Opportunity for ANZIC Members to apply to participate in JOIDES Resolution Expedition 399:  

Building Blocks of Life, Atlantis Massif

7 April to 7 June 2023

The Atlantis Massif (AM) Oceanic Core Complex (30°N, Mid-Atlantic Ridge) is one of the earliest sites recognized for the extensive exposure of ultramafic and mafic rocks at the seafloor caused by an oceanic detachment fault, and has been the focus of four IODP Expeditions (304, 305, 340T, and 357). The Lost City Hydrothermal Field (LCHF) is hosted in peridotite on its southern wall and vents alkaline fluids rich in H2 as a by-product of serpentinization. The AM is therefore an ideal natural laboratory for studying tectonics, magmatism, and the interaction between the ocean and lithosphere, as well as their combined influence on ocean chemistry and the subseafloor biosphere.

Expedition 399 has three main scientific objectives:

1. Characterizing the life-cycle of an oceanic core complex including links among igneous, metamorphic, structural, and fluid flow processes.

2. Accessing the chemical kitchen preceding the appearance of life on Earth, including the formation of organic molecules of prebiotic interest at high and low temperatures.

3. Identifying the extent of the deep biosphere and limits for life, including how they are influenced by lithological substrate, porosity and permeability, temperature, fluid chemistry, and reactive gradients

A principle aim of the expedition is to sample fluids and rocks in a stable regime where active serpentinization may be occurring, creating the conditions where the building blocks for life (H2, CH4, and more complex organic compounds form abiotically. IODP Hole U1309D, located 5 km north of the LCHF, is the deepest (1415 m) hole drilled so far in young (<2 Ma) ocean crust, and recovered a primitive series of gabbroic rocks interpreted in part to be metasomatised peridotite. Expedition 399 will sample fluids in the existing Hole U1309D using newly developed temperature-sensitive sampling tools. It will also deepen Hole U1309D to ~2060 mbsf, where temperatures up to 220°C are predicted, and leave it available for future logging and fluid sampling once thermal equilibrium has returned. The proportion of ultramafic rocks is expected to increase with depth, and at these temperatures serpentinization and hydrogen generation by redox reactions should be actively occurring. Volatiles and organic molecules will be sampled in fluid inclusions to identify the physicochemical conditions that lead to their formation.

A second shallow (~200 mbsf) hole will be cored close to the LCHF to obtain a complete section through a detachment fault zone in serpentinized peridotite, extending the findings of Expedition 357. It targets zones of higher porosity that may facilitate geochemical and microbial processes. A re-entry system will be installed to allow for future deeper drilling, logging, fluid sampling, and a borehole observatory. The thermal structure of this Hole will place important constraints on the Lost City circulation system, and there is a possibility of intersecting Lost City fluids pathways

For more information on the expedition science objectives and the JOIDES Resolution expedition schedule, see This site includes links to individual expedition web pages with the original IODP proposals and expedition planning information.

Application deadline: 1 February 2022

WHO SHOULD APPLY: We encourage applications from all qualified scientists. The JOIDES Resolution Science Operator (JRSO) is committed to a policy of broad participation and inclusion, and to providing a safe, productive, and welcoming environment for all program participants. Opportunities exist for researchers (including graduate students) in all shipboard specialties, including petrologists, structural geologists, geochemists interested in igneous processes, fluid-rock interaction, gases and organic geochemistry, microbiologists, physical properties specialists, paleomagnetists, and borehole geophysicists. Good working knowledge of the English language is required.


Australian ANZIC member applicants :

  1.  All applicants must have their sign off by their institution DVC-Research or other appropriate institutional level, that their institution approves their travel and will insure them for that travel to and from the port of departure and arrival.
  2. It is agreed that Institutions will cover any additional cost related to delays to a return or additional quarantine costs.
  3. ANZIC will cover:
  • flights and ground transport/incidentals to/from the ship, any pre-departure mandatory quarantine period (up to ~A$3000 for Australian members (accommodation and hotel meals); the cost of a pre-flight COVID test (if required, and as outlined in the IODP COVID policy)
  • will continue to support the selected expeditioner with coverage of required pre-cruise medicals (Aust only; NZ to detail)
  •  up to $40K (over 2 years, Australian members) is available to conduct the expected research related to the international expedition.
  • Visa expenses will be covered by ANZIC  but organised by the expeditioner in consultation with the JRSO if an ANZIC candidate is selected to sail.

Without this sign off an applicant will not be assessed by ANZIC for the expeditioner role advertised and, therefore, will not be forwarded to the JRSO for consideration as an expeditioner

New Zealand ANZIC Member Applicants: Please contact Stuart Henrys ( prior to submitting your application to inquire about the prerequisites that will apply.