The Magellan Seamounts (also known as Magellan Seamount Group[1] and previously called Magellan Rise[2][3] ) stretch from the Mariana Trench to Ita Mai Tai Guyot.[4] Geological studies have demonstrated unique features with implications on understanding of ocean island basalt volcanism.[5] Contracts exist with the International Seabed Authority to exploit the areas potential mineral wealth.[6]
^Cite error: The named reference MGMS was invoked but never defined (see the help page).
^Zakharov, Yu D.; Pletnev, S. P.; Mel’nikov, M. E.; Smyshlyaeva, O. P.; Khudik, V. D.; Evseev, G. A.; Punina, T. A.; Safronov, P. P.; Popov, A. M. (1 February 2007). "The first finds of cretaceous belemnites from the Magellan Rise, Pacific Ocean". Russian Journal of Pacific Geology. 1 (1): 30. Bibcode:2007RuJPG...1...29Z. doi:10.1134/S1819714007010058. ISSN1819-7140. S2CID129404630.
^Mel'nikov, M. E.; Pletnev, S. P.; Basov, I. A. (2006). "New Geological and Paleontological Data on Fedorov Guyot, Magellan Seamounts, Pacific". Tikhookean. Geol. (in Russian). 25 (1): 3–13.
^Wei, Xun; Zhang, Yan; Shi, Xue-Fa; Castillo, Paterno R; Xu, Yi-Gang; Yan, Quan-Shu; Liu, Ji-Hua (2022). "Co-Occurrence of HIMU and EM1 Components in a Single Magellan Seamount: Implications for the Formation of West Pacific Seamount Province". Journal of Petrology. 63 (4). doi:10.1093/petrology/egac022.