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Methane gas hydrate forming below a rock overhang at the sea floor on the Blake Ridge diapir. This image, taken from the DSV Alvin during the NOAA-sponsored Deep East cruise in 2001, marked the first discovery of gas hydrate at the sea floor on the Blake Ridge. Methane bubbling out of the sea floor below this overhang quickly freezes. forming this downward hanging hydrate deposit, dubbed the "inverted snowcone." Click image for larger view.
Windows to the Deep
Exploration of the Blake Ridge
July 22 August 3, 2003
On this exploration, scientists used the Alvin submersible and other tools to explore the biology, physics, and chemistry of sea-floor methane seeps at water depths of 2,000 m to 2,800 m off the coast of the southeastern United States. These seeps occur where methane hydrate depositsa solid form of methane and water stable at high pressures and low temperaturesrise to shallow depths beneath the sea floor and break down to produce methane gas. The Alvin dives explored three sea-floor features where scientists found chemosynthetic communities that live on or near the sea-floor emission sites.
Background information for this exploration can be found on the left side of the page. Daily updates and more detailed logs and summaries of exploration activities are posted below and to the right.
Updates & Logs
Click images or links below for detailed mission logs.
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