Tectonic-structural systems of Mars: Is it possible to use them to reconstruct its thermal evolution?
Barosio, Antonio H.; Valdés Galicia, J. F.
Instituto de Geofísica, UNAM, publicado en Geofísica Internacional, y cosechado de Revistas UNAM
dor_id: 4133426
506.#.#.a: Público
590.#.#.d: Los artículos enviados a la revista "Geofísica Internacional", se juzgan por medio de un proceso de revisión por pares
510.0.#.a: Consejo Nacional de Ciencia y Tecnología (CONACyT); Scientific Electronic Library Online (SciELO); SCOPUS, Dialnet, Directory of Open Access Journals (DOAJ); Geobase
561.#.#.u: https://www.geofisica.unam.mx/
650.#.4.x: Físico Matemáticas y Ciencias de la Tierra
336.#.#.b: article
336.#.#.3: Artículo de Investigación
336.#.#.a: Artículo
351.#.#.6: http://revistagi.geofisica.unam.mx/index.php/RGI
351.#.#.b: Geofísica Internacional
351.#.#.a: Artículos
harvesting_group: RevistasUNAM
270.1.#.p: Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx
590.#.#.c: Open Journal Systems (OJS)
270.#.#.d: MX
270.1.#.d: México
590.#.#.b: Concentrador
883.#.#.u: https://revistas.unam.mx/catalogo/
883.#.#.a: Revistas UNAM
590.#.#.a: Coordinación de Difusión Cultural
883.#.#.1: https://www.publicaciones.unam.mx/
883.#.#.q: Dirección General de Publicaciones y Fomento Editorial
850.#.#.a: Universidad Nacional Autónoma de México
856.4.0.u: http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/927/876
100.1.#.a: Barosio, Antonio H.; Valdés Galicia, J. F.
524.#.#.a: Barosio, Antonio H., et al. (2004). Tectonic-structural systems of Mars: Is it possible to use them to reconstruct its thermal evolution?. Geofísica Internacional; Vol. 43 Núm. 2: Abril 1, 2004; 295-299. Recuperado de https://repositorio.unam.mx/contenidos/4133426
245.1.0.a: Tectonic-structural systems of Mars: Is it possible to use them to reconstruct its thermal evolution?
502.#.#.c: Universidad Nacional Autónoma de México
561.1.#.a: Instituto de Geofísica, UNAM
264.#.0.c: 2004
264.#.1.c: 2004-04-01
653.#.#.a: Marte; Esfuerzos; Deformaciones; Crestas arrugadas; Evolución térmica; Mars; Stresses; Deformations; Wrinkle ridges; Thermal evolution
506.1.#.a: La titularidad de los derechos patrimoniales de esta obra pertenece a las instituciones editoras. Su uso se rige por una licencia Creative Commons BY-NC-SA 4.0 Internacional, https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.es, para un uso diferente consultar al responsable jurídico del repositorio por medio del correo electrónico revistagi@igeofisica.unam.mx
884.#.#.k: http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/927
001.#.#.#: 063.oai:revistagi.geofisica.unam.mx:article/927
041.#.7.h: spa
520.3.#.a: This work tries to establish the possible relationship among cortical stresses evidenced by faults mapped in the surface and thermal evolution on Mars. To achieve it, we made an initial classification of the tectonic-structural systems that appear in surface, which were detected by diverse missions from orbit. This classification was based on the association of the tectonic-structural features with specific geologic features, which allows to divide them in four groups: I) Grabens and normal faults parallel and radially associated to the Tharsis volcanic bulge. II) Tectonic systems associated to the volcanoes that crown the Tharsis bulge, to the volcanic mons of Elysium and the surroundings of the Isidis, Argyre and Hellas impact basins. III) Wrinkle ridges that extend for almost the entire planet. IV) A series of secondary ridges associated to the crustal dichotomy. Later we suggest a classification based on the surface extension and on the possible geologic processes that could have originated the different tectonic structures. This last classification allows to associate stresses to specific processes and it contemplates three groups of deformations: local, regional and global deformations. Finally the possible causes of the stresses are suggested, which include: global stresses due to expansion or thermal contraction, regional or local stresses due to thermal anomalies in the mantle and to lithospheric loads, stresses due to impacts, among others. This allowed to suggest a possible thermal evolution that outlines an initial heating for accretion, followed by an abrupt cooling in a very short period of time and a later secular cooling, which remains in the present time.doi: https://doi.org/10.22201/igeof.00167169p.2004.43.2.182
773.1.#.t: Geofísica Internacional; Vol. 43 Núm. 2: Abril 1, 2004; 295-299
773.1.#.o: http://revistagi.geofisica.unam.mx/index.php/RGI
022.#.#.a: ISSN-L: 2954-436X; ISSN impreso: 0016-7169
310.#.#.a: Trimestral
300.#.#.a: Páginas: 295-299
264.#.1.b: Instituto de Geofísica, UNAM
doi: https://doi.org/10.22201/igeof.00167169p.2004.43.2.182
handle: 00817e09eaf7cc17
harvesting_date: 2023-06-20 16:00:00.0
856.#.0.q: application/pdf
file_creation_date: 2022-07-19 17:53:32.0
file_modification_date: 2022-07-19 17:53:32.0
file_creator: Antonio H. Barosio
file_name: 16a425df3fb13ae9200dae152925b632918fa49c41981c792e6a9c6702363f64.pdf
file_pages_number: 5
file_format_version: application/pdf; version=1.3
file_size: 1054617
245.1.0.b: Tectonic-structural systems of Mars: Is it possible to use them to reconstruct its thermal evolution?
last_modified: 2023-06-20 16:00:00
license_url: https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.es
license_type: by-nc-sa
Barosio, Antonio H.; Valdés Galicia, J. F.
Instituto de Geofísica, UNAM, publicado en Geofísica Internacional, y cosechado de Revistas UNAM
Barosio, Antonio H., et al. (2004). Tectonic-structural systems of Mars: Is it possible to use them to reconstruct its thermal evolution?. Geofísica Internacional; Vol. 43 Núm. 2: Abril 1, 2004; 295-299. Recuperado de https://repositorio.unam.mx/contenidos/4133426