Day 2: Muddy Water

Day 2 Many sediment cores and fish are on the way

Ahoy, salty explorers! Teacher Patty and I are reporting from the night shift. We worked with the geochemist (Dave Hollander, Patrick Schwing and David Hastings) to collect ~16 sediment cores. It did not take long before we were snapping coring bottles in place on the Lunar Lander (Multi-core sampler).


After sediment samples were retrieved from the ocean floor the cores were transferred from the Lander to new core liners for future processing. This was definitely a wet and muddy job! The sediment at 100 and 200 meters was well mixed and silty with a light brown color. One core from each location is split in two sections, photographed and visually described in more detail.

Here in the field we are collecting samples 24/7 and once we return to shore the lab work will begin to describe the sediment samples. The scientific information that will be collected from shore includes age dating (short-lived isotopes, like Lead 210, Radium 234), benthic ecology (microfossils- forams), microbial ecology of bacteria/viruses, hydrocarbon chemistry and basic sedimentology and redox biochemistry .

Some of the nighttime sightings included several dolphin chasing flying fish. Sometimes the flying fish would land on the deck of the vessel and we would help return them to the water.


All in all an excellent first day at sea with the C-IMAGE scientist, students and Weatherbird II crew.

Before sailing safety is first concern aboard the Weatherbird II

Bon Voyage! The adventure begins…Day 1

Ahoy, fellow explorers. After a ~500 mile drive to Panama City, loading the vessel and setting sail just before we are now sailing 50 miles from shore to first sampling station. Whew, a full day of anticipation as Patty saw the Weatherbird II for the first time, met the 6 member WB II crew, and 13 members of the science party. First things first… SAFETY DRILL.

Before sailing safety is first concern aboard the Weatherbird II


Patty’s first impressions… “this is not the Royal Caribbean!” and, “where is the  chocolate fountain?” Seriously, it was really cool to see up close and personal the oceanic equipment that I teach my students about and soon I will see how it all works as we begin our first sampling at 11:30PM.


Now that everything is loaded we have set sail. Meet some of the VIP’s aboard the expedition.

During this Adventure at Sea, your ‘cruise director’, Teresa Greely did not bring Rocky the USF Bull aboard but has the honor of sailing with the USF College of Marine Science’s Dean, Jacqueline Dixon and our C-IMAGE Teacher at Sea, Patty Smukall.


Jacqueline Dixon, Dean USF College of Marine Science

(Marine Geologist- Volcanologist)


C-IMAGE Teacher at Sea, Patty Smukall from Wekiva High School


Keep sailing with us as we all prepare to work around the clock, 24/7 to gather as much scientific information as possible during our seven day Expedition in the Northern Gulf of Mexico.

Coming soon, meet the scientist, students and crew aboard the WBII and discover how the samples of sediment and fishes are collected.





A New Adventure: USF C-IMAGE Scientists Host Teacher at Sea Program

Ahoy, ocean adventurers! Join us as we set sail on a new Adventure at Sea to the northern Gulf of Mexico with Patty Murphy Smukall, our first Teacher @ Sea. The expedition will be from August 14-21. We will board the research vessel Weatherbird II in Panama City then sail to Desoto Canyon to begin the research. Follow us as we join USF scientists to help answer questions about the current ecology of the Gulf.


The mission of the C-IMAGE cruises is to help to answer several fundamental questions about the Deep Water Horizon (DWH) event and subsequent impacts on the plankton population, reef and fish communities and the microbial communities. Deep sea sediment samples, plankton and fishes collected during these expeditions will be the data source. Teachers will be part of the scientific crew and participate in the at sea research. Sampling activities include the use of the Sipper plankton sampler, multi-core sediment system and long line surveys to assess fish health.



While at sea teachers will be the ship to shore communicators via social media (Twitter and daily blogs) and LIVE video conferencing with formal and informal classrooms. Marine scientists, post-docs and graduate students participating in the C-IMAGE cruises will collaborate with the teacher on board to communicate the science, technology and life at sea experiences to educational and general audiences.






While on shore teachers will translate their At Sea learning experience to understandable inquiry-based lessons about the science and technology encompassing the northern Gulf of Mexico ecology, the DWH event and subsequent impacts. Lessons developed from the cruises will inform a future series of C-IMAGE Teacher Professional Developments during Phase 2 of Outreach & Communication. Once developed lessons will be available to science educators electronically via the College of Marine Science Education & Outreach . The overarching goal of our outreach activities is to advance ocean sciences literacy and education by understanding and applying the science we learn along the way.


If your classroom, school or other educational facility would like to participate in a LIVE video conference during our expedition, please contact Teresa Greely, for details.

Teresa on deck of JOIDES Resolution during LIVE! Aboard the JR video-conference to USF Honors students. Photo credit Etienne Claasse


Follow USF alumni, PATTY MURPHY SMUKALL, as our first Teacher at Sea!

Patty’s science footsteps. Patty is a science teacher who has taught Marine Biology, Biology, Earth Science and Physical Science. This school year she will be teaching 11-12 grade Marine Science classes. She has been teaching in the classroom for 22 years and 5 years at zoos/aquariums, including Sea World and Mill Mt. Zoo. Patty has always been interested in the ocean and its inhabitants, ever since she watched “Flipper” as a little girl. She followed the dream of working with dolphins by attending USF and majoring in Zoology. The dream became reality when she began her science career working at Sea World with dolphins, manatees, sea lions and other marine mammals. Later, she realized that the best way to have an impact on conservation is to teach the next generation to care. She has spent the last several years teaching Marine Science, currently at Wekiva High School in Apopka, Florida.

Patty’s recent visit to Alaska.

Cruise Plan

The goal of this cruise is to evaluate the extent of fish disease and to characterize the distribution and fate of oiled sediment at sites on the continental shelf and slope of the northern Gulf of Mexico Gulf of Mexico. Sampling activity will include long-line fishing, sediment coring and water column hydrography.

2012 August Coring and Longline Survey in the Gulf of Mexico

Map view of proposed sampling sites and ship routes for Leg 1 (green) and Leg 2 (red).

Gulf of Mexico Teacher @ Sea Program

The C-IMAGE Gulf of Mexico Teacher at Sea Program is offering three expeditions for In-service Science Teachers in Florida. Current dates of the expeditions are:

  • August 12-21 Fish Health Surveys………. Application Deadline 7/25/2012
  • October 19-31Deep Ocean Sediments……..Application Deadline 9/19/2012
  • November 2-8 Zooplankton Survey…………Application Deadline 10/02/2012


The C-IMAGE program strives to integrate facts with other research, integrate facts into knowledge, and disseminate information to the public and decision makers


Gulf of Mexico Research Initiative logo

This research is made possible by a grant from BP/The Gulf of Mexico Research Initiative.

Contract #SA 12-10/GoMRI-007

Image of cirrus clouds appearing to circle around the sun.

Halo Around the Sun

This post is by Michael Martinez, a USF graduate student aboard the JOIDES Resolution.

Image of cirrus clouds appearing to circle around the sun.

This is amazing.  It is the third one I have seen so far in my whole life.  First time was a long time ago on an island far-far away in middle school.   This halo around the sun is made when you have cirrus clouds high in the atmosphere.  They will refract sunlight (or bend the light) forming this halo or “rainbow” around the sun.

Picture of two humpback whales off the sides of the JOIDES Resolution.

Humpback Whales

This post is by Michael Martinez, a USF graduate student aboard the JOIDES Resolution.

Picture of two humpback whales off the sides of the JOIDES Resolution.

This is really AWESOME!!!!!!.  These are humpback whales.  I have never seen them that close.  These two lovely mammals passed by the aft (back), port (left), bow (front), and stern (right) sides of the Joides Resolution.  So you could say they were curious and wanted to take a look at our underwater operations while allowing to be mesmerized by their raw natural magnificence  :-)

Teresa on deck of JR during LIVE! Aboard the JR videoconference to USF Honors students. Photo credit Etienne Claasse

Visit JR Expedition 340 Blog

Readers please visit the expedition blog at for details about weekly science findings, people aboard, and other curiosities during Expedition 340.

Teresa on deck of JR during LIVE! Aboard the JR videoconference to USF Honors students. Photo credit Etienne Claassen

A few days ago I was able to give a lesson to my students, but this time the JR was the classroom. This was made possible thanks to the JOIDES Resolution Live! program that is sponsored by the Deep Earth Academy providing live video broadcasts with the educators and scientists on board the ship during every expedition. This is the first time a USF class has been taught while a professor was at sea. This provides a unique opportunity for students in my natural sciences classes to experience more directly the field based aspects of scientific research as well as ask questions about the science
as it is unfolding during our expedition in the Lesser Antilles. We are broadcasting to two locations in the USF family—campuses in Tampa and St. Petersburg Florida. A special thanks again to Deep Earth Academy for this
nything but typical ‘science’ class.

From stern of JR the island of Montserrat with the volcano Soufriere Hills in sight. Photo credit Etienne Claasse

Why Submarine Sediments near Volcanic Islands?


Island of Montserrat with active volcano Soufriere Hills in view. Photo credit Takeshi Saito.

We are sailing in the Lesser Antilles or West Indies of the Caribbean Sea. Scientists aboard the JR such as volcanologist, sedimentologist, inorganic geochemist, and micropaleontologist are at this location in the ocean because of the volcano on Montserrat, called the Soufriere Hills volcano. This is one of the best studied volcanoes on the planet. The eruptions began in 1995 and continue today. In 2003 the dome (top) of the volcano collapsed. Scientists estimate that over 70% of the erupted material has washed into the adjacent ocean. The surrounding seafloor was quickly covered with volcanic deposits.

From stern of JR the island of Montserrat with the volcano Soufriere Hills in sight. Photo credit Etienne Claassen


Since the 1995 eruptions the volcano has been under continuous surveillance. Both England and France have observatories on the island to measure and document the behavior of the volcano. In particular a detailed series of data before and after eruptive events has been compiled. Scientists have generated lots of data from land-based measures and from submarine cores collected to depths of about 6 meters in the seafloor. This means that Montserrat is one of the best studied volcanoes on the planet!




Assembling drill pipe for drill string. Photo credit Adam Stinton

Now it is time to go deeper into the seafloor to discover the volcanic history of Montserrat over several million years
ago, maybe even longer. A major question for Expedition 340 is to explore what happens when the majority of volcanic material (pyroclastics) extruded from magma, flows into the ocean? Now for the first time with the technology and brawn of the JOIDES Resolution we can obtain cores from deeper in the seafloor, thus on longer time scales than previously known. The 340 expedition is going back in geologic time to gather data about the long-term history of the volcano over the past million years. This task can only be accomplished through scientific ocean drilling. The data from Expedition 340 will help scientists around the world better understand the modern day events occurring in the Lesser Antilles island arc, in particular the potential for future hazards such as eruptions and tsunamis.


 By retrieving ocean based cores we are sampling the geologic archive that lies beneath the seafloor.
Moon pool is a 7 meter opening in the main deck of the JR where the drill string, bottom hole assembly and logging instruments are lowered to the seafloor.

Rocky and Teresa visit moon pool

Our favorite memory for today

Today, lil’ Rocky the Bull (VIP Aboard the JR) and I visited the moon pool. This is one of the coolest places on the Jr. It is located below the drill floor a deck below where my office is located on the Foc’sle Deck (Forecastle or F Deck). A hard hat and safety glasses are required, ear plugs are suggested too. What is the moon pool? The moon pool is a 7 meter opening in the main deck of the ship, giving access to the water below, allowing technicians or researchers to lower tools and instruments into the sea. The drill string is lowered from an opening in the drill floor through the moon pool to the seafloor. Hope you enjoy these photos as much as I enjoyed my visit.

Moon pool is a 7 meter opening in the main deck of the JR where the drill string, bottom hole assembly and logging instruments are lowered to the seafloor. Photo credit, Bill Crawford, IODP photographer

A close-up view of the moonpool. Photo credit, Bill Crawford, IODP photographer

JR Drill Floor, the drill string is the brown structure in center of photo, this is a series of pipes joined together to transcend the depths of seawater then penetrate the seafloor with a drill attached at the base.

JR Drill Floor: Where it all begins

This is where all the action begins– the drill floor. Take some time to enjoy this YouTube video of the
JR Core Journey from Rig Floor to Core Receiving Deck to Core Lab (really nice narrated video)

JR Drill Floor, the drill string is the brown structure in center of photo, this is a series of pipes joined together to transcend the depths of seawater then penetrate the seafloor with a drill attached at the base. Photo credit, Adam Stinton, Expedition 340 Volcanologist

The island of Montserrat, showing the Soufriere Hills volcano.

Work on the JOIDES Resolution

This post is by Michael Martinez, a USF graduate student aboard the JOIDES Resolution.

The island of Montserrat, showing the Soufriere Hills volcano.

This is a photomosaic of the island of Montserrat in the Lesser Antilles.  The big hill in the center background is the Soufriére Hills volcano.  This is an active volcano and has undergone several eruptions since 1995.  We are studying the volcanic sediments deposited below sea level to understand the evolution of this volcanic island.  This picture was taken approximately 60 miles offshore.

JOIDES Resolution core sample, which shows different sediments.This picture shows a section of one of the cores drilled by the JOIDES Resolution drilling crew.  What you see are hemipelagic sediments (light colors) interbedded or “mixed” with volcanic rich sediments (darker color).  You will notice numerous bands of different colors made by marine organisms that live within the sediments (infaunal).  This process is called bioturbation and it occurs after sediments are being deposited.

Benthic Foraminifera fossils, which look like little spheres attached to one another.These fossils are benthic Foraminifera.  They are single celled protists that make a shell of calcite (calcium carbonate).  You will see that each one is made out of several little spheres.  These spheres are known as chambers and each one represents a different growth stage.  The benthic foraminifer shown here is known as Siphonodosaria cooperensis.  This species of benthic foraminifer became extinct approximately 0.58 MA or 580,000 years ago.  We use foraminifers like this to give an age of the sediments in which they lived in.  The scale at the bottom left is 1 mm.

Sedimentology/Micropaleontology LaboratoryThis is a photomosaic of the Sedimentology/Micropaleontology laboratory.  Our lab is the best one in the ship because we got two windows!!!!!!!!!  This laboratory has all the equipment, materials, and chemicals (Hydrochloric acid, Acetic acid, Sulfuric acid, acetone, etc.) needed for micropaleontologists, like me, to process our samples.  On the left side you have two sinks, MilliQ water source, numerous drawers with materials and gadgets (like sieves, mortars, slides, etc.).  This lab is equipped with two fume hoods, oven, centrifuge, hot plates, and humidifiers. When a sample is received from the core deck, the first step is to get in our lab and process the sample. It might take between 10 minutes to 2 hours to fully prepare a sample before looking at it under the microscope!!!!  If sediments are very sandy it takes like 10 minutes.  But, when we get clay rich sediments it takes a long time because typically most clay sediments tend to be very sticky (depending on composition).

Michael's Work StationThis is my working station.  I got a corner desk so I have more space to redistribute my stuff.  Here you can see a PC computer, my laptop, camera, cell phone, and headphones.   Sometimes it gets very tedious to look for foraminifers under the microscope since it takes me like one hour to analyze a sample.  To maximize my efforts and work faster, I brought with me several TV series like The big Bang Theory, The Simpsons, and the X-Files (behind my laptop) to keep me entertained while working.

A translucent, shell-shaped creatureThis benthic foraminifer is the MOST BEAUTIFUL one I have ever seen.  I cannot imagine how these critters develop such morphologies.  This foram is known as Laticarinina pauperta and is commonly found at depths close to or greater than 2000 meters below sea level.  The scale base is 1 mm.

An image comparing the shape of the Sputnik satellite to that of a Oolina sp. benthic foraminifer.This is really cool.  The photo on the left (not to scale) is the Sputnik satellite.  First object to orbit the Earth made by the Russians in the 1950’s.  The photo on the right is an Oolina sp. benthic foraminifer.  I am amazed by the resemblance between pictures!!!!  The scale is 1 mm.