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LATE FORMATIVE FLOODING OF IZAPA AFTER AN ERUPTION OF TACANÁ VOLCANO

Published online by Cambridge University Press:  04 January 2019

José Luis Macías*
Affiliation:
Instituto de Geofísica, Unidad Michoacán, Universidad Nacional Autónoma de México, Campus-Morelia, Morelia, 58090, Michoacán, Mexico
José Luis Arce
Affiliation:
Instituto de Geología, Universidad Nacional Autónoma de México, Ciudad de México, Coyoacán 04510, Mexico
Lucia Capra
Affiliation:
Centro de Geociencias, Universidad Nacional Autónoma de México, Blvd. Juriquilla No. 3001, Juriquilla, Querétaro 76230, Mexico
Ricardo Saucedo
Affiliation:
Instituto de Geología, Universidad Autónoma de San Luis Potosí, Dr. M. Nava no 5, Zona Universitaria, San Luis Potosí 78240, Mexico
Juan Manuel Sánchez-Núñez
Affiliation:
Centro Interdisciplinario de Investigaciones y Estudios sobre Medio Ambiente y Desarrollo, Instituto Politécnico Nacional, Miguel Othón de Mendizabal s/n. Col. La Escalera., 16 Del. Gustavo A. Madero, Mexico City 07320, Mexico
*
E-mail correspondence to: jlmacias@igeofisica.unam.mx
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Abstract

Between the years of 30 b.c. to a.d. 80, during the Late Formative period, the site of Izapa was flooded by lahars associated with an explosive eruption of the San Antonio volcano (part of the Tacaná Volcanic Complex). Computer simulations suggest that hot pyroclastic flows did not impact Izapa directly, but did impact the region considerably, filling and clogging the Cahuacan and Mixcun rivers with hot debris. The material was quickly saturated by heavy rains and, as the water from the rivers overtopped the obstruction, remobilized in the form of a hot mixture of mud and water known as a lahar (or flood of volcanic origin), which flowed down through the piedmont zone along the Cahuacan, Mixcun-Suchiate, and Izapa rivers. At Izapa, the flood took the form of a 6-m catastrophic wave of mud and water that likely destroyed crops and caused many causalities, surrounding the architectural mounds at Izapa with a muddy landscape. The floods also dramatically affected the rivers downstream, undoubtedly wreaking serious damage to the transport and trade of goods along the coast.

Information

Type
Research Article
Copyright
Copyright © Cambridge University Press 2018 
Figure 0

Figure 1. (a) Sketch map showing the location of Tacaná at the Mexico-Guatemala border. (b) Digital elevation model of the Tacaná volcano region. Notice the main drainage system around the volcano and the alluvial/pyroclastic fan where Tapachula and other towns are settled. A, Ahuacatlán; Ca, Cacahoatán; TC, Tuxtla Chico; SR, San Rafael; and VV, Vega del Volcán. Red dashed line indicates the maximum extent of the pyroclastic flow deposits of the San Antonio eruption (30 b.c.–a.d. 80 eruption). Numbers and circles on top of Tacaná correspond to location photographs of Figure 3. Image prepared by Guillermo Cisneros.

Figure 1

Figure 2. (a) Table showing the main eruptions of the Tacaná Volcanic Complex and their correlation with the chronology periods of Chiapanecan Soconuco (Lesure 2011) and Izapa (Rosenswig et al. 2014). (b) Diagrams of modeled calibrated ages of Tacaná eruptions calibrated by using the online version of Oxcal 4.2 (Ramsey 2009) with the IntCal_13 calibration curve (Reimer et al. 2013). Calibration graphs were prepared by Laura Beramendi, with final edits by Macías.

Figure 2

Table 1. Radiocarbon ages of the Tacaná Volcanic Complex compiled by Macías et al. (2015) were calibrated using the online version of Oxcal 4.2 (Bronk Ramsey 2009) with the IntCal_13 calibration curve (Reimer et al. 2013). Samples were arranged in a sequence model, with those related to the same event grouped as a Phase with boundaries. Calibrated ages are reported as the 95.4% (2σ) posterior probability density intervals, with the corresponding median in b.c./a.d. The modeled ages suggest that the Mixcun eruption occurred between 30 b.c.–a.d. 80, which coincides with the Hato phase of the Izapa chronology. A = agreement index. Negative numbers in columns indicate dates Before Christ.

Figure 3

Figure 3. (a) Panoramic view from the southeast of the Tacaná Volcanic Complex. PA, Plan de las Ardillas Dome; SA, San Antonio Volcano. (b) Panoramic view to the northwest of the 1986 explosion crater. It is about 20 × 15 m in diameter (point 1 in Figure 1b) Photograph by Macías. (c) Photograph showing the fumarolic zone at San Antonio Volcano and the hydrothermal alteration (point 2 in Figure 1b). (d) Outcrop of the a.d. 1150–1270 pumice fall deposit (point 3 in Figure 1b). The deposit consists of continuous ash layers at the bottom overlaid by a lapilli-size layer with pumice fragments, totaling 40 cm in thickness. (a–c) Photographs by Arce.

Figure 4

Figure 4. (a) Area covered by the simulation of the Titan-3d computer code for the 30 b.c.–a.d. 80 eruption of the San Antonio Volcano. The simulation was routed over a digital elevation model of 30 m-pixels in horizontal resolution obtained from NASA Shuttle Radar Topography Mission data (SRTM, 1 arc-second). (b) Inundation zones resulted from the Flow-2d computer simulation for the lahars generated after the 30 b.c.–a.d. 80 eruption. (c) Close-up of the inundated area at Izapa Archaeological zone by lahars simulated in Figure 4b. I and II are profiles interpreted in Figure 4d. (d) Inundation profiles at Izapa zone resulting from the lahar simulation. Images prepared by Capra.