Saturday, September 18, 2010

Capricious Seas and Symphonies

Station 8

42° 24.257’ N, 59° 17.522’ W

13:35 EST

Winds: 6.5 knots

Last night we were rolling and pitching, but yesterday morning was sublime. We hoisted the CTD back on deck at approximately 4 am and the seas began to rest. The ship was holding station and engines were quiet. In the blackness of night over the blackness of the sea, it was hard to tell if we were floating on water or floating in space. I was certain, however, that the sunrise would be a peaceful reward to a long night’s work.

And then it happened. Not suddenly, but subtly. Iridescent cirrus clouds began to shine. They failed to light the night, but rather snaked across like pale Northern Lights. We stood on the aft deck and watched in silence as the show evolved. To paraphrase my friend, Drew, it was a symphony. Strings and woodwinds brushed a heavenly canvas in smooth violet strokes. Occasionally, one instrument would outshine the others then fade into the palette. Slowly, almost imperceptibly, the kindle began to blaze. We moved to the bow and enjoyed the music that started our day.



But the seas keep us guessing. Our ship’s dynamic positioning (DP) system keeps us on station, while our Planet’s systems keeps flowing by. The Atmosphere can change on a much shorter time scale than our present occupation of Station 8. Which leads us to wonder, what movement will the symphony play next?

Thursday, September 16, 2010

Conductivity, Pressure, and Depth

Station 6

42° 53.684’ N, 59° 48.143’ W

21:23 EST

Winds: 21 knots

The CTD is back on Atlantis. What is it, anyway? While the letters “CTD” are shorthand for Conductivity, Temperature, Depth, “the CTD” commonly refers to a collection of instruments and water bottles (Niskin bottles) bundled onto a steel frame (see photo: WHOI's Joe Murray collects water from the CTD for Radium analyses, 14 Sep 2010). Collectively, this is the primary tool that I use to collect water samples anywhere between the surface and the bottom of the sea. I’m often asked if I dive to collect my samples. While I would love to experience the deep sea untethered, the CTD is a much easier way to grab a few liters of water. Here’s one reason why. Liquid water is a very dense fluid (1 gram per milliliter). Think of a gallon of milk. That’s about 8 pounds. Now think of a stack of 10,000 milk jugs resting one on top of the other on top of your head. That’s about how much pressure we would feel at the depths we are sampling. I would rather use the CTD.

Basically, we lower the CTD over the side of the ship while monitoring the instruments on a computer. This gives us a continuous readout of the water temperature, pressure, salinity (conductivity), oxygen concentrations, etc… throughout the water column beneath us. Among other things, this information reveals where life is most abundant, where particles are raining down, and where the water comes from. After the CTD reaches its maximum depth, we hoist it back to the surface, stopping frequently to fill our Niskin bottles with water samples. We can do all of this from the comforts of our ship.

Recovering the CTD takes a good team and clear communication. It is heavy. And it happens to swing from a crane above the perpetually wet deck of a rolling ship. So you gear up with steel-toe boots, a life vest, and a hard hat. You look over the rail at the wire that disappears beneath the waves. The winch operator keeps winding it in. Faintly, it comes into view—a pale blue leviathan rising from the deep. It breaches the surface with a roar and sprays foam through the waves. Our job at that moment is to grab the swinging mass with 20-foot long hooks, safely assist it over the rail and onto the deck, and then bolt it down for safety.

All of this takes time, of course. Our first CTD cast at Station-6 lasted 5 hours from deployment to recovery. It will be weeks before we can begin analyzing these water samples back at WHOI. It will be months before we will see results. In the meantime, we have 4 more CTD casts and 1 sediment core to complete before moving to deeper waters…

Wednesday, September 15, 2010

Light winds

Station 6, 20:10 EST

42° 53.684’ N, 59° 48.143’ W

Winds: 33 knots

The CTD on is on its way back to the surface. Two hours ago it was only 10 meters above the seafloor, 2984 meters down into the cold, calm darkness, gently hanging from a 1/4 inch cable. The journey started 3 hours ago when the seas were calm and the winds were light. But three hours can change everything. The winds have picked up to 33 knots, white caps cover the sea like stars cover the night, and Atlantis is starting to roll. And as I type, the sky opened up. It is pouring. But it could be worse... Time to suit up and get this thing back on deck.

Sunday, September 12, 2010

Safety First

42°14.385’N, 64°59.658’ W

We arrived at our test station tonight. This is where we work out the kinks in our procedures and equipment before continuing on. We have also sampled some sediment cores. It’s kind of like removing a straw full of milkshake from a cup, except that we dropped the straw 1 kilometer down to the bottom of the ocean, the Atlantic ocean is the cup, and the milkshake is marine sediment. Generally, the older sediment is at the bottom of the straw and the most recently deposited sediment is at the top. Therefore, these cores allow us to read a record of Earth’s history when we analyze their chemical composition from top to bottom. This is just one facet of our work on understanding the carbon cycle.

How do we know what to do each day? It’s planned well in advance, but the plan is constantly revised. For example, we ran into some choppy seas overnight that slowed our progress to this station. We also had some troubleshooting that took longer than expected, so one of our tests will be delayed. You get the idea. That’s why each day starts with an email telling us what to expect. Here is what I read this morning:

“Plan of the Day - September 11, 2010

Hi All,

Here's the schedule for today's activities.

10:30 Fire and safety drill - rear of Main Lab.

13:00 Science party meeting - Library

~18:30 Arrive @ test station (1000 m water depth).

Tentative order of activities:

1. In situ pump test cast

2. Multicorer test.

3. Hybrid CTD rosette/pump test cast”

The first event today was a safety drill. We learned about the various alarms, where to muster if there is a problem, and how to get into a “gumby suit” (see photo) among other things. It’s all part of getting our sea legs. But tomorrow we steam to our first official station. Ready or not, the science begins!

Saturday, September 11, 2010

Moving On

40°28.04’ N, 68°50.19’ W

We are now officially cruising into the North Atlantic! The first day is always exciting. Bustling to load and lash our gear in the labs. Last minute purchases from the stockroom. Calling loved ones before losing cell service for one month. But then the horn blows and the ship slowly pulls away from land. You glide through the calm blue waters of the harbor, stand on the aft deck and see your town from a new perspective for the first time. The tiny buildings and green trees fade below the horizon. You now have a vast blue world to explore.

The RV Atlantis is an incredible place to work. The resources are unbelievable (I still can’t believe that I’m blogging from here) and it is full of treasures. Take Alvin for instance. This little sub is perhaps the most famous oceanographic diver, and it is right here with us. The crew is even more impressive. This is their home and they went out of their way to welcome us aboard. Not to mention the food they served us. You may think we subside on canned beans and sour kraut, but our cook prepared some delicious sesame-crusted tuna steaks for dinner. Did I mention this place is incredible?

The sea is calm, the ship is stable, our gear is stowed, and all is well. It’s time to get some rest before the big day tomorrow. We will be gearing up for some tests at approximately 1730 h (Eastern time) before moving on.

Monday, September 6, 2010

Why go to sea?

September 10th. That is the day we leave port and begin living a "National Geographic Moment" for almost 1 month. Wrestling a 500 pound lead weight swinging from the crane as the ship rolls and pitches. Stinging your fingertips with freezing-cold water pulled from 4 kilometers below the surface. Working on the deck with 10 people who were strangers only days ago, but now who are colleagues that you trust with your life. You are part of a team. You focus. You take the A-frame in. Stop. Shackle the instruments to the line. Stop. A-frame out. Watch the Boatswain. His arm is up. His finger is tracing circles in the sky. Stay focused. His fist clenches above his hardhat. STOP. And you do stop. And you continue to focus. But all the while you notice the sun is rising behind him. It hasn't breached the horizon yet, but is illuminating clouds above that didn't exist moments ago. When you started this morning the sky was black and the your entire world stretched from the illuminated deck below your feet to the blackness just beyond. The sound of water splashing against the ship was your only assurance an ocean was out there, but there was nothing else for hundreds of miles. You wonder what your teammates might be seeing so you turn around. The sky is subtly purple, the sea is metallic, and a single storm petrel is cruising between the waves. Focus. You turn around and the sun has already breached the horizon. A red hot coal lighting the sky, warming your face, and casting long shadows that get shorter by the minute. These are the days that keep drawing us back to the sea.

We will be heading into the North Atlantic on September 10th for an opportunity to explore our Earth. We aim to take samples of seawater, its chemical constituents, and sediments from a series of "stations" between Nova Scotia and the Mid-Atlantic Bight. What could we possibly learn there that we haven't already? After all, ships have been traversing these waters for nearly 500 years. And it is just saltwater. Right? All fair questions. It turns out that the vast majority of what we understand about Earth was learned within roughly the last 50 years. And we still have a long way to go. Looking down on our planet from above, it is clear that the vast majority of its surface is ocean blue. A sapphire gem reflecting the light of our sun. Take a look for yourself at what I consider to be one of the most beautiful of human endeavors--a NASA video of our Earth spinning through 1 full day (NASA/Goddard Space Flight Center Scientific Visualization Studio).

We have accumulated a sufficient body of knowledge to create the cameras, communications, and rockets necessary to launch a satellite into space, turn it around, record photons bouncing off Earth's surface, and finally send the images back to us. More importantly, we had the vision to do so. By any measure, humans are a small component of the universe. But we are the only component of the universe (so far as we know) that actively tries to understand itself. This video is proof. It is also proof that the ocean is much larger than you or I. It would take a tremendous amount of time and resources to explore all of it. And even if we did, we cannot forget the most fundamental variable of all: time. What we observe today will not necessarily manifest tomorrow. Furthermore, new observations beget new questions, and new questions beget new perspectives on what needs further study.

These factors--the enormity of the oceans, their variability over time, and novel insights--are what makes oceanography interesting, but also challenging. The working environment doesn't help either. One of the first orders of business on a research cruise is lashing down all of our equipment. Nothing of value or heft should be sitting untethered before leaving port or else it will fall. The ocean will see to it. It is relentless, constantly working the ship, wave after wave, trying to bring it down. The high humidity and vibrations from the engines can change the responsiveness and sensitivity of our instruments. And those are the good days. On bad days when wind are blowing at 30 knots, when your ship is listing 30°, when the water is breaching the rail, you simply do not work for safety's sake. And if anything breaks on the high seas, it will not work again unless you are very clever (either at repairing instruments with improvised tools, or at thinking ahead and packing spare parts). The oceans are unexplored because they challenge us.

So, why go to sea? We know it can be a thrilling adventure. We also know that the ocean is largely unexplored, both physically and intellectually. But I would also argue that we go to sea because of urgency. Science can be an incredibly slow process, and surely we've all contemplated this at one time or another in own lives. "If only science could find cures for diseases before our loved ones succumb to them." Or perhaps you have considered this generality: "If I knew then what I know now, I might have done things differently." We are collectively, often unknowingly, driving the largest experiments that this planet has ever seen. We are redistributing elements and energy throughout the Earth at an industrial pace. We are growing in number exponentially, and our demands for food and other resources are following suit. We know that the Earth must respond in some way to these changes, but we haven't even constrained how it works in our absence. We go to sea and hopefully become more informed and responsible stewards of our home.

We go to sea September 10th.

Friday, September 3, 2010

The Adventures Begin...

Sea spray exploded over the bow as we crashed into the canyon. The ship shuttered--280 feet of vibrating iron beams and rivets--and our stomachs were shackled to it. She rolled to port then began to rise. Heavily. She rolled hard back to starboard before surging through the crest of the 50 foot monster and free-falling into another canyon. Smoke fumed from the stacks, foam washed across the deck, chairs crashed down the hall, the smell of diesel filled the air, and every door was dogged shut. We were in a storm and it wasn't going to stop. Not for 3 more days. We were crossing The Drake Passage.

Despite our technology--GPS navigation systems, satellite communications, powerful diesel engines, and a profound history of engineering achievement--the sea reminded us of what we really were on that day in November, 1998: planetary explorers. We were crossing an ocean ultimately created over billions of years from immense nuclear reactions, exploding stars, massive colliding rocks, volcanic outgassing, and planetary evolution. This was the Southern Ocean, and we were at it's mercy. As scientists, we were there to discover its secrets.

This blog is for students of Earth and planetary science, whether amateur or formally enrolled, who are interested in learning more about science and scientists. What is a "scientist" anyway? We are often categorized based on our areas of expertise: chemist, biologist, physicist, geologist, oceanographer, etc... But that is a little misleading. Perhaps we are best described by what we have in common. Namely, scientists share an innate, insatiable curiosity about the world around us and the desire to find answers to our questions. Sound boring? Consider a few more examples of what some scientists do.
  • trek across the glaciers of Greenland, Antarctica, and the Himalaya to discover changes in our planet's climate that were recorded in the ice itself;
  • live for weeks to months on an icebreaker studying the frozen seas, their currents, chemical compositions, and the organisms that somehow survive there;
  • dive in submarines to explore undersea volcanoes, vast fields of methane hydrates, and the incredible life surrounding hydrothermal vents;
  • fly into the heaving winds of hurricanes to understand how they work and, among other things, improve our ability to predict them (this is a particularly germane example of scientific adventure given Hurricane Earl's expected arrival in Cape Cod tonight);
  • orbit the Earth at 17,000 mph to perform experiments in an environment that is more common in the universe than Earth's surface, but much more difficult to simulate;
  • Walk on the Moon! (Dr. Harrison Schmidt, geologist, Apollo 17, December 1972)
These particular adventures, their associated thrills, and inherent risks, were born of the desire to explore frontiers of knowledge, clarify what is unknown, and ultimately discover and understand something that no one else ever has. Science is the work of a detective; it is not a collection of facts.

My intention is to provide insights into the life of a chemical oceanographer working aboard a research vessel on an upcoming cruise. I may not be able to provide regular updates because the work is demanding and satellite connections are not infallible. However, I do hope to provide sufficient detail to satisfy your curiosity.

We will depart Woods Hole aboard the Research Vessel Atlantis on September 10th and return to port on October 5th. We are heading into the North Atlantic to study carbon dynamics along the North American margin. More on that later...

In the meantime, I'm sitting in my room in Falmouth, MA, tuning-in to NOAA's weather report on my two-way radio, watching the wundermap radar for Cape Cod, and listening to our Planet outside. Hurricane Earl has arrived.

The adventure begins...