’s process of oxygen production. They were not talked about outside of a small academic circle, and no mention of them appeared in major oceanography textbooks.

      After his doctoral studies, Waterbury settled into his job as a research scientist at the Oceanographic Institution. A primary mission in the field at the time was to study ocean bacteria, of which not much was known. Field trips were a regular part of the investigation, and in August 1977 Waterbury headed out on the research vessel Atlantis II to the Arabian Sea, the mass of ocean between India and Saudi Arabia known for having very high levels of inorganic nutrients and a rich marine life. His team’s mission was to analyze samples from the ocean using a new technology: epifluorescence microscopy. The goal was to establish typical levels of known bacteria in the ocean with this new technique.

      The basics of epifluorescence microscopy are straightforward. Tags, made up of the building blocks of DNA, are added to a sample of water, where they attach themselves to corresponding parts of the DNA of bacteria, like puzzle pieces fitting together. Under the blue light of the microscope, these bacteria then fluoresce green from their newly attached tags. If no matching bacteria are present, the tags won’t be activated, and the view in the microscope will remain blank.

      Before adding his DNA tags to the Arabian Sea water, Waterbury did one thing that all students are taught in science class, a mandatory step for every experiment at every level of science, from middle school classrooms to Nobel Prize–winning labs: he set up a rigorous control to ensure his results would be valid. Scientists know that controls are the backbone of all discovery. To find something abnormal, one needs to be able to see, and prove, the existence of what one thinks is normal. So, prior to adding the DNA tags, Waterbury analyzed an unaltered specimen of water from the Arabian Sea under the new epifluorescence microscope so that he would have a baseline for comparison.

      Waterbury assumed he would see nothing unusual in the Arabian Sea water, but instead he was stunned. The blue light of the epifluorescence microscope went through the water, and a bright-orange fluorescence came shooting back out of the eyepiece. Because of his background in cyanobacteria, Waterbury recognized the orange light as the natural fluorescence of phycoerythrin, a photosynthetic pigment that works with chlorophyll to drive the all-important carbon-dioxide-to-oxygen-and-carbon reaction, making life on this planet possible. Cyanobacteria had never been reported to exist in deep-sea salt water, so this was a monumental new finding.

      The initial discovery of cyanobacteria in the Arabian Sea was an introduction, but in order to be able to study saltwater cyanobacteria in depth, Waterbury knew he would have to grow them in culture. He tried for months, each time using a new medium and different nutrition to coax the cyanobacteria to replicate. But each time the same thing happened—within twenty-four hours the cells were all dead. Culturing these bacteria was a must if the study of saltwater cyanobacteria was going to advance. In order to succeed, Waterbury had to go back to basic environmental biology.

      Ocean organisms and freshwater organisms behave very differently. Normally we think of ocean creatures as hardy and adaptable, and the ocean as a rough and wild place. Freshwater bodies, by comparison, seem quiet and tranquil, without sharks and stingrays and deadly jelly­fish. This is the human perspective. From the perspective of bacteria, the reverse is true.

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