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Monday, December 19th, 2016

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    12:00a
    New study sets oxygen-breathing limit for ocean’s hardiest organisms

    Around the world, wide swaths of open ocean are nearly depleted of oxygen. Not quite dead zones, they are “oxygen minimum zones,” where a confluence of natural processes has led to extremely low concentrations of oxygen.

    Only the hardiest of organisms can survive in such severe conditions, and now MIT oceanographers have found that these tough little life-forms — mostly bacteria — have a surprisingly low limit to the amount of oxygen they need to breathe.

    In a paper published by the journal Limnology and Oceanography, the team reports that ocean bacteria can survive on oxygen concentrations as low as approximately 1 nanomolar per liter. To put this in perspective, that’s about 1/10,000th the minimum amount of oxygen that most small fish can tolerate and about 1/1,000th the level that scientists previously suspected for marine bacteria.

    The researchers have found that below this critical limit, microbes either die off or switch to less common, anaerobic forms of respiration, taking up nitrogen instead of oxygen to breathe.

    With climate change, the oceans are projected to undergo a widespread loss of oxygen, potentially increasing the spread of oxygen minimum zones around the world. The MIT team says that knowing the minimum oxygen requirements for ocean bacteria can help scientists better predict how future deoxygenation will change the ocean’s balance of nutrients and the marine ecosystems that depend on them.

    “There’s a question, as circulation and oxygen change in the ocean: Are these oxygen minimum zones going to shoal and become more shallow, and decrease the habitat for those fish near the surface?” says Emily Zakem, the paper’s lead author and a graduate student in MIT’s Department of Earth, Atmospheric and Planetary Sciences (EAPS). “Knowing this biological control on the process is really necessary to making those sorts of predictions.”

    Zakem’s co-author is EAPS Associate Professor Mick Follows.

    How low does oxygen go?

    Oxygen minimum zones, sometimes referred to as “shadow zones,” are typically found at depths of 200 to 1,000 meters. Interestingly, these oxygen-depleted regions are often located just below a layer of high oxygen fluxes and primary productivity, where fish swimming near the surface are in contact with the oxygen-rich atmosphere. Such areas generate a huge amount of organic matter that sinks to deeper layers of the ocean, where bacteria use oxygen — far less abundant than at the surface — to consume the detritus. Without a source to replenish the oxygen supply at such depths, these zones quickly become depleted.

    Other groups have recently measured oxygen concentrations in depleted zones using a highly sensitive instrument and observed, to their surprise, levels as low as a few nanomolar per liter — about 1/1,000th of what many others had previously measured — across hundreds of meters of deep ocean.

    Zakem and Follows sought to identify an explanation for such low oxygen concentrations, and looked to bacteria for the answer.

    “We’re trying to understand what controls big fluxes in the Earth system, like concentrations of carbon dioxide and oxygen, which set the parameters of life,” Zakem says. “Bacteria are among the organisms on Earth that are integral to setting large-scale nutrient distributions. So we came into this wanting to develop how we think of bacteria at the climate scale.”

    Setting a limit

    The researchers developed a simple model to simulate how a bacterial cell grows. They focused on particularly resourceful strains that can switch between aerobic, oxygen-breathing respiration, and anaerobic, nonoxygen-based respiration. Zakem and Follows assumed that when oxygen is present, such microbes should use oxygen to breathe, as they would expend less energy to do so. When oxygen concentrations dip below a certain level, bacteria should switch over to other forms of respiration, such as using nitrogen instead of oxygen to fuel their metabolic processes.

    The team used the model to identify the critical limit at which this switch occurs. If that critical oxygen concentration is the same as the lowest concentrations recently observed in the ocean, it would suggest that bacteria regulate the ocean’s lowest oxygen zones.

    To identify bacteria’s critical oxygen limit, the team included in its model several key parameters that regulate a bacterial population: the size of an individual bacterial cell; the temperature of the surrounding environment; and the turnover rate of the population, or the rate at which cells grow and die. They modeled a single bacterial cell’s oxygen intake with changing parameter values and found that, regardless of the varying conditions, bacteria’s critical limit for oxygen intake centered around vanishingly small values.

    “What’s interesting is, we found that across all this parameter space, the critical limit was always centered at about 1 to 10 nanomolar per liter,” Zakem says. “This is the minimum concentration for most of the realistic space you would see in the ocean. This is useful because we now think we have a good handle on how low oxygen gets in the ocean, and [we propose] that bacteria control that process.”

    Ocean fertility

    Looking forward, Zakem says the team’s simple bacterial model can be folded into global models of atmospheric and ocean circulation. This added nuance, she says, can help scientists better predict how changes to the world’s climate, such as widespread warming and ocean deoxygenation, may affect bacteria.

    While they are the smallest organisms, bacteria can potentially have global effects, Zakem says. For instance, as more bacteria switch over to anaerobic forms of respiration in deoxygenated zones, they may consume more nitrogen and give off as a byproduct nitrogen dioxide, which can be released back into the atmosphere as a potent greenhouse gas.

    “We can think of this switch in bacteria as setting the ocean’s fertility,” Zakem says. “When nitrogen is lost from the ocean, you’re losing accessible nutrients back into the atmosphere. To know how much denitrification and nitrogen dioxide flux will change in the future, we absolutely need to know what controls that switch from using oxygen to using nitrogen. In that regard, this work is very fundamental.”

    This research was supported, in part, by the Gordon and Betty Moore Foundation, the Simons Foundation, NASA, and the National Science Foundation.

    5:45p
    Chikang Li brings the Crab Nebula to the lab

    Senior research scientist Chikang Li wants to experiment with the stars. Intrigued by a curious “kink” phenomenon observed in the Crab Nebula, an interstellar cloud of gas and dust that formed in the wake of a supernova explosion, he has been looking for answers. Images from the Chandra X-ray observatory show that a jet of plasma pouring straight out from the neutron star at the center of the nebula appears to change direction every few years, without changing its structure. Why? Scientists have hypothesized that magnetic fields with the right properties could explain this behavior, but Li wanted proof.

    “How do you design an experiment on Earth to explain mysteries that are happening 6,500 light years away, and stretching over 13 light years of space?” he asks. “Traditional astrophysics is based on observation. Typically after you make an observation, you build a theoretical model, you do some numerical simulations. But that’s it. How can you go there and measure anything? How can you do an experiment to test this model?”

    Li has been part of MIT’s Plasma Science and Fusion Center (PSFC) since becoming a graduate student in 1987. As a co-founder and associate head of the PSFC’s High-Energy-Density Physics (HEDP) Division, Li has collaborated regularly with the National Ignition Facility and the University of Rochester’s Laboratory for Laser Energetics on inertial confinement fusion and laboratory-astrophysical experiments. He decided to see if he could also use the lab's OMEGA laser to mimic the conditions in the Crab Nebula, and prove the hypothesis that magnetic fields were responsible for the “kink in the crab”.

    Instead of training OMEGA’s multiple laser beams on a single pellet of hydrogen fuel, as he would for a fusion experiment, Li bounced lasers off two 3 x 3 mm foils hinged together at a 60-degree angle. Using two laser beams to heat each side, he generated plasma bubbles, or plumes. Li knew that because they are very dense and hot, these plumes would immediately expand, colliding in the middle plane between the two foils to form a jet.

    Li notes that even though laboratory-generated jets and astrophysical jets have very different size scales, the fundamental physics can be the same because critical dimensionless parameters are similar. As a result, they share enough physical properties to allow Li to scale his laboratory experiments, as one would do from a wind tunnel to an airplane, to conditions in the crab nebula.

    While the kink in the nebula jet occurs over a period of a few years, the laboratory experiment creates a jet in one nanosecond (billionth of a second), which then propagates for five to six nanoseconds.  Li laughs as he considers the speed of the experiments: “You have to generate that, diagnose that, characterize that, quantify that in this period of time!”

    To measure the magnetic fields generated by the experiment, Li used a monoenergetic proton radiography (MPR) diagnostic invented by his division in 2005, allowing him, through the deflection of the protons, to make a radiograph of the fields. With the quantitative measurements in hand, he has been able to prove that the nebula jet behavior is governed by weak magnetic fields along the jet, which keep its structure largely straight, and other magnetic fields circling around the jet, which create the instability responsible for the directional change. The results were recently published in Nature Communications.

    HEDP division head Richard Petrasso noted the importance of Li’s work: “Through his understanding of instabilities and his development of the MPR diagnostic to map transient magnetic fields in the laboratory, Chikang has been able to explore and explicate, for the first time, such puzzling phenomena as the jetting in the Crab Nebula.” 

    Li, and graduate students working under his supervision, are now in the process of extending this methodology to a range of other astrophysical phenomena, such as the turbulent generation and amplification of magnetic fields, and the observation of collisionless shocks and their associated magnetic fields.

    With the ability to create measurable astrophysical conditions on earth using the National Ignition Facility and OMEGA lasers, the sky’s the limit.

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