Abstract
In this study different experimental designs for monitoring of sediment plumes produced by deep-sea mining are presented. Plumes of sediment stirred up from the seabed by mining machines are considered to represent a major environmental pressure which may extend far beyond the actual mining area. Two industry field tests with the scaled mining vehicle Apollo II of Royal IHC conducted in a relatively shallow setting offshore southern Spain provided valuable insights for anticipated monitoring of nodule mining activities in the deep Pacific. Although the tests were performed in only 300 m water depth, much less than the depth where future deep-sea mining will take place, the weakly stratified bottom water, tide-dominated near-bed currents with mean magnitude of around 5–10 cm s−1, and gently sloping seabed covered with fine muddy sediment provide a good analogue to operational conditions in the deep sea. The plume of suspended sediment mobilised by the mining vehicle was monitored with turbidity sensors deployed on a ship-operated CTD system and on a static array of moored sensors and monitored visually using a ship-operated ROV. It was found that the generated sediment plume extended no >2 m above the seabed close to the source (<100 m) but increased in height at greater distance. Furthermore, turbidity values decreased rapidly with increasing distance to the source. Even though plume monitoring suffered interference from bottom trawling activities in neighbouring areas, a distinct turbidity signal generated by the mining equipment could still be distinguished above background turbidity at 350 m away from the source. From the experience gained in shallow water, recommendations are made on how a combination of sensors operated from moving and moored platforms may be a suitable and successful strategy for monitoring man-made sediment plumes in the deep sea.
| Original language | English |
|---|---|
| Article number | 106971 |
| Pages (from-to) | 1-20 |
| Journal | Marine Geology |
| Volume | 456 |
| DOIs | |
| Publication status | Published - Feb 2023 |
Bibliographical note
Funding Information:We thank the captains and crew of RV Sarmiento de Gamboa for their essential assistance during the two field tests. Technical assistance onboard the ship was provided by Arturo Castellón and his team of the Marine Technology Unit of the Spanish Research Council UTM-CSIC. The ROV team of the Flanders Marine Institute (VLIZ) assisted in the field tests by seabed surveys and plume observations with ROV Zonnebloem and supporting underwater navigation with the GAPS system. The engineering team of IHC Mining, responsible for driving Apollo II, played a key role in carrying out the field tests. We thank our colleagues from the NIOZ-EDS department for borrowing their LISST-200X and in particular Dr. Karline Soetaert for her assistance with the processing of the data. This research was funded by the Blue Nodules project (EC grant agreement no. 6887851). HdS, CM and LdJ acknowledge additional funding from the Blue Harvesting project (EIT RM grant no. 18138). We thank three anonymous reviewers for insightful comments and constructive criticism which improved the manuscript.
Funding Information:
We thank the captains and crew of RV Sarmiento de Gamboa for their essential assistance during the two field tests. Technical assistance onboard the ship was provided by Arturo Castellón and his team of the Marine Technology Unit of the Spanish Research Council UTM-CSIC. The ROV team of the Flanders Marine Institute (VLIZ) assisted in the field tests by seabed surveys and plume observations with ROV Zonnebloem and supporting underwater navigation with the GAPS system. The engineering team of IHC Mining, responsible for driving Apollo II, played a key role in carrying out the field tests. We thank our colleagues from the NIOZ-EDS department for borrowing their LISST-200X and in particular Dr. Karline Soetaert for her assistance with the processing of the data. This research was funded by the Blue Nodules project (EC grant agreement no. 6887851 ). HdS, CM and LdJ acknowledge additional funding from the Blue Harvesting project (EIT RM grant no. 18138 ). We thank three anonymous reviewers for insightful comments and constructive criticism which improved the manuscript.
Publisher Copyright:
© 2022 The Authors
Funding
We thank the captains and crew of RV Sarmiento de Gamboa for their essential assistance during the two field tests. Technical assistance onboard the ship was provided by Arturo Castellón and his team of the Marine Technology Unit of the Spanish Research Council UTM-CSIC. The ROV team of the Flanders Marine Institute (VLIZ) assisted in the field tests by seabed surveys and plume observations with ROV Zonnebloem and supporting underwater navigation with the GAPS system. The engineering team of IHC Mining, responsible for driving Apollo II, played a key role in carrying out the field tests. We thank our colleagues from the NIOZ-EDS department for borrowing their LISST-200X and in particular Dr. Karline Soetaert for her assistance with the processing of the data. This research was funded by the Blue Nodules project (EC grant agreement no. 6887851). HdS, CM and LdJ acknowledge additional funding from the Blue Harvesting project (EIT RM grant no. 18138). We thank three anonymous reviewers for insightful comments and constructive criticism which improved the manuscript. We thank the captains and crew of RV Sarmiento de Gamboa for their essential assistance during the two field tests. Technical assistance onboard the ship was provided by Arturo Castellón and his team of the Marine Technology Unit of the Spanish Research Council UTM-CSIC. The ROV team of the Flanders Marine Institute (VLIZ) assisted in the field tests by seabed surveys and plume observations with ROV Zonnebloem and supporting underwater navigation with the GAPS system. The engineering team of IHC Mining, responsible for driving Apollo II, played a key role in carrying out the field tests. We thank our colleagues from the NIOZ-EDS department for borrowing their LISST-200X and in particular Dr. Karline Soetaert for her assistance with the processing of the data. This research was funded by the Blue Nodules project (EC grant agreement no. 6887851 ). HdS, CM and LdJ acknowledge additional funding from the Blue Harvesting project (EIT RM grant no. 18138 ). We thank three anonymous reviewers for insightful comments and constructive criticism which improved the manuscript.
Keywords
- Deep-sea mining
- Plume monitoring
- Polymetallic nodules
- Sediment plume
- Sensor array