dor_id: 4132818

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/265/253

100.1.#.a: Poveda, A.; Cordero, G.

524.#.#.a: Poveda, A., et al. (2008). Chicxulubites: A new class of meteorites?. Geofísica Internacional; Vol. 47 Núm. 3: Julio 1, 2008; 167-172. Recuperado de https://repositorio.unam.mx/contenidos/4132818

245.1.0.a: Chicxulubites: A new class of meteorites?

502.#.#.c: Universidad Nacional Autónoma de México

561.1.#.a: Instituto de Geofísica, UNAM

264.#.0.c: 2008

264.#.1.c: 2008-07-01

653.#.#.a: Chicxulub; cráteres secundarios; fragmentos arrojados; Chicxulub; secondary craters; ejected fragments

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/265

001.#.#.#: 063.oai:revistagi.geofisica.unam.mx:article/265

041.#.7.h: spa

520.3.#.a: It is well known that asteroidal impacts on the Moon and Mars have ejected a large number of fragments that, after traveling in the inner planetary system for thousands or millions of years, occasionally fall on Earth and are recovered as meteorites.It is of interest, therefore, to ask the question: what fraction of the mass excavated from the Chicxulub crater was ejected with escape velocities as the result of the 100 million megaton explosion? These fragments, similarly to what happened with lunar and martian ejecta, can fall onto the Moon, as well as back on the Earth as meteorites: Chicxulubites.A 10 km–diameter asteroid, like the one at Chicxulub, could have produced a number of high velocity fragments with a total mass of about one thousandth of the mass of the projectile. From the work of Vickery (1987) on secondary craters on Mercury, the Moon and Mars, we estimated the mass and the diameter of the largest fragments that would have a velocity larger than the Earth"s escape velocity. Assuming Dohnanyi"s mass frequency distribution, we estimated that the number of fragments with sizes larger than 10 cm and 2 cm is about 4x1010 and 2x1012, respectively. We also estimated the expected fraction of these Chicxulubites to the total number of earth–crossing asteroids (ECA"s) of similar diameter.We conclude that a number of fragments from the Chicxulub crater have fallen onto the Moon and the Earth after becoming ECAs, and are waiting to be identified as Chicxulubites.doi: https://doi.org/10.22201/igeof.00167169p.2008.47.3.77  

773.1.#.t: Geofísica Internacional; Vol. 47 Núm. 3: Julio 1, 2008; 167-172

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: 167-172

264.#.1.b: Instituto de Geofísica, UNAM

doi: https://doi.org/10.22201/igeof.00167169p.2008.47.3.77

handle: 00a5b5c78bf88702

harvesting_date: 2023-06-20 16:00:00.0

856.#.0.q: application/pdf

file_creation_date: 2008-06-30 20:08:02.0

file_modification_date: 2022-05-27 19:30:49.0

file_creator: Poveda A.

file_name: feab53dbf21c56ad7119f394257956cc6b60bcaef8af2572a320d548d913ad77.pdf

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245.1.0.b: Chicxulubites: A new class of meteorites?

last_modified: 2023-06-20 16:00:00

license_url: https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.es

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Artículo

Chicxulubites: A new class of meteorites?

Poveda, A.; Cordero, G.

Instituto de Geofísica, UNAM, publicado en Geofísica Internacional, y cosechado de Revistas UNAM

Licencia de uso

Procedencia del contenido

Entidad o dependencia
Instituto de Geofísica, UNAM
Revista
Repositorio
Contacto
Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx

Cita

Poveda, A., et al. (2008). Chicxulubites: A new class of meteorites?. Geofísica Internacional; Vol. 47 Núm. 3: Julio 1, 2008; 167-172. Recuperado de https://repositorio.unam.mx/contenidos/4132818

Descripción del recurso

Autor(es)
Poveda, A.; Cordero, G.
Tipo
Artículo de Investigación
Área del conocimiento
Físico Matemáticas y Ciencias de la Tierra
Título
Chicxulubites: A new class of meteorites?
Fecha
2008-07-01
Resumen
It is well known that asteroidal impacts on the Moon and Mars have ejected a large number of fragments that, after traveling in the inner planetary system for thousands or millions of years, occasionally fall on Earth and are recovered as meteorites.It is of interest, therefore, to ask the question: what fraction of the mass excavated from the Chicxulub crater was ejected with escape velocities as the result of the 100 million megaton explosion? These fragments, similarly to what happened with lunar and martian ejecta, can fall onto the Moon, as well as back on the Earth as meteorites: Chicxulubites.A 10 km–diameter asteroid, like the one at Chicxulub, could have produced a number of high velocity fragments with a total mass of about one thousandth of the mass of the projectile. From the work of Vickery (1987) on secondary craters on Mercury, the Moon and Mars, we estimated the mass and the diameter of the largest fragments that would have a velocity larger than the Earth"s escape velocity. Assuming Dohnanyi"s mass frequency distribution, we estimated that the number of fragments with sizes larger than 10 cm and 2 cm is about 4x1010 and 2x1012, respectively. We also estimated the expected fraction of these Chicxulubites to the total number of earth–crossing asteroids (ECA"s) of similar diameter.We conclude that a number of fragments from the Chicxulub crater have fallen onto the Moon and the Earth after becoming ECAs, and are waiting to be identified as Chicxulubites.doi: https://doi.org/10.22201/igeof.00167169p.2008.47.3.77  
Tema
Chicxulub; cráteres secundarios; fragmentos arrojados; Chicxulub; secondary craters; ejected fragments
Idioma
spa
ISSN
ISSN-L: 2954-436X; ISSN impreso: 0016-7169

Enlaces