Article Geochemistry 3 Volume 7, Number 5 Geophysics 2 May 2006 GeosystemsG Q05001, doi:10.1029/2005GC001086 G ISSN: 1525-2027 AN ELECTRONIC JOURNAL OF THE EARTH SCIENCES Published by AGU and the Geochemical Society Submarine radial vents on Mauna Loa Volcano, Hawai`i V. Dorsey Wanless and M. O. Garcia Department of Geology and Geophysics, University of Hawai`i, Honolulu, Hawaii 96822, USA (
[email protected]) F. A. Trusdell Hawaiian Volcano Observatory, U.S. Geological Survey, Hawai`i National Park, Hawaii 96718, USA J. M. Rhodes Department of Geosciences, University of Massachusetts, Amherst, Massachusetts 01003, USA M. D. Norman Research School of Earth Sciences, Australian National University, Canberra, ACT 0200, Australia Dominique Weis Department of Earth and Ocean Sciences, University of British Columbia, Vancouver, BC, Canada V6T 1Z4 D. J. Fornari and M. D. Kurz Woods Hole Oceanographic Institution, Woods Hole, Massachusetts 02543, USA Herve´ Guillou Laboratorie des Sciences du Climat et de l’Environnement Domaine du CNRS, F-91198 Gif sur Yvette, France [1] A 2002 multibeam sonar survey of Mauna Loa’s western flank revealed ten submarine radial vents and three submarine lava flows. Only one submarine radial vent was known previously. The ages of these vents are constrained by eyewitness accounts, geologic relationships, Mn-Fe coatings, and geochemical stratigraphy; they range from 128 years B.P. to possibly 47 ka. Eight of the radial vents produced degassed lavas despite eruption in water depths sufficient to inhibit sulfur degassing. These vents formed truncated cones and short lava flows. Two vents produced undegassed lavas that created ‘‘irregular’’ cones and longer lava flows.