| dc.creator | Gómez Samus, Mauro Leandro | |
| dc.creator | Chimento Ortiz, Nicolás Roberto | |
| dc.creator | Löffler, J. | |
| dc.creator | Rico, Yamile | |
| dc.creator | Sierra, L. | |
| dc.creator | Bidegain, Juan Carlos | |
| dc.date | 2017 | |
| dc.date | 2021-05-11T18:53:29Z | |
| dc.date.accessioned | 2023-07-15T01:41:07Z | |
| dc.date.available | 2023-07-15T01:41:07Z | |
| dc.identifier | http://sedici.unlp.edu.ar/handle/10915/118685 | |
| dc.identifier | issn:1886-7995 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7459194 | |
| dc.description | This paper aims to contribute to the stratigraphic and geochronological knowledge of the Neogene–Quaternary of the geologic province of Tandilia by doing lithostratigraphic, paleomagnetic and paleontological analyses.
Four lithostratigraphic units have been recognized. The oldest (Late Miocene) constitutes a unit composed of colluvium deposits; it lays in erosional unconformity over the Neoproterozoic rocks. This unconformity is related to important events in the Andes during the Middle-Late Miocene. Over the oldest colluvial sediments, and placed in erosional unconformity, there are sediments assigned to the Barker Formation which are essentially fluvial deposits with a development of several paleosols. Owing to the fossil remains, this unit is assigned to the Montehermosan- Chapadmalalan Stage/Age, whereas the paleomagnetic record would correspond to C3A, Gilbert and Gauss chrons. So, the age is narrowed to the timespan 7.1–3.1 Ma (Late Miocene–Early Pliocene). The Vela Formation lays in erosional unconformity over the Barker Formation. It also has fluvial origin, while the youngest unit (Las Ánimas Formation) corresponds to loess. Both units provide normal polarity and were assigned to Brunhes chron (\0.78 Ma). The Vela Formation presents fossil remains from Bonaerian- Lujanian Stage/Age and belongs to the Middle Pleistocene. The hiatus between the Barker and Vela Formations seems to be considerable: it represents at least 2.6 million years. The reason for the lack of sedimentary records is still a matter of discussion. The deposition of Las Animas Formation seems to span the last 40,000 years. However, this could be linked to a major entrance of windcarried sediments during dry periods, including the Last Glacial Maximum. The hiatus between the Vela and Las A ´ nimas Formations may have been over 100,000 years.This paper aims to contribute to the stratigraphic and geochronological knowledge of the Neogene–Quaternary of the geologic province of Tandilia by doing lithostratigraphic, paleomagnetic and paleontological analyses. Four lithostratigraphic units have been recognized. The oldest (Late Miocene) constitutes a unit composed of colluvium deposits; it lays in erosional unconformity over the Neoproterozoic rocks. This unconformity is related to important events in the Andes during the Middle-Late Miocene. Over the oldest colluvial sediments, and placed in erosional unconformity, there are sediments assigned to the Barker Formation which are essentially fluvial deposits with a development of several paleosols. Owing to the fossil remains, this unit is assigned to the Montehermosan- Chapadmalalan Stage/Age, whereas the paleomagnetic record would correspond to C3A, Gilbert and Gauss chrons. So, the age is narrowed to the timespan 7.1–3.1 Ma (Late Miocene–Early Pliocene). The Vela Formation lays in erosional unconformity over the Barker Formation. It also has fluvial origin, while the youngest unit (Las Ánimas Formation) corresponds to loess. Both units provide normal polarity and were assigned to Brunhes chron (\0.78 Ma). The Vela Formation presents fossil remains from Bonaerian- Lujanian Stage/Age and belongs to the Middle Pleistocene. The hiatus between the Barker and Vela Formations seems to be considerable: it represents at least 2.6 million years. The reason for the lack of sedimentary records is still a matter of discussion. The deposition of Las Animas Formation seems to span the last 40,000 years. However, this could be linked to a major entrance of windcarried sediments during dry periods, including the Last Glacial Maximum. The hiatus between the Vela and Las Ánimas Formations may have been over 100,000 years. | |
| dc.description | El objetivo del presente trabajo es contribuir al conocimiento estratigráfico y geocronológico del Neógeno-Cuaternario de la provincia geológica de Tandilia por medio de análisis litoestratigráficos, paleomagnéticos y paleontológicos. Se han reconocido cuatro unidades litoestratigráficas. La más antigua (Mioceno tardío) está compuesta por depósitos coluviales y se encuentra en discordancia erosiva sobre las rocas neoproterozoicas. El origen de esta discordancia se relaciona con importantes eventos en los Andes durante el Mioceno medio-tardío. Sobre los mencionados sedimentos coluviales, mediante una discordancia erosiva, yacen los sedimentos asignados a la Formación Barker. Son esencialmente fluviales, con desarrollo de varios paleosuelos. Debido a los restos fósiles, esta unidad es asignada a la Edad/Piso Montehermosense-Chapadmalalense, mientras que el registro paleomagnético correspondería a los crones C3A, Gilbert y Gauss. Por lo tanto, la edad de la unidad se encuentra en el lapso 7.1–3.1 Ma (Mioceno tardío–Plioceno temprano). La Formación Vela se apoya mediante discordancia erosiva sobre la Formación Barker. También tiene origen fluvial, mientras que la unidad más joven (Formación Las Ánimas) corresponde a loess. Ambas unidades proporcionan polaridad normal y se asignan al Cron Brunhes (<0.78 Ma). La Formación Vela presenta restos fósiles de Edad/Piso Bonaerense-Lujanense y se asigna al Pleistoceno medio. El hiato entre las formaciones de Barker y Vela parece ser considerable: representa al menos 2.6 millones de años. La razón de la falta de registro sedimentario entre ambas unidades es aun motivo de discusión. La depositación de la Formación Las Animas parece abarcar los últimos 40,000 años. Sin embargo, esto podría estar relacionado con un ingreso principal de sedimentos transportados por el viento durante los períodos secos, incluido el último máximo glacial. El hiato entre las formaciones Vela y Las Ánimas puede involucrar más de 100,000 años. | |
| dc.description | Facultad de Ciencias Naturales y Museo | |
| dc.description | Comisión de Investigaciones Científicas de la provincia de Buenos Aires | |
| dc.format | application/pdf | |
| dc.language | en | |
| dc.rights | http://creativecommons.org/licenses/by/4.0/ | |
| dc.rights | Creative Commons Attribution 4.0 International (CC BY 4.0) | |
| dc.subject | Ciencias Naturales | |
| dc.subject | Late Cenozoic | |
| dc.subject | Loess | |
| dc.subject | Argentina | |
| dc.subject | Hiatus | |
| dc.subject | Tandil | |
| dc.title | Neogene-Quaternary in Tandilia, South America: litho- bio- magnetostratigraphy | |
| dc.type | Articulo | |
| dc.type | Articulo | |
