Hydrocarbon-Based Communities in the Ultra-Deep Gulf of Mexico: Protecting the Asphalt Ecosystem

The term ‘asphalt volcanism’ was coined to describe marine sites where extrusions of highly degraded oil form large expanses of hard substratum, which is then colonized by chemosynthetic fauna and sessile invertebrates. A site named ‘Chapopote’, a knoll at 3200m in the southern Gulf of Mexico, was described as the type specimen of asphalt volcanism in 2003. A joint German-Mexican-U.S. expedition on the German ship F/S METEOR returned to the region in February and March, 2015 to quantify the extent and characteristics of Chapopote and other asphalt-hosting knolls using the SEAL AUV, QUEST ROV, shipborne acoustics, and autonomous instrument landers. Preliminary findings have greatly expanded the number of confirmed asphalt volcanoes, as well as sites where seepage was detected as gas flares in the water column. The morphology of asphalt flows, which was investigated using large-scale photo-mosaicking techniques, indicated that they form with a complex interplay of gravity flows, buoyant uplift, and chemical weathering. An unexpected finding was the occurrence of gas hydrate mounds, some exceeding 1000 m² in area and 10 m in relief. Gas hydrate forms almost instantly at ambient depths and temperatures and there was evidence that large plugs of hydrate that can rapidly breach the seafloor. Older mounds are colonized by massive tubeworm aggregations that may serve to stabilize the hydrate. Mexico recently announced the first energy production lease sales in their ‘ultra-deep’ offshore. In contrast to the U.S. Gulf, where extensive safeguards for chemosynthetic communities have been in place for over 25 years, few existing protocols protect the Mexican deep-sea asphalt ecosystem. The combination of extensive asphalt pavements and exposed gas hydrate also pose unusual hazards for exploration piston coring or drilling operations. The time is ripe to consider what conservation model would best serve the region.