An eruptive history of Maderas volcano using new 40Ar/39Ar ages and geochemical analyses

被引:5
|
作者
Kapelanczyk, Lara [1 ]
Rose, William I. [1 ]
Jicha, Brian [2 ]
机构
[1] Michigan Technol Univ, Dept Geol & Min Engn & Sci, Houghton, MI 49931 USA
[2] Univ Wisconsin, Dept Geosci, Madison, WI USA
基金
美国国家科学基金会;
关键词
40Ar/39Ar dating; Eruptive history; Volcano; Maderas; SANTA-MARIA; EVOLUTION; COMPLEX; SLIP;
D O I
10.1007/s00445-012-0644-7
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Maderas volcano is a small, andesitic stratovolcano located on the island of Ometepe in Lake Nicaragua, Nicaragua, with no record of historic activity. Twenty-one samples were collected in 2010 from lava flows of Maderas. The selected samples were analyzed for whole-rock geochemistry using ICP-AES and/or were dated using the 40Ar/39Ar method. The results of these analyses were combined with previously collected data from Maderas as well as field observations to determine the eruptive history of the volcano and create a geologic map. The results of the geochemical analyses indicate that Maderas has higher concentrations of alkalies than most Nicaraguan and Costa Rican volcanoes including its nearest neighbor, Concepcin volcano. It is also different from Concepcin in that it displays higher incompatible elements. Determined age dates range from 179.2 +/- 16.4 ka to 70.5 +/- 6.1 ka. Based on these ages and the geomorphology of the volcano which is characterized by a bisecting graben, it is proposed that Maderas experienced two generations of development: initial build-up of the older cone including pre-graben lava flows, followed by post-graben lava flows. The ages also indicate that Maderas is markedly older than Concepcin which is historically active. Volcanic hazards were also assessed. The 40Ar/39Ar ages indicate that Maderas has likely been inactive for tens of thousands of years and future volcanic eruptions are not considered an immediate hazard. However, earthquake and lahar hazards exist for the communities around the volcano. The steep slopes of the eroded older cone are the most likely sources of lahar hazards.
引用
收藏
页码:2007 / 2021
页数:15
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