Sohn Robert A, Willis Claire, Humphris Susan, Shank Timothy M, Singh Hanumant, Edmonds Henrietta N, Kunz Clayton, Hedman Ulf, Helmke Elisabeth, Jakuba Michael, Liljebladh Bengt, Linder Julia, Murphy Christopher, Nakamura Ko-Ichi, Sato Taichi, Schlindwein Vera, Stranne Christian, Tausenfreund Maria, Upchurch Lucia, Winsor Peter, Jakobsson Martin, Soule Adam
Woods Hole Oceanographic Institution, Woods Hole, Massachusetts 02543, USA.
Nature. 2008 Jun 26;453(7199):1236-8. doi: 10.1038/nature07075.
Roughly 60% of the Earth's outer surface is composed of oceanic crust formed by volcanic processes at mid-ocean ridges. Although only a small fraction of this vast volcanic terrain has been visually surveyed or sampled, the available evidence suggests that explosive eruptions are rare on mid-ocean ridges, particularly at depths below the critical point for seawater (3,000 m). A pyroclastic deposit has never been observed on the sea floor below 3,000 m, presumably because the volatile content of mid-ocean-ridge basalts is generally too low to produce the gas fractions required for fragmenting a magma at such high hydrostatic pressure. We employed new deep submergence technologies during an International Polar Year expedition to the Gakkel ridge in the Arctic Basin at 85 degrees E, to acquire photographic and video images of 'zero-age' volcanic terrain on this remote, ice-covered ridge. Here we present images revealing that the axial valley at 4,000 m water depth is blanketed with unconsolidated pyroclastic deposits, including bubble wall fragments (limu o Pele), covering a large (>10 km(2)) area. At least 13.5 wt% CO(2) is necessary to fragment magma at these depths, which is about tenfold the highest values previously measured in a mid-ocean-ridge basalt. These observations raise important questions about the accumulation and discharge of magmatic volatiles at ultraslow spreading rates on the Gakkel ridge and demonstrate that large-scale pyroclastic activity is possible along even the deepest portions of the global mid-ocean ridge volcanic system.
地球大约60%的外表面由大洋中脊火山作用形成的洋壳组成。尽管这片广袤的火山地形中只有一小部分经过了目视勘查或采样,但现有证据表明,大洋中脊的爆发性火山喷发很罕见,尤其是在低于海水临界点(3000米)的深度。在3000米以下的海底从未观测到火山碎屑沉积物,大概是因为大洋中脊玄武岩的挥发物含量通常过低,无法在如此高的静水压力下产生使岩浆破碎所需的气体比例。在国际极地年考察期间,我们利用新的深潜技术前往位于东经85度的北极盆地加克尔海脊,获取这片偏远的、被冰覆盖的海脊上“零年龄”火山地形的照片和视频图像。在此,我们展示的图像显示,水深4000米处的轴谷覆盖着未固结的火山碎屑沉积物,包括气泡壁碎片(贝利熔岩),覆盖面积很大(>10平方千米)。在这些深度使岩浆破碎至少需要13.5%(重量)的二氧化碳,这大约是之前在大洋中脊玄武岩中测得的最高值的十倍。这些观测结果引发了关于加克尔海脊超慢速扩张速率下岩浆挥发物的聚集和排放的重要问题,并表明即使在全球大洋中脊火山系统最深的部分也可能发生大规模的火山碎屑活动。