- published: 15 Jan 2014
- views: 143
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Mars Reconnaissance Orbiter
Fissure near Cerberus Fossae with Tectonic Morphologies
Looking for Salts on Mars
Recent Volcanism in Valles Marineris
Dunes on the Rim of the Hellas Impact Basin
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. The fossae (Latin plural for a “ditch” or “depression”) are in close proximity and related to the formation of Athabasca Valles, which lies to the west. These rifts are collapse features believed to form by volcanic and tectonic processes. In this composite image (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), we can see that the rift is not continuous, but discontinuous and offset. The offset could be the result of a preexisting subsurface discontinuity, such as a fault.
The close-up view of HiRISE infrared color (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-2.jpg) shows us a plethora of information about Cerberus Fossae and the great amount of detail that HiRISE captures. The clear view of boulders strewn in shadowed areas of the rift is a testament to the high signal-to-noise capability and high resolution of the HiRISE camera; aeolian dunes along with boulders deposited from erosion of the rift walls are also visible in detail.
Using the pixel-length of the shadow within the rift, the incidence angle of the Sun at the time the image was taken, and some trigonometry, the approximate depth of the various sections of Cerberus Fossae can be estimated. Based on this simple method, an approximate depth is 260 meters. This estimate suggests that the rift is as wide as it is deep.
Another remarkable aspect of this image is the stark contrasts it captures: light-toned dusty surfaces that surround the rift versus the dark blue basaltic sands and the shadows within the rift. The detail that HiRISE can provide is indeed phenomenal, and as demonstrated here, the infrared color provides additional information. Why, for instance, is the floor of Cerberus Fossae a deep blue, and why is there such a contrast with the orange-grayish Martian surface? It's not water! The volcanic and mafic sand contains unoxidized iron, which appears a deep blue, while the Martian surface is covered by oxidized iron-bearing dust which appears orange-grayish.
Written by: Kayle Hansen, Livio Tornabene, Eric Pilles, Ryan Hopkins (audio: Tre Gibbs) (7 January 2015)
Related Media
Mars Tectonic Processes:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8mztHqDMYlVtd9UD3CiGJEH
HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument):
http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ
HiRISE, High Resolution Imaging Science Experiment:
"Explore Mars, one giant image at a time."
The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.
HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera.
Credit: NASA/JPL/University of Arizona
- published: 11 Aug 2015
- views: 39
The linearity of the volcanic vent shown in this HiRISE image (http://static.uahirise.org/images/2014/details/cut/ESP_034716_1875.jpg), in conjunction with evidence of lava flow from the vent, suggests control by combined volcano-tectonic processes. The details of this vent gained by HiRISE should provide insight into those volcano-tectonic processes along Cerberus Fossae fissures in two ways. The nature of both the volcanic products along this fissure, and the geometries of the linear vent, will permit comparison with similar, non-volcanic fissures at Cerberus. And results from these comparisons will provide insight into the orientation of the underlying dike system that may have controlled the ascent of water to the surface in the Cerberus region.
Future topographic analysis with a second image in order to create a 3D picture will enable us to measure the heights of the associated flows and better understand their volcanic history.
Written by: HiRISE Science Team (15 January 2014)
Related Media
Mars Volcanic Processes:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8m4E3fk4bmS3Nus6rtvm0s7
HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument):
http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ
HiRISE, High Resolution Imaging Science Experiment:
"Explore Mars, one giant image at a time."
The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.
HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera.
Credit: NASA/JPL/University of Arizona
- published: 15 Jan 2014
- views: 358
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.) http://www.uahirise.org/ESP_039187_1915
- published: 07 Jan 2015
- views: 212
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de rifts localizados en Elysium Planitia, justo al norte del ecuador de Marte. Las fossae (el término plural en latín para las palabras “zanja” o “depresión”) están próximas y relacionadas con la formación de Athabasca Valles, que se encuentra al oeste. Estos rifts son formas de colapso que se piensa están formadas por procesos volcánicos y tectónicos. En esta imagen compuesta (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), podemos ver que el rift no es continuo, sino discontinuo y está desplazado. Estos desplazamientos podrían ser el resultado de una discontinuidad presente bajo la superficie, como una falla.
La imagen de cerca de la HiRISE (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-2.jpg) en color infrarrojo nos aporta una gran diversidad de información sobre Cerberus Fossae y una gran cantidad de detalles que es capaz de capturar la HiRISE. La imagen clara de rocas esparcidas en las zonas en sombra del rift es un testamento de la gran capacidad en la relación señal/ruido y la alta resolución de la cámara HiRISE. Las dunas eólicas, junto con las rocas depositadas por la erosión que ocurre en las paredes del rift también son visibles en detalle.
Usando la longitud en píxeles de la sombra dentro del rift, el ángulo de incidencia del Sol a la hora que se hizo la foto y un poco de trigonometría, podemos estimar de una manera aproximada la profundidad de varios segmentos de Cerberus Fossae. Basándonos en este simple método se calcula una profundidad aproximada de 260 metros. Esta estimación sugiere que el rift es tan ancho como profundo.
Otro aspecto destacable de esta imagen son los fuertes contrastes que captura: las superficies polvorientas de tonos claros que rodean el rift contra las arenas basálticas de color oscuro y también las sombras que hay dentro del rift. Los detalles que la HiRISE puede mostrar son ciertamente fenomenales, y como se demuestra aquí, los colores en el infrarrojo nos aportan una información adicional. ¿Por qué, por ejemplo, tiene el fondo de Cerberus Fossae un color azul oscuro, y por qué hay tanto contraste con la superficie de Marte de tonos grises y anaranjados? ¡No es agua! La arena volcánica y máfica contiene hierro sin oxidar, que aparece de un color azul oscuro, mientras que la superficie de Marte está cubierta por polvo que contiene hierro en estado oxidado y que aparece con tonos grises y anaranjados.
(7 de enero de 2015)
Traducción: Nahúm Méndez Chazarra
Geología de Marte: HiRISE Cámara del Orbitador Reconocimiento Marte MRO - Mars Reconnaissance Orbiter:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8mzXnC-vP_IQMKiQvh5_gR3
NASA/Jet Propulsion Laboratory/Universidad de Arizona
Cámara HiRISE (High-Resolution Imaging Science Experiment, Experimento Científico de Imágenes de Alta Resolución) montada a bordo de la nave espacial MRO.
Imágenes desde HiRISE, la cámara de alta resolución a bordo de la sonda MRO. La Mars Reconnaissance Orbiter (acrónimo: MRO) es una nave espacial multipropósito, lanzada el 12 de agosto de 2005 para el avance del conocimiento humano de Marte a través de la observación detallada, con el fin de examinar potenciales zonas de aterrizaje para futuras misiones en la superficie y de realizar transmisiones para éstas. Es el cuarto satélite artificial en Marte (uniéndose a Mars Express, Mars Odyssey y Mars Global Surveyor). El 10 de octubre de 2006 comenzó su inserción en la la órbita marciana, concluyendo su fase de aerofrenado el 4 de septiembre. Sus estudios comienzan tras la conjunción solar de noviembre del mismo año.
La High Resolution Imaging Science Experiment es una cámara situada a bordo del Mars Reconnaissance Orbiter. Con un peso de 65 kg, este instrumento de 40 millones de dólares fue construido por Ball Aerospace & Technologies Corp bajo la dirección del departamento lunar y planetario de la Universidad de Arizona. Consiste en un Telescopio reflector de 0,5 metros de diámetro, el más grande de cualquier misión interplanetaria. Permite fotografiar con una resolución por encima de los 0,3 metros, diferenciando objetos de 1 metro de diámetro (aproximadamente una bola de playa).
Gracias a las fotos de alta resolución se han descubierto nuevos detalles de la geología marciana, los cuales dieron como resultado el descubrimiento de terreno que indicaba la presencia dióxido de carbono líquido o agua en la superficie en su pasado geológico reciente.
En agosto de 2015 la MRO cumplió diez años desde su lanzamiento, siguiendo la observación de Marte desde una órbita en torno a él y enviando a la Tierra información sobre el Planeta Rojo.
- published: 04 Oct 2015
- views: 90
This is a small volcano superposed on the flanks of a larger one of the Cerberus Tholi. This smaller feature has a single vent (http://static.uahirise.org/images/2012/details/cut/ESP_024378_1880.jpg), aligned along a Cerberus Fossae trough, and it has flows radiating away from this vent in all directions, somewhat looking like a flower. These flows appear somewhat darker than their surroundings, though this might be owing to roughness as much as to relative youth. Note that even at Context Camera (CTX) scale, we can see that there are some small impact craters superimposed on this feature, indicating that it is not entirely young.
This caption is based on the original science rationale.
Written by: HiRISE Science Team (4 January 2012)
Related Media
Mars Volcanic Processes:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8m4E3fk4bmS3Nus6rtvm0s7
HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument):
http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ
HiRISE, High Resolution Imaging Science Experiment:
"Explore Mars, one giant image at a time."
The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.
HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera.
Credit: NASA/JPL/University of Arizona
- published: 09 Aug 2015
- views: 19
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.)
http://www.uahirise.org/ESP_039187_1915
Credit: NASA/JPL/University of Arizona
- published: 09 Jan 2015
- views: 15
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de "rifts" localizados en Elysium Planitia, justo al norte del ecuador de Marte. http://www.uahirise.org/es/ESP_039187_1915
- published: 04 Feb 2015
- views: 12
Cerberus is a large "dark spot" (an albedo feature) located on Mars and named after the mythical dog Cerberus. The arcuate markings in the upper right are in the Amazonis plains and may be sand drifts. The Elysium volcano, a yellow area north of Cerberus, has several channels radiating from its flanks. The three bright spots, upper left, are volcanoes partially veiled by thin clouds.
High resolution images show the bulk of the Cerberus Plains is covered by platy-ridged and inflated lavas, which are interpreted as insulated sheet flows. Eastern Cerberus Plains lavas originate at Cerberus Fossae fissures and shields. Some flows extend for 2000 km through Marte Valles into Amazonis Planitia. Athabasca Valles are both incised into pristine lavas and embayed by pristine lavas, indicating that Athabascan fluvial events were contemporaneous with volcanic eruptions. Deposits of the Medusae Fossae Formation lie both over and under lavas, suggesting the deposition of the Medusae Fossae Formation was contemporaneous with volcanism. Statistics of small craters indicate lavas in the Western Cerberus Plains may be less than a million years old, but the model isochrons may be unreliable if the small crater population is dominated by secondary craters. Images showing no large craters with diameters 500 m superimposed on Western Cerberus Plains lavas indicate the same surface is younger than 49 Ma.
"Batman's Fortress" on Cerberus, Mars
These are my own observations. In future I'll upload more and more interesting things seen in NASA's images, so please subscribe!
I will also add the coordinates soon; until then please try to have some fun finding them for yourself, surely you will find more interesting stuff!
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All thanks go to NASA/JPL/Malin Space Science Systems. and European Space Agency for providing the images used in this video.
http://www.nasa.gov/
http://www.jpl.nasa.gov/
http://www.msss.com/
http://www.esa.int
Bibliography: http://en.wikipedia.org
- published: 14 Feb 2015
- views: 469
This observation was taken to investigate the topography near the source of fluids from the Cerberus Fossae fractures in the Elysium Planitia region of Mars.
There are distinct channels carved into the terrain here, presumably by floods of water. However, the terrain is coated with lava, and this situation--where flood-eroded channels are completely coated with lava--is seen in many parts of Mars.
This leads some researchers to suggest that the channels were actually carved by the flowing lava, and that there was no flood of water. Images like these are helping to test these ideas.
credit: NASA/JPL/University of Arizona
source: http://www.uahirise.org/ESP_026303_1945
- published: 12 Apr 2012
- views: 1479
location on Google Map
The Cerberus Fossae are a series of semi-parallel fissures on Mars formed by faults which pulled the crust apart in the Cerberus region (9°N, 197°W). Ripples seen at the bottom of the fault are sand blown by the wind [1]. The underlying cause for the faulting was magma pressure related to the formation of the Elysium Volcanic field, located to the northwest. The faults pass through pre-existing features such as hills, indicating that it is a younger feature[2]. The formation of the fossae is suspected to have released pressurised underground water, previously confined by the cryosphere, with flow rates up to 2 × 106 m3s−1, leading to the creation of the Athabasca Valles.
However, early radar analysis suggests there's no evidence of 'pack ice' tens of metres thick as hypothesised based on the images from Mars Express of the area. This is in support of the US view of images of the area, based on impact crater morphology which do not show any evidences of meteorite hitting anything but solid stone lava fields.
This page contains text from Wikipedia, the Free Encyclopedia -
http://en.wikipedia.org/wiki/Cerberus_Fossae
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
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4:18Cerberus Fossae, Mars
Cerberus Fossae, MarsCerberus Fossae, Mars
Mars Reconnaissance Orbiter Fissure near Cerberus Fossae with Tectonic Morphologies Looking for Salts on Mars Recent Volcanism in Valles Marineris Dunes on the Rim of the Hellas Impact Basin -
2:18Mars Geology: The Eastern Portion of Cerberus Fossae
Mars Geology: The Eastern Portion of Cerberus FossaeMars Geology: The Eastern Portion of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. The fossae (Latin plural for a “ditch” or “depression”) are in close proximity and related to the formation of Athabasca Valles, which lies to the west. These rifts are collapse features believed to form by volcanic and tectonic processes. In this composite image (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), we can see that the rift is not continuous, but discontinuous and offset. The offset could be the result of a preexisting subsurface discontinuity, such as a fault. The close-up view of HiRISE infrared color (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-2.jpg) shows us a plethora of information about Cerberus Fossae and the great amount of detail that HiRISE captures. The clear view of boulders strewn in shadowed areas of the rift is a testament to the high signal-to-noise capability and high resolution of the HiRISE camera; aeolian dunes along with boulders deposited from erosion of the rift walls are also visible in detail. Using the pixel-length of the shadow within the rift, the incidence angle of the Sun at the time the image was taken, and some trigonometry, the approximate depth of the various sections of Cerberus Fossae can be estimated. Based on this simple method, an approximate depth is 260 meters. This estimate suggests that the rift is as wide as it is deep. Another remarkable aspect of this image is the stark contrasts it captures: light-toned dusty surfaces that surround the rift versus the dark blue basaltic sands and the shadows within the rift. The detail that HiRISE can provide is indeed phenomenal, and as demonstrated here, the infrared color provides additional information. Why, for instance, is the floor of Cerberus Fossae a deep blue, and why is there such a contrast with the orange-grayish Martian surface? It's not water! The volcanic and mafic sand contains unoxidized iron, which appears a deep blue, while the Martian surface is covered by oxidized iron-bearing dust which appears orange-grayish. Written by: Kayle Hansen, Livio Tornabene, Eric Pilles, Ryan Hopkins (audio: Tre Gibbs) (7 January 2015) Related Media Mars Tectonic Processes: https://www.youtube.com/playlist?list=PL6vzpF_OEV8mztHqDMYlVtd9UD3CiGJEH HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument): http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ HiRISE, High Resolution Imaging Science Experiment: "Explore Mars, one giant image at a time." The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena. HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera. Credit: NASA/JPL/University of Arizona -
0:56Mars Geology: Fissure near Cerberus Fossae with Tectonic Morphologies
Mars Geology: Fissure near Cerberus Fossae with Tectonic MorphologiesMars Geology: Fissure near Cerberus Fossae with Tectonic Morphologies
The linearity of the volcanic vent shown in this HiRISE image (http://static.uahirise.org/images/2014/details/cut/ESP_034716_1875.jpg), in conjunction with evidence of lava flow from the vent, suggests control by combined volcano-tectonic processes. The details of this vent gained by HiRISE should provide insight into those volcano-tectonic processes along Cerberus Fossae fissures in two ways. The nature of both the volcanic products along this fissure, and the geometries of the linear vent, will permit comparison with similar, non-volcanic fissures at Cerberus. And results from these comparisons will provide insight into the orientation of the underlying dike system that may have controlled the ascent of water to the surface in the Cerberus region. Future topographic analysis with a second image in order to create a 3D picture will enable us to measure the heights of the associated flows and better understand their volcanic history. Written by: HiRISE Science Team (15 January 2014) Related Media Mars Volcanic Processes: https://www.youtube.com/playlist?list=PL6vzpF_OEV8m4E3fk4bmS3Nus6rtvm0s7 HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument): http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ HiRISE, High Resolution Imaging Science Experiment: "Explore Mars, one giant image at a time." The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena. HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera. Credit: NASA/JPL/University of Arizona -
2:18The Eastern Portion of Cerberus Fossae
The Eastern Portion of Cerberus FossaeThe Eastern Portion of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.) http://www.uahirise.org/ESP_039187_1915 -
3:56The Cerberus Fossae, Woodford
The Cerberus Fossae, WoodfordThe Cerberus Fossae, Woodford
-
1:01Cerberus Fossae: In the Relay Zone
Cerberus Fossae: In the Relay Zone -
2:35Geología de Marte: La Parte Oriental de Cerberus Fossae
Geología de Marte: La Parte Oriental de Cerberus FossaeGeología de Marte: La Parte Oriental de Cerberus Fossae
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de rifts localizados en Elysium Planitia, justo al norte del ecuador de Marte. Las fossae (el término plural en latín para las palabras “zanja” o “depresión”) están próximas y relacionadas con la formación de Athabasca Valles, que se encuentra al oeste. Estos rifts son formas de colapso que se piensa están formadas por procesos volcánicos y tectónicos. En esta imagen compuesta (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), podemos ver que el rift no es continuo, sino discontinuo y está desplazado. Estos desplazamientos podrían ser el resultado de una discontinuidad presente bajo la superficie, como una falla. La imagen de cerca de la HiRISE (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-2.jpg) en color infrarrojo nos aporta una gran diversidad de información sobre Cerberus Fossae y una gran cantidad de detalles que es capaz de capturar la HiRISE. La imagen clara de rocas esparcidas en las zonas en sombra del rift es un testamento de la gran capacidad en la relación señal/ruido y la alta resolución de la cámara HiRISE. Las dunas eólicas, junto con las rocas depositadas por la erosión que ocurre en las paredes del rift también son visibles en detalle. Usando la longitud en píxeles de la sombra dentro del rift, el ángulo de incidencia del Sol a la hora que se hizo la foto y un poco de trigonometría, podemos estimar de una manera aproximada la profundidad de varios segmentos de Cerberus Fossae. Basándonos en este simple método se calcula una profundidad aproximada de 260 metros. Esta estimación sugiere que el rift es tan ancho como profundo. Otro aspecto destacable de esta imagen son los fuertes contrastes que captura: las superficies polvorientas de tonos claros que rodean el rift contra las arenas basálticas de color oscuro y también las sombras que hay dentro del rift. Los detalles que la HiRISE puede mostrar son ciertamente fenomenales, y como se demuestra aquí, los colores en el infrarrojo nos aportan una información adicional. ¿Por qué, por ejemplo, tiene el fondo de Cerberus Fossae un color azul oscuro, y por qué hay tanto contraste con la superficie de Marte de tonos grises y anaranjados? ¡No es agua! La arena volcánica y máfica contiene hierro sin oxidar, que aparece de un color azul oscuro, mientras que la superficie de Marte está cubierta por polvo que contiene hierro en estado oxidado y que aparece con tonos grises y anaranjados. (7 de enero de 2015) Traducción: Nahúm Méndez Chazarra Geología de Marte: HiRISE Cámara del Orbitador Reconocimiento Marte MRO - Mars Reconnaissance Orbiter: https://www.youtube.com/playlist?list=PL6vzpF_OEV8mzXnC-vP_IQMKiQvh5_gR3 NASA/Jet Propulsion Laboratory/Universidad de Arizona Cámara HiRISE (High-Resolution Imaging Science Experiment, Experimento Científico de Imágenes de Alta Resolución) montada a bordo de la nave espacial MRO. Imágenes desde HiRISE, la cámara de alta resolución a bordo de la sonda MRO. La Mars Reconnaissance Orbiter (acrónimo: MRO) es una nave espacial multipropósito, lanzada el 12 de agosto de 2005 para el avance del conocimiento humano de Marte a través de la observación detallada, con el fin de examinar potenciales zonas de aterrizaje para futuras misiones en la superficie y de realizar transmisiones para éstas. Es el cuarto satélite artificial en Marte (uniéndose a Mars Express, Mars Odyssey y Mars Global Surveyor). El 10 de octubre de 2006 comenzó su inserción en la la órbita marciana, concluyendo su fase de aerofrenado el 4 de septiembre. Sus estudios comienzan tras la conjunción solar de noviembre del mismo año. La High Resolution Imaging Science Experiment es una cámara situada a bordo del Mars Reconnaissance Orbiter. Con un peso de 65 kg, este instrumento de 40 millones de dólares fue construido por Ball Aerospace & Technologies Corp bajo la dirección del departamento lunar y planetario de la Universidad de Arizona. Consiste en un Telescopio reflector de 0,5 metros de diámetro, el más grande de cualquier misión interplanetaria. Permite fotografiar con una resolución por encima de los 0,3 metros, diferenciando objetos de 1 metro de diámetro (aproximadamente una bola de playa). Gracias a las fotos de alta resolución se han descubierto nuevos detalles de la geología marciana, los cuales dieron como resultado el descubrimiento de terreno que indicaba la presencia dióxido de carbono líquido o agua en la superficie en su pasado geológico reciente. En agosto de 2015 la MRO cumplió diez años desde su lanzamiento, siguiendo la observación de Marte desde una órbita en torno a él y enviando a la Tierra información sobre el Planeta Rojo. -
0:44Mars Geology: Small Floral-Shaped Volcano on Cerberus Fossae
Mars Geology: Small Floral-Shaped Volcano on Cerberus FossaeMars Geology: Small Floral-Shaped Volcano on Cerberus Fossae
This is a small volcano superposed on the flanks of a larger one of the Cerberus Tholi. This smaller feature has a single vent (http://static.uahirise.org/images/2012/details/cut/ESP_024378_1880.jpg), aligned along a Cerberus Fossae trough, and it has flows radiating away from this vent in all directions, somewhat looking like a flower. These flows appear somewhat darker than their surroundings, though this might be owing to roughness as much as to relative youth. Note that even at Context Camera (CTX) scale, we can see that there are some small impact craters superimposed on this feature, indicating that it is not entirely young. This caption is based on the original science rationale. Written by: HiRISE Science Team (4 January 2012) Related Media Mars Volcanic Processes: https://www.youtube.com/playlist?list=PL6vzpF_OEV8m4E3fk4bmS3Nus6rtvm0s7 HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument): http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ HiRISE, High Resolution Imaging Science Experiment: "Explore Mars, one giant image at a time." The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena. HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera. Credit: NASA/JPL/University of Arizona -
2:18Mars: The Eastern Portion of Cerberus Fossae
Mars: The Eastern Portion of Cerberus FossaeMars: The Eastern Portion of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.) http://www.uahirise.org/ESP_039187_1915 Credit: NASA/JPL/University of Arizona -
2:35La parte oriental de Cerberus Fossae
La parte oriental de Cerberus FossaeLa parte oriental de Cerberus Fossae
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de "rifts" localizados en Elysium Planitia, justo al norte del ecuador de Marte. http://www.uahirise.org/es/ESP_039187_1915 -
0:40Mars News: "Batman's Fortress" on Cerberus
Mars News: "Batman's Fortress" on CerberusMars News: "Batman's Fortress" on Cerberus
Cerberus is a large "dark spot" (an albedo feature) located on Mars and named after the mythical dog Cerberus. The arcuate markings in the upper right are in the Amazonis plains and may be sand drifts. The Elysium volcano, a yellow area north of Cerberus, has several channels radiating from its flanks. The three bright spots, upper left, are volcanoes partially veiled by thin clouds. High resolution images show the bulk of the Cerberus Plains is covered by platy-ridged and inflated lavas, which are interpreted as insulated sheet flows. Eastern Cerberus Plains lavas originate at Cerberus Fossae fissures and shields. Some flows extend for 2000 km through Marte Valles into Amazonis Planitia. Athabasca Valles are both incised into pristine lavas and embayed by pristine lavas, indicating that Athabascan fluvial events were contemporaneous with volcanic eruptions. Deposits of the Medusae Fossae Formation lie both over and under lavas, suggesting the deposition of the Medusae Fossae Formation was contemporaneous with volcanism. Statistics of small craters indicate lavas in the Western Cerberus Plains may be less than a million years old, but the model isochrons may be unreliable if the small crater population is dominated by secondary craters. Images showing no large craters with diameters 500 m superimposed on Western Cerberus Plains lavas indicate the same surface is younger than 49 Ma. "Batman's Fortress" on Cerberus, Mars These are my own observations. In future I'll upload more and more interesting things seen in NASA's images, so please subscribe! I will also add the coordinates soon; until then please try to have some fun finding them for yourself, surely you will find more interesting stuff! Join our facebook group: https://www.facebook.com/groups/marsancientnews/?fref=ts All thanks go to NASA/JPL/Malin Space Science Systems. and European Space Agency for providing the images used in this video. http://www.nasa.gov/ http://www.jpl.nasa.gov/ http://www.msss.com/ http://www.esa.int Bibliography: http://en.wikipedia.org -
0:40Eroded Terrain Near Volcanic Fissures [720p]
Eroded Terrain Near Volcanic Fissures [720p]Eroded Terrain Near Volcanic Fissures [720p]
This observation was taken to investigate the topography near the source of fluids from the Cerberus Fossae fractures in the Elysium Planitia region of Mars. There are distinct channels carved into the terrain here, presumably by floods of water. However, the terrain is coated with lava, and this situation--where flood-eroded channels are completely coated with lava--is seen in many parts of Mars. This leads some researchers to suggest that the channels were actually carved by the flowing lava, and that there was no flood of water. Images like these are helping to test these ideas. credit: NASA/JPL/University of Arizona source: http://www.uahirise.org/ESP_026303_1945
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Cerberus Fossae, Mars
Mars Reconnaissance Orbiter Fissure near Cerberus Fossae with Tectonic Morphologies Looking for Salts on Mars Recent Volcanism in Valles Marineris Dunes on the Rim of the Hellas Impact Basin -
Mars Geology: The Eastern Portion of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. The fossae (Latin plural for a “ditch” or “depression”) are in close proximity and related to the formation of Athabasca Valles, which lies to the west. These rifts are collapse features believed to form by volcanic and tectonic processes. In this composite image (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), we can see that the rift is not continuous, but discontinuous and offset. The offset could be the result of a preexisting subsurface discontinuity, such as a fault. The close-up view of HiRISE infrared color (http://static.uahirise.org/images/2015/details/... -
Mars Geology: Fissure near Cerberus Fossae with Tectonic Morphologies
The linearity of the volcanic vent shown in this HiRISE image (http://static.uahirise.org/images/2014/details/cut/ESP_034716_1875.jpg), in conjunction with evidence of lava flow from the vent, suggests control by combined volcano-tectonic processes. The details of this vent gained by HiRISE should provide insight into those volcano-tectonic processes along Cerberus Fossae fissures in two ways. The nature of both the volcanic products along this fissure, and the geometries of the linear vent, will permit comparison with similar, non-volcanic fissures at Cerberus. And results from these comparisons will provide insight into the orientation of the underlying dike system that may have controlled the ascent of water to the surface in the Cerberus region. Future topographic analysis with a seco... -
The Eastern Portion of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.) http://www.uahirise.org/ESP_039187_1915 -
The Cerberus Fossae, Woodford
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Geología de Marte: La Parte Oriental de Cerberus Fossae
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de rifts localizados en Elysium Planitia, justo al norte del ecuador de Marte. Las fossae (el término plural en latín para las palabras “zanja” o “depresión”) están próximas y relacionadas con la formación de Athabasca Valles, que se encuentra al oeste. Estos rifts son formas de colapso que se piensa están formadas por procesos volcánicos y tectónicos. En esta imagen compuesta (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), podemos ver que el rift no es continuo, sino discontinuo y está desplazado. Estos desplazamientos podrían ser el resultado de una discontinuidad presente bajo la superficie, como una falla. La imagen de cerca de la HiRISE (http://static.uahirise.org... -
Mars Geology: Small Floral-Shaped Volcano on Cerberus Fossae
This is a small volcano superposed on the flanks of a larger one of the Cerberus Tholi. This smaller feature has a single vent (http://static.uahirise.org/images/2012/details/cut/ESP_024378_1880.jpg), aligned along a Cerberus Fossae trough, and it has flows radiating away from this vent in all directions, somewhat looking like a flower. These flows appear somewhat darker than their surroundings, though this might be owing to roughness as much as to relative youth. Note that even at Context Camera (CTX) scale, we can see that there are some small impact craters superimposed on this feature, indicating that it is not entirely young. This caption is based on the original science rationale. Written by: HiRISE Science Team (4 January 2012) Related Media Mars Volcanic Processes: https://w... -
Mars: The Eastern Portion of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.) http://www.uahirise.org/ESP_039187_1915 Credit: NASA/JPL/University of Arizona -
La parte oriental de Cerberus Fossae
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de "rifts" localizados en Elysium Planitia, justo al norte del ecuador de Marte. http://www.uahirise.org/es/ESP_039187_1915 -
Mars News: "Batman's Fortress" on Cerberus
Cerberus is a large "dark spot" (an albedo feature) located on Mars and named after the mythical dog Cerberus. The arcuate markings in the upper right are in the Amazonis plains and may be sand drifts. The Elysium volcano, a yellow area north of Cerberus, has several channels radiating from its flanks. The three bright spots, upper left, are volcanoes partially veiled by thin clouds. High resolution images show the bulk of the Cerberus Plains is covered by platy-ridged and inflated lavas, which are interpreted as insulated sheet flows. Eastern Cerberus Plains lavas originate at Cerberus Fossae fissures and shields. Some flows extend for 2000 km through Marte Valles into Amazonis Planitia. Athabasca Valles are both incised into pristine lavas and embayed by pristine lavas, indicating that ... -
Eroded Terrain Near Volcanic Fissures [720p]
This observation was taken to investigate the topography near the source of fluids from the Cerberus Fossae fractures in the Elysium Planitia region of Mars. There are distinct channels carved into the terrain here, presumably by floods of water. However, the terrain is coated with lava, and this situation--where flood-eroded channels are completely coated with lava--is seen in many parts of Mars. This leads some researchers to suggest that the channels were actually carved by the flowing lava, and that there was no flood of water. Images like these are helping to test these ideas. credit: NASA/JPL/University of Arizona source: http://www.uahirise.org/ESP_026303_1945
Cerberus Fossae, Mars
- Order: Reorder
- Duration: 4:18
- Updated: 15 Jan 2014
- views: 143
Mars Reconnaissance Orbiter
Fissure near Cerberus Fossae with Tectonic Morphologies
Looking for Salts on Mars
Recent Volcanism in Valles Marineris
Dunes on ...
Mars Reconnaissance Orbiter
Fissure near Cerberus Fossae with Tectonic Morphologies
Looking for Salts on Mars
Recent Volcanism in Valles Marineris
Dunes on the Rim of the Hellas Impact Basin
wn.com/Cerberus Fossae, Mars
Mars Reconnaissance Orbiter
Fissure near Cerberus Fossae with Tectonic Morphologies
Looking for Salts on Mars
Recent Volcanism in Valles Marineris
Dunes on the Rim of the Hellas Impact Basin
- published: 15 Jan 2014
- views: 143
Mars Geology: The Eastern Portion of Cerberus Fossae
- Order: Reorder
- Duration: 2:18
- Updated: 11 Aug 2015
- views: 39
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysiu...
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. The fossae (Latin plural for a “ditch” or “depression”) are in close proximity and related to the formation of Athabasca Valles, which lies to the west. These rifts are collapse features believed to form by volcanic and tectonic processes. In this composite image (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), we can see that the rift is not continuous, but discontinuous and offset. The offset could be the result of a preexisting subsurface discontinuity, such as a fault.
The close-up view of HiRISE infrared color (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-2.jpg) shows us a plethora of information about Cerberus Fossae and the great amount of detail that HiRISE captures. The clear view of boulders strewn in shadowed areas of the rift is a testament to the high signal-to-noise capability and high resolution of the HiRISE camera; aeolian dunes along with boulders deposited from erosion of the rift walls are also visible in detail.
Using the pixel-length of the shadow within the rift, the incidence angle of the Sun at the time the image was taken, and some trigonometry, the approximate depth of the various sections of Cerberus Fossae can be estimated. Based on this simple method, an approximate depth is 260 meters. This estimate suggests that the rift is as wide as it is deep.
Another remarkable aspect of this image is the stark contrasts it captures: light-toned dusty surfaces that surround the rift versus the dark blue basaltic sands and the shadows within the rift. The detail that HiRISE can provide is indeed phenomenal, and as demonstrated here, the infrared color provides additional information. Why, for instance, is the floor of Cerberus Fossae a deep blue, and why is there such a contrast with the orange-grayish Martian surface? It's not water! The volcanic and mafic sand contains unoxidized iron, which appears a deep blue, while the Martian surface is covered by oxidized iron-bearing dust which appears orange-grayish.
Written by: Kayle Hansen, Livio Tornabene, Eric Pilles, Ryan Hopkins (audio: Tre Gibbs) (7 January 2015)
Related Media
Mars Tectonic Processes:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8mztHqDMYlVtd9UD3CiGJEH
HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument):
http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ
HiRISE, High Resolution Imaging Science Experiment:
"Explore Mars, one giant image at a time."
The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.
HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera.
Credit: NASA/JPL/University of Arizona
wn.com/Mars Geology The Eastern Portion Of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. The fossae (Latin plural for a “ditch” or “depression”) are in close proximity and related to the formation of Athabasca Valles, which lies to the west. These rifts are collapse features believed to form by volcanic and tectonic processes. In this composite image (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), we can see that the rift is not continuous, but discontinuous and offset. The offset could be the result of a preexisting subsurface discontinuity, such as a fault.
The close-up view of HiRISE infrared color (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-2.jpg) shows us a plethora of information about Cerberus Fossae and the great amount of detail that HiRISE captures. The clear view of boulders strewn in shadowed areas of the rift is a testament to the high signal-to-noise capability and high resolution of the HiRISE camera; aeolian dunes along with boulders deposited from erosion of the rift walls are also visible in detail.
Using the pixel-length of the shadow within the rift, the incidence angle of the Sun at the time the image was taken, and some trigonometry, the approximate depth of the various sections of Cerberus Fossae can be estimated. Based on this simple method, an approximate depth is 260 meters. This estimate suggests that the rift is as wide as it is deep.
Another remarkable aspect of this image is the stark contrasts it captures: light-toned dusty surfaces that surround the rift versus the dark blue basaltic sands and the shadows within the rift. The detail that HiRISE can provide is indeed phenomenal, and as demonstrated here, the infrared color provides additional information. Why, for instance, is the floor of Cerberus Fossae a deep blue, and why is there such a contrast with the orange-grayish Martian surface? It's not water! The volcanic and mafic sand contains unoxidized iron, which appears a deep blue, while the Martian surface is covered by oxidized iron-bearing dust which appears orange-grayish.
Written by: Kayle Hansen, Livio Tornabene, Eric Pilles, Ryan Hopkins (audio: Tre Gibbs) (7 January 2015)
Related Media
Mars Tectonic Processes:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8mztHqDMYlVtd9UD3CiGJEH
HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument):
http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ
HiRISE, High Resolution Imaging Science Experiment:
"Explore Mars, one giant image at a time."
The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.
HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera.
Credit: NASA/JPL/University of Arizona
- published: 11 Aug 2015
- views: 39
Mars Geology: Fissure near Cerberus Fossae with Tectonic Morphologies
- Order: Reorder
- Duration: 0:56
- Updated: 15 Jan 2014
- views: 358
The linearity of the volcanic vent shown in this HiRISE image (http://static.uahirise.org/images/2014/details/cut/ESP_034716_1875.jpg), in conjunction with evid...
The linearity of the volcanic vent shown in this HiRISE image (http://static.uahirise.org/images/2014/details/cut/ESP_034716_1875.jpg), in conjunction with evidence of lava flow from the vent, suggests control by combined volcano-tectonic processes. The details of this vent gained by HiRISE should provide insight into those volcano-tectonic processes along Cerberus Fossae fissures in two ways. The nature of both the volcanic products along this fissure, and the geometries of the linear vent, will permit comparison with similar, non-volcanic fissures at Cerberus. And results from these comparisons will provide insight into the orientation of the underlying dike system that may have controlled the ascent of water to the surface in the Cerberus region.
Future topographic analysis with a second image in order to create a 3D picture will enable us to measure the heights of the associated flows and better understand their volcanic history.
Written by: HiRISE Science Team (15 January 2014)
Related Media
Mars Volcanic Processes:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8m4E3fk4bmS3Nus6rtvm0s7
HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument):
http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ
HiRISE, High Resolution Imaging Science Experiment:
"Explore Mars, one giant image at a time."
The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.
HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera.
Credit: NASA/JPL/University of Arizona
wn.com/Mars Geology Fissure Near Cerberus Fossae With Tectonic Morphologies
The linearity of the volcanic vent shown in this HiRISE image (http://static.uahirise.org/images/2014/details/cut/ESP_034716_1875.jpg), in conjunction with evidence of lava flow from the vent, suggests control by combined volcano-tectonic processes. The details of this vent gained by HiRISE should provide insight into those volcano-tectonic processes along Cerberus Fossae fissures in two ways. The nature of both the volcanic products along this fissure, and the geometries of the linear vent, will permit comparison with similar, non-volcanic fissures at Cerberus. And results from these comparisons will provide insight into the orientation of the underlying dike system that may have controlled the ascent of water to the surface in the Cerberus region.
Future topographic analysis with a second image in order to create a 3D picture will enable us to measure the heights of the associated flows and better understand their volcanic history.
Written by: HiRISE Science Team (15 January 2014)
Related Media
Mars Volcanic Processes:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8m4E3fk4bmS3Nus6rtvm0s7
HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument):
http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ
HiRISE, High Resolution Imaging Science Experiment:
"Explore Mars, one giant image at a time."
The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.
HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera.
Credit: NASA/JPL/University of Arizona
- published: 15 Jan 2014
- views: 358
The Eastern Portion of Cerberus Fossae
- Order: Reorder
- Duration: 2:18
- Updated: 07 Jan 2015
- views: 212
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysiu...
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.) http://www.uahirise.org/ESP_039187_1915
wn.com/The Eastern Portion Of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.) http://www.uahirise.org/ESP_039187_1915
- published: 07 Jan 2015
- views: 212
The Cerberus Fossae, Woodford
- Order: Reorder
- Duration: 3:56
- Updated: 15 Aug 2012
- views: 27
- published: 15 Aug 2012
- views: 27
Cerberus Fossae: In the Relay Zone
- Order: Reorder
- Duration: 1:01
- Updated: 18 Feb 2015
- views: 238
These trenches or "fossae" are about a kilometer (0.62 miles) across. This area shows where two segments have joined up and are close to a third section. uahiri...
These trenches or "fossae" are about a kilometer (0.62 miles) across. This area shows where two segments have joined up and are close to a third section. uahirise.org/ESP_039121_1905 (Audio by Tre Gibbs. Enhanced color images are 1 km across.)
wn.com/Cerberus Fossae In The Relay Zone
Geología de Marte: La Parte Oriental de Cerberus Fossae
- Order: Reorder
- Duration: 2:35
- Updated: 04 Oct 2015
- views: 90
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de rifts localizados en Elysium Planitia, justo al norte del ecuad...
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de rifts localizados en Elysium Planitia, justo al norte del ecuador de Marte. Las fossae (el término plural en latín para las palabras “zanja” o “depresión”) están próximas y relacionadas con la formación de Athabasca Valles, que se encuentra al oeste. Estos rifts son formas de colapso que se piensa están formadas por procesos volcánicos y tectónicos. En esta imagen compuesta (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), podemos ver que el rift no es continuo, sino discontinuo y está desplazado. Estos desplazamientos podrían ser el resultado de una discontinuidad presente bajo la superficie, como una falla.
La imagen de cerca de la HiRISE (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-2.jpg) en color infrarrojo nos aporta una gran diversidad de información sobre Cerberus Fossae y una gran cantidad de detalles que es capaz de capturar la HiRISE. La imagen clara de rocas esparcidas en las zonas en sombra del rift es un testamento de la gran capacidad en la relación señal/ruido y la alta resolución de la cámara HiRISE. Las dunas eólicas, junto con las rocas depositadas por la erosión que ocurre en las paredes del rift también son visibles en detalle.
Usando la longitud en píxeles de la sombra dentro del rift, el ángulo de incidencia del Sol a la hora que se hizo la foto y un poco de trigonometría, podemos estimar de una manera aproximada la profundidad de varios segmentos de Cerberus Fossae. Basándonos en este simple método se calcula una profundidad aproximada de 260 metros. Esta estimación sugiere que el rift es tan ancho como profundo.
Otro aspecto destacable de esta imagen son los fuertes contrastes que captura: las superficies polvorientas de tonos claros que rodean el rift contra las arenas basálticas de color oscuro y también las sombras que hay dentro del rift. Los detalles que la HiRISE puede mostrar son ciertamente fenomenales, y como se demuestra aquí, los colores en el infrarrojo nos aportan una información adicional. ¿Por qué, por ejemplo, tiene el fondo de Cerberus Fossae un color azul oscuro, y por qué hay tanto contraste con la superficie de Marte de tonos grises y anaranjados? ¡No es agua! La arena volcánica y máfica contiene hierro sin oxidar, que aparece de un color azul oscuro, mientras que la superficie de Marte está cubierta por polvo que contiene hierro en estado oxidado y que aparece con tonos grises y anaranjados.
(7 de enero de 2015)
Traducción: Nahúm Méndez Chazarra
Geología de Marte: HiRISE Cámara del Orbitador Reconocimiento Marte MRO - Mars Reconnaissance Orbiter:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8mzXnC-vP_IQMKiQvh5_gR3
NASA/Jet Propulsion Laboratory/Universidad de Arizona
Cámara HiRISE (High-Resolution Imaging Science Experiment, Experimento Científico de Imágenes de Alta Resolución) montada a bordo de la nave espacial MRO.
Imágenes desde HiRISE, la cámara de alta resolución a bordo de la sonda MRO. La Mars Reconnaissance Orbiter (acrónimo: MRO) es una nave espacial multipropósito, lanzada el 12 de agosto de 2005 para el avance del conocimiento humano de Marte a través de la observación detallada, con el fin de examinar potenciales zonas de aterrizaje para futuras misiones en la superficie y de realizar transmisiones para éstas. Es el cuarto satélite artificial en Marte (uniéndose a Mars Express, Mars Odyssey y Mars Global Surveyor). El 10 de octubre de 2006 comenzó su inserción en la la órbita marciana, concluyendo su fase de aerofrenado el 4 de septiembre. Sus estudios comienzan tras la conjunción solar de noviembre del mismo año.
La High Resolution Imaging Science Experiment es una cámara situada a bordo del Mars Reconnaissance Orbiter. Con un peso de 65 kg, este instrumento de 40 millones de dólares fue construido por Ball Aerospace & Technologies Corp bajo la dirección del departamento lunar y planetario de la Universidad de Arizona. Consiste en un Telescopio reflector de 0,5 metros de diámetro, el más grande de cualquier misión interplanetaria. Permite fotografiar con una resolución por encima de los 0,3 metros, diferenciando objetos de 1 metro de diámetro (aproximadamente una bola de playa).
Gracias a las fotos de alta resolución se han descubierto nuevos detalles de la geología marciana, los cuales dieron como resultado el descubrimiento de terreno que indicaba la presencia dióxido de carbono líquido o agua en la superficie en su pasado geológico reciente.
En agosto de 2015 la MRO cumplió diez años desde su lanzamiento, siguiendo la observación de Marte desde una órbita en torno a él y enviando a la Tierra información sobre el Planeta Rojo.
wn.com/Geología De Marte La Parte Oriental De Cerberus Fossae
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de rifts localizados en Elysium Planitia, justo al norte del ecuador de Marte. Las fossae (el término plural en latín para las palabras “zanja” o “depresión”) están próximas y relacionadas con la formación de Athabasca Valles, que se encuentra al oeste. Estos rifts son formas de colapso que se piensa están formadas por procesos volcánicos y tectónicos. En esta imagen compuesta (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-1.jpg), podemos ver que el rift no es continuo, sino discontinuo y está desplazado. Estos desplazamientos podrían ser el resultado de una discontinuidad presente bajo la superficie, como una falla.
La imagen de cerca de la HiRISE (http://static.uahirise.org/images/2015/details/cut/ESP_039187_1915-2.jpg) en color infrarrojo nos aporta una gran diversidad de información sobre Cerberus Fossae y una gran cantidad de detalles que es capaz de capturar la HiRISE. La imagen clara de rocas esparcidas en las zonas en sombra del rift es un testamento de la gran capacidad en la relación señal/ruido y la alta resolución de la cámara HiRISE. Las dunas eólicas, junto con las rocas depositadas por la erosión que ocurre en las paredes del rift también son visibles en detalle.
Usando la longitud en píxeles de la sombra dentro del rift, el ángulo de incidencia del Sol a la hora que se hizo la foto y un poco de trigonometría, podemos estimar de una manera aproximada la profundidad de varios segmentos de Cerberus Fossae. Basándonos en este simple método se calcula una profundidad aproximada de 260 metros. Esta estimación sugiere que el rift es tan ancho como profundo.
Otro aspecto destacable de esta imagen son los fuertes contrastes que captura: las superficies polvorientas de tonos claros que rodean el rift contra las arenas basálticas de color oscuro y también las sombras que hay dentro del rift. Los detalles que la HiRISE puede mostrar son ciertamente fenomenales, y como se demuestra aquí, los colores en el infrarrojo nos aportan una información adicional. ¿Por qué, por ejemplo, tiene el fondo de Cerberus Fossae un color azul oscuro, y por qué hay tanto contraste con la superficie de Marte de tonos grises y anaranjados? ¡No es agua! La arena volcánica y máfica contiene hierro sin oxidar, que aparece de un color azul oscuro, mientras que la superficie de Marte está cubierta por polvo que contiene hierro en estado oxidado y que aparece con tonos grises y anaranjados.
(7 de enero de 2015)
Traducción: Nahúm Méndez Chazarra
Geología de Marte: HiRISE Cámara del Orbitador Reconocimiento Marte MRO - Mars Reconnaissance Orbiter:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8mzXnC-vP_IQMKiQvh5_gR3
NASA/Jet Propulsion Laboratory/Universidad de Arizona
Cámara HiRISE (High-Resolution Imaging Science Experiment, Experimento Científico de Imágenes de Alta Resolución) montada a bordo de la nave espacial MRO.
Imágenes desde HiRISE, la cámara de alta resolución a bordo de la sonda MRO. La Mars Reconnaissance Orbiter (acrónimo: MRO) es una nave espacial multipropósito, lanzada el 12 de agosto de 2005 para el avance del conocimiento humano de Marte a través de la observación detallada, con el fin de examinar potenciales zonas de aterrizaje para futuras misiones en la superficie y de realizar transmisiones para éstas. Es el cuarto satélite artificial en Marte (uniéndose a Mars Express, Mars Odyssey y Mars Global Surveyor). El 10 de octubre de 2006 comenzó su inserción en la la órbita marciana, concluyendo su fase de aerofrenado el 4 de septiembre. Sus estudios comienzan tras la conjunción solar de noviembre del mismo año.
La High Resolution Imaging Science Experiment es una cámara situada a bordo del Mars Reconnaissance Orbiter. Con un peso de 65 kg, este instrumento de 40 millones de dólares fue construido por Ball Aerospace & Technologies Corp bajo la dirección del departamento lunar y planetario de la Universidad de Arizona. Consiste en un Telescopio reflector de 0,5 metros de diámetro, el más grande de cualquier misión interplanetaria. Permite fotografiar con una resolución por encima de los 0,3 metros, diferenciando objetos de 1 metro de diámetro (aproximadamente una bola de playa).
Gracias a las fotos de alta resolución se han descubierto nuevos detalles de la geología marciana, los cuales dieron como resultado el descubrimiento de terreno que indicaba la presencia dióxido de carbono líquido o agua en la superficie en su pasado geológico reciente.
En agosto de 2015 la MRO cumplió diez años desde su lanzamiento, siguiendo la observación de Marte desde una órbita en torno a él y enviando a la Tierra información sobre el Planeta Rojo.
- published: 04 Oct 2015
- views: 90
Mars Geology: Small Floral-Shaped Volcano on Cerberus Fossae
- Order: Reorder
- Duration: 0:44
- Updated: 09 Aug 2015
- views: 19
This is a small volcano superposed on the flanks of a larger one of the Cerberus Tholi. This smaller feature has a single vent (http://static.uahirise.org/image...
This is a small volcano superposed on the flanks of a larger one of the Cerberus Tholi. This smaller feature has a single vent (http://static.uahirise.org/images/2012/details/cut/ESP_024378_1880.jpg), aligned along a Cerberus Fossae trough, and it has flows radiating away from this vent in all directions, somewhat looking like a flower. These flows appear somewhat darker than their surroundings, though this might be owing to roughness as much as to relative youth. Note that even at Context Camera (CTX) scale, we can see that there are some small impact craters superimposed on this feature, indicating that it is not entirely young.
This caption is based on the original science rationale.
Written by: HiRISE Science Team (4 January 2012)
Related Media
Mars Volcanic Processes:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8m4E3fk4bmS3Nus6rtvm0s7
HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument):
http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ
HiRISE, High Resolution Imaging Science Experiment:
"Explore Mars, one giant image at a time."
The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.
HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera.
Credit: NASA/JPL/University of Arizona
wn.com/Mars Geology Small Floral Shaped Volcano On Cerberus Fossae
This is a small volcano superposed on the flanks of a larger one of the Cerberus Tholi. This smaller feature has a single vent (http://static.uahirise.org/images/2012/details/cut/ESP_024378_1880.jpg), aligned along a Cerberus Fossae trough, and it has flows radiating away from this vent in all directions, somewhat looking like a flower. These flows appear somewhat darker than their surroundings, though this might be owing to roughness as much as to relative youth. Note that even at Context Camera (CTX) scale, we can see that there are some small impact craters superimposed on this feature, indicating that it is not entirely young.
This caption is based on the original science rationale.
Written by: HiRISE Science Team (4 January 2012)
Related Media
Mars Volcanic Processes:
https://www.youtube.com/playlist?list=PL6vzpF_OEV8m4E3fk4bmS3Nus6rtvm0s7
HiRISE, High Resolution Imaging Science Experiment (Mars Reconnaissance Orbiter Instrument):
http://www.youtube.com/playlist?list=PL6vzpF_OEV8nfAL7zVkUWJpw-_9jkJjtZ
HiRISE, High Resolution Imaging Science Experiment:
"Explore Mars, one giant image at a time."
The Mars Reconnaissance Orbiter Project is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.
HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Malin Space Science Systems, San Diego, built and operates the Context Camera.
Credit: NASA/JPL/University of Arizona
- published: 09 Aug 2015
- views: 19
Mars: The Eastern Portion of Cerberus Fossae
- Order: Reorder
- Duration: 2:18
- Updated: 09 Jan 2015
- views: 15
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysiu...
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.)
http://www.uahirise.org/ESP_039187_1915
Credit: NASA/JPL/University of Arizona
wn.com/Mars The Eastern Portion Of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meters), which are comprised of a series of rifts present located in Elysium Planitia just north the Martian equator. (Audio by Tre Gibbs. Enhanced color images are 1 km across.)
http://www.uahirise.org/ESP_039187_1915
Credit: NASA/JPL/University of Arizona
- published: 09 Jan 2015
- views: 15
La parte oriental de Cerberus Fossae
- Order: Reorder
- Duration: 2:35
- Updated: 04 Feb 2015
- views: 12
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de "rifts" localizados en Elysium Planitia, justo al norte del ecu...
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de "rifts" localizados en Elysium Planitia, justo al norte del ecuador de Marte. http://www.uahirise.org/es/ESP_039187_1915
wn.com/La Parte Oriental De Cerberus Fossae
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conjunto de "rifts" localizados en Elysium Planitia, justo al norte del ecuador de Marte. http://www.uahirise.org/es/ESP_039187_1915
- published: 04 Feb 2015
- views: 12
Mars News: "Batman's Fortress" on Cerberus
- Order: Reorder
- Duration: 0:40
- Updated: 14 Feb 2015
- views: 469
Cerberus is a large "dark spot" (an albedo feature) located on Mars and named after the mythical dog Cerberus. The arcuate markings in the upper right are in th...
Cerberus is a large "dark spot" (an albedo feature) located on Mars and named after the mythical dog Cerberus. The arcuate markings in the upper right are in the Amazonis plains and may be sand drifts. The Elysium volcano, a yellow area north of Cerberus, has several channels radiating from its flanks. The three bright spots, upper left, are volcanoes partially veiled by thin clouds.
High resolution images show the bulk of the Cerberus Plains is covered by platy-ridged and inflated lavas, which are interpreted as insulated sheet flows. Eastern Cerberus Plains lavas originate at Cerberus Fossae fissures and shields. Some flows extend for 2000 km through Marte Valles into Amazonis Planitia. Athabasca Valles are both incised into pristine lavas and embayed by pristine lavas, indicating that Athabascan fluvial events were contemporaneous with volcanic eruptions. Deposits of the Medusae Fossae Formation lie both over and under lavas, suggesting the deposition of the Medusae Fossae Formation was contemporaneous with volcanism. Statistics of small craters indicate lavas in the Western Cerberus Plains may be less than a million years old, but the model isochrons may be unreliable if the small crater population is dominated by secondary craters. Images showing no large craters with diameters 500 m superimposed on Western Cerberus Plains lavas indicate the same surface is younger than 49 Ma.
"Batman's Fortress" on Cerberus, Mars
These are my own observations. In future I'll upload more and more interesting things seen in NASA's images, so please subscribe!
I will also add the coordinates soon; until then please try to have some fun finding them for yourself, surely you will find more interesting stuff!
Join our facebook group: https://www.facebook.com/groups/marsancientnews/?fref=ts
All thanks go to NASA/JPL/Malin Space Science Systems. and European Space Agency for providing the images used in this video.
http://www.nasa.gov/
http://www.jpl.nasa.gov/
http://www.msss.com/
http://www.esa.int
Bibliography: http://en.wikipedia.org
wn.com/Mars News Batman's Fortress On Cerberus
Cerberus is a large "dark spot" (an albedo feature) located on Mars and named after the mythical dog Cerberus. The arcuate markings in the upper right are in the Amazonis plains and may be sand drifts. The Elysium volcano, a yellow area north of Cerberus, has several channels radiating from its flanks. The three bright spots, upper left, are volcanoes partially veiled by thin clouds.
High resolution images show the bulk of the Cerberus Plains is covered by platy-ridged and inflated lavas, which are interpreted as insulated sheet flows. Eastern Cerberus Plains lavas originate at Cerberus Fossae fissures and shields. Some flows extend for 2000 km through Marte Valles into Amazonis Planitia. Athabasca Valles are both incised into pristine lavas and embayed by pristine lavas, indicating that Athabascan fluvial events were contemporaneous with volcanic eruptions. Deposits of the Medusae Fossae Formation lie both over and under lavas, suggesting the deposition of the Medusae Fossae Formation was contemporaneous with volcanism. Statistics of small craters indicate lavas in the Western Cerberus Plains may be less than a million years old, but the model isochrons may be unreliable if the small crater population is dominated by secondary craters. Images showing no large craters with diameters 500 m superimposed on Western Cerberus Plains lavas indicate the same surface is younger than 49 Ma.
"Batman's Fortress" on Cerberus, Mars
These are my own observations. In future I'll upload more and more interesting things seen in NASA's images, so please subscribe!
I will also add the coordinates soon; until then please try to have some fun finding them for yourself, surely you will find more interesting stuff!
Join our facebook group: https://www.facebook.com/groups/marsancientnews/?fref=ts
All thanks go to NASA/JPL/Malin Space Science Systems. and European Space Agency for providing the images used in this video.
http://www.nasa.gov/
http://www.jpl.nasa.gov/
http://www.msss.com/
http://www.esa.int
Bibliography: http://en.wikipedia.org
- published: 14 Feb 2015
- views: 469
Eroded Terrain Near Volcanic Fissures [720p]
- Order: Reorder
- Duration: 0:40
- Updated: 12 Apr 2012
- views: 1479
This observation was taken to investigate the topography near the source of fluids from the Cerberus Fossae fractures in the Elysium Planitia region of Mars.
...
This observation was taken to investigate the topography near the source of fluids from the Cerberus Fossae fractures in the Elysium Planitia region of Mars.
There are distinct channels carved into the terrain here, presumably by floods of water. However, the terrain is coated with lava, and this situation--where flood-eroded channels are completely coated with lava--is seen in many parts of Mars.
This leads some researchers to suggest that the channels were actually carved by the flowing lava, and that there was no flood of water. Images like these are helping to test these ideas.
credit: NASA/JPL/University of Arizona
source: http://www.uahirise.org/ESP_026303_1945
wn.com/Eroded Terrain Near Volcanic Fissures 720P
This observation was taken to investigate the topography near the source of fluids from the Cerberus Fossae fractures in the Elysium Planitia region of Mars.
There are distinct channels carved into the terrain here, presumably by floods of water. However, the terrain is coated with lava, and this situation--where flood-eroded channels are completely coated with lava--is seen in many parts of Mars.
This leads some researchers to suggest that the channels were actually carved by the flowing lava, and that there was no flood of water. Images like these are helping to test these ideas.
credit: NASA/JPL/University of Arizona
source: http://www.uahirise.org/ESP_026303_1945
- published: 12 Apr 2012
- views: 1479
-
Cerberus Fossae, Mars
Mars Reconnaissance Orbiter The Eastern Portion of Cerberus Fossae A Recent Impact in Elysium Planitia A Polar Smile Strange Flow Landslide, Impact Melt or Lava -
Marte: Paseo turístico por lo desconocido / Travel guide to Mars [IGEO.TV]
Colabora con nosotros: http://igeo.tv/contribuye-al-proyecto/ Vamos a dar una vuelta por Marte y ver uno de los mejores destinos turísticos virtuales posibles Aunque a simple vista no lo parezca, Marte es un planeta dinámico, sus campos de dunas son mecidos por el viento marciano Y sus casquetes polares cambian con las estaciones del año (mucho más largas que en nuestro planeta, puesto que un año en marte son 687 días terrestres) Son varios los siglos que el hombre lleva estudiando el planeta marte. Y Los científicos creen que en un futuro próximo existirán guías turísticas de Marte en muchos de nuestros hogares, pero hasta entonces... ¿cuáles son los principales atractivos del planeta rojo? Lo averiguaremos en esta "ruta turística por marte" Nuestro primer destino es el imponente M... -
Plan your next holiday to Mars (1)
Plan your next holiday to Mars - part 1 PIA17928: Shapes and Spots on a Polar Sand Dune http://photojournal.jpl.nasa.gov/catalog/PIA17928 PIA17981: Dunes Flying in Formation http://photojournal.jpl.nasa.gov/catalog/PIA17981 PIA17986: Fall Frost Accumulation on Russell Crater Dunes http://photojournal.jpl.nasa.gov/catalog/PIA17986 PIA18244: The Active Dunes of Nili Patera http://photojournal.jpl.nasa.gov/catalog/PIA18244 PIA18512: Touring a Dusty Region http://photojournal.jpl.nasa.gov/catalog/PIA18512 PIA18586: Blockfall on the North Polar Layered Deposits http://photojournal.jpl.nasa.gov/catalog/PIA18586 PIA18632: Water-Bearing Rocks in Noctis Labyrinthus http://photojournal.jpl.nasa.gov/catalog/PIA18632 PIA18634: Frosty Gullies http://photojournal.jpl.nasa.gov/catalog/PI... -
Plan your next holiday to Mars (2)
Plan your next holiday to Mars - part 2 PIA12956: Cerberus Fossae East of the Head of Athabasca Valles PIA13076: Proctor Crater Dune Field PIA17573: Colorful Dunes PIA17628: Two Generations of Windblown Sediments PIA17629: Martian Glaciers and Brain Terrain PIA17630: Layers, Bedrock Ridges, and Dark Sand in Schiaparelli Crater PIA17633: Utopia Planitia's Surface PIA17638: Bright Dunes in Syria Planum PIA17640: Lava Against an Impact Crater in Elysium Planitia PIA17641: Frosted Impact Crater in Late Northern Winter PIA17643: Basin in the West Candor Chasma Layered Deposits PIA17699: Colorful Sediments near Hellas Basin PIA17857: Rippled Surfaces on a Slope in Coloe Fossae PIA17875: Looking for Salts on Mars PIA17878: Bright Tracks from Bouncing and Rolling Boulders PIA17910:... -
Cerberus Fossae, Mars
- Order: Reorder
- Duration: 4:28
- Updated: 11 Jan 2015
- views: 64
Mars Reconnaissance Orbiter
The Eastern Portion of Cerberus Fossae
A Recent Impact in Elysium Planitia
A Polar Smile
Strange Flow Landslide, Impact Melt or Lav...
Mars Reconnaissance Orbiter
The Eastern Portion of Cerberus Fossae
A Recent Impact in Elysium Planitia
A Polar Smile
Strange Flow Landslide, Impact Melt or Lava
wn.com/Cerberus Fossae, Mars
Mars Reconnaissance Orbiter
The Eastern Portion of Cerberus Fossae
A Recent Impact in Elysium Planitia
A Polar Smile
Strange Flow Landslide, Impact Melt or Lava
- published: 11 Jan 2015
- views: 64
Marte: Paseo turístico por lo desconocido / Travel guide to Mars [IGEO.TV]
- Order: Reorder
- Duration: 4:11
- Updated: 16 May 2014
- views: 3443
Colabora con nosotros: http://igeo.tv/contribuye-al-proyecto/
Vamos a dar una vuelta por Marte y ver uno de los mejores destinos turísticos virtuales posibles ...
Colabora con nosotros: http://igeo.tv/contribuye-al-proyecto/
Vamos a dar una vuelta por Marte y ver uno de los mejores destinos turísticos virtuales posibles Aunque a simple vista no lo parezca, Marte es un planeta dinámico, sus campos de dunas son mecidos por el viento marciano
Y sus casquetes polares cambian con las estaciones del año (mucho más largas que en nuestro planeta, puesto que un año en marte son 687 días terrestres)
Son varios los siglos que el hombre lleva estudiando el planeta marte.
Y Los científicos creen que en un futuro próximo existirán guías turísticas de Marte en muchos de nuestros hogares, pero hasta entonces... ¿cuáles son los principales atractivos del planeta rojo?
Lo averiguaremos en esta "ruta turística por marte"
Nuestro primer destino es el imponente Monte olimpo: el volcán más grande del sistema solar. Tres veces más alto que el Everest y con una extensión similar a la de gran Bretaña. Este monte se encuentra situado en la altiplanicie volcánica denominada Tharsis (de 10 km de altitud) y tan extensa como europa.
La siguiente parada de nuestra ruta es: Valles marineris: un cañon que comparado con el del colorado se antoja descomunal. Sus dimensiones son de 4.500 km de longitud, 200 km de anchura y 11 km de profundidad máxima.
Seguimos nuestra visita por "Cerberus fossae" Una serie de fisuras situadas cerca del ecuador y formadas por fallas que separan la corteza.
Y aprovechamos para pasar por "Marte Vallis" que se encuentra en las llanuras de elysium planita y es un valle de 185 km de longitud.
La conocida como "ciudad Inca": es uno de los grandes misterios de marte resuelto hace muy poco. Esta división de espacio propio de los asentamientos inca resulto ser una parte aislada de una estructura circular mayor de unos 86 km de diámetro. Fruto de un fuerte impacto contra el planeta.
El Crater Hellas Planitia: Con un díametro de unos 2.300 km es el cráter de impacto más grande de la superficie de marte.
Si nos dirigimos a las inmediaciones del polo norte encontraremos campos de dunas majestuosos: ya que la mayor extensión circunda los campos de hielo del polo norte. Estas son Las extensiónes de dunas más grandes de todo el sistema solar.
Por último nos dirigimos hacía el polo sur del planeta, dónde recientemente se han descubierto la presencia de geisers de arena, un espectáculo más que fascinante...
The Martian wind sways the dunes of Mars. And its polar caps change with the seasons. Which are the main attractions of the Red Planet?
We'll find out in this travel Guide to Mars. the largest volcano in the solar system. A huge canyon.
Igeo TV in english: watch this video, agency news and footage: http://www.youtube.com/channel/UCZR81PO2OtnJsB3V1pD3WrQ
wn.com/Marte Paseo Turístico Por Lo Desconocido Travel Guide To Mars Igeo.Tv
Colabora con nosotros: http://igeo.tv/contribuye-al-proyecto/
Vamos a dar una vuelta por Marte y ver uno de los mejores destinos turísticos virtuales posibles Aunque a simple vista no lo parezca, Marte es un planeta dinámico, sus campos de dunas son mecidos por el viento marciano
Y sus casquetes polares cambian con las estaciones del año (mucho más largas que en nuestro planeta, puesto que un año en marte son 687 días terrestres)
Son varios los siglos que el hombre lleva estudiando el planeta marte.
Y Los científicos creen que en un futuro próximo existirán guías turísticas de Marte en muchos de nuestros hogares, pero hasta entonces... ¿cuáles son los principales atractivos del planeta rojo?
Lo averiguaremos en esta "ruta turística por marte"
Nuestro primer destino es el imponente Monte olimpo: el volcán más grande del sistema solar. Tres veces más alto que el Everest y con una extensión similar a la de gran Bretaña. Este monte se encuentra situado en la altiplanicie volcánica denominada Tharsis (de 10 km de altitud) y tan extensa como europa.
La siguiente parada de nuestra ruta es: Valles marineris: un cañon que comparado con el del colorado se antoja descomunal. Sus dimensiones son de 4.500 km de longitud, 200 km de anchura y 11 km de profundidad máxima.
Seguimos nuestra visita por "Cerberus fossae" Una serie de fisuras situadas cerca del ecuador y formadas por fallas que separan la corteza.
Y aprovechamos para pasar por "Marte Vallis" que se encuentra en las llanuras de elysium planita y es un valle de 185 km de longitud.
La conocida como "ciudad Inca": es uno de los grandes misterios de marte resuelto hace muy poco. Esta división de espacio propio de los asentamientos inca resulto ser una parte aislada de una estructura circular mayor de unos 86 km de diámetro. Fruto de un fuerte impacto contra el planeta.
El Crater Hellas Planitia: Con un díametro de unos 2.300 km es el cráter de impacto más grande de la superficie de marte.
Si nos dirigimos a las inmediaciones del polo norte encontraremos campos de dunas majestuosos: ya que la mayor extensión circunda los campos de hielo del polo norte. Estas son Las extensiónes de dunas más grandes de todo el sistema solar.
Por último nos dirigimos hacía el polo sur del planeta, dónde recientemente se han descubierto la presencia de geisers de arena, un espectáculo más que fascinante...
The Martian wind sways the dunes of Mars. And its polar caps change with the seasons. Which are the main attractions of the Red Planet?
We'll find out in this travel Guide to Mars. the largest volcano in the solar system. A huge canyon.
Igeo TV in english: watch this video, agency news and footage: http://www.youtube.com/channel/UCZR81PO2OtnJsB3V1pD3WrQ
- published: 16 May 2014
- views: 3443
Plan your next holiday to Mars (1)
- Order: Reorder
- Duration: 4:22
- Updated: 22 Feb 2015
- views: 206
Plan your next holiday to Mars - part 1
PIA17928: Shapes and Spots on a Polar Sand Dune
http://photojournal.jpl.nasa.gov/catalog/PIA17928
PIA17981: Dunes Fl...
Plan your next holiday to Mars - part 1
PIA17928: Shapes and Spots on a Polar Sand Dune
http://photojournal.jpl.nasa.gov/catalog/PIA17928
PIA17981: Dunes Flying in Formation
http://photojournal.jpl.nasa.gov/catalog/PIA17981
PIA17986: Fall Frost Accumulation on Russell Crater Dunes
http://photojournal.jpl.nasa.gov/catalog/PIA17986
PIA18244: The Active Dunes of Nili Patera
http://photojournal.jpl.nasa.gov/catalog/PIA18244
PIA18512: Touring a Dusty Region
http://photojournal.jpl.nasa.gov/catalog/PIA18512
PIA18586: Blockfall on the North Polar Layered Deposits
http://photojournal.jpl.nasa.gov/catalog/PIA18586
PIA18632: Water-Bearing Rocks in Noctis Labyrinthus
http://photojournal.jpl.nasa.gov/catalog/PIA18632
PIA18634: Frosty Gullies
http://photojournal.jpl.nasa.gov/catalog/PIA18634
PIA18646: The Side of Chasma Boreale
http://photojournal.jpl.nasa.gov/catalog/PIA18646
PIA18771: At the Edge of a Polar Cap
http://photojournal.jpl.nasa.gov/catalog/PIA18771
PIA18806: Banded TARs in Iapygia
http://photojournal.jpl.nasa.gov/catalog/PIA18806
PIA18818: Continual Dune and Ripple Migration in Nili Patera
http://photojournal.jpl.nasa.gov/catalog/PIA18818
PIA18819: Bright Slope Streaks in Arabia Terra
http://photojournal.jpl.nasa.gov/catalog/PIA18819
PIA18820: Dome and Barchan Dunes in Newton Crater
http://photojournal.jpl.nasa.gov/catalog/PIA18820
PIA18832: Perennial Frost in a Crater on the Northern Plains
http://photojournal.jpl.nasa.gov/catalog/PIA18832
PIA19116: Seeing Beneath the Surface in Morava Valles
http://photojournal.jpl.nasa.gov/catalog/PIA19116
PIA19117: Frosted Gullies in a Central Pit
http://photojournal.jpl.nasa.gov/catalog/PIA19117
PIA19118: Recurring Slope Lineae in Juventae Chasma
http://photojournal.jpl.nasa.gov/catalog/PIA19118
PIA19120: Polar Layered Deposit Slopes
http://photojournal.jpl.nasa.gov/catalog/PIA19120
PIA19122: Frosty Slopes in Late Spring
http://photojournal.jpl.nasa.gov/catalog/PIA19122
PIA19139: Crater Slopes: The Power of a Repeat Image
http://photojournal.jpl.nasa.gov/catalog/PIA19139
PIA19289: Pits in Hale Crater Ejecta
http://photojournal.jpl.nasa.gov/catalog/PIA19289
PIA19291: Yardangs in Arsinoes Chaos, Mars
http://photojournal.jpl.nasa.gov/catalog/PIA19291
PIA19292: Icy Wonderland
http://photojournal.jpl.nasa.gov/catalog/PIA19292
PIA19294: Gullies and Bedrock in Nirgal Vallis
http://photojournal.jpl.nasa.gov/catalog/PIA19294
PIA17636: Polygonal Surface Patterns at the South Pole
http://photojournal.jpl.nasa.gov/catalog/PIA17636
PIA17723: Mawrth Vallis Geodiversity
http://photojournal.jpl.nasa.gov/catalog/PIA17723
PIA17876: Fissure near Cerberus Fossae with Tectonic Morphologies
http://photojournal.jpl.nasa.gov/catalog/PIA17876
PIA17879: Raindrops of Sand in Copernicus Crater
http://photojournal.jpl.nasa.gov/catalog/PIA17879
PIA17919: Two-Color Dunes in Meridiani Terra
http://photojournal.jpl.nasa.gov/catalog/PIA17919
All thanks go to NASA/JPL/Malin Space Science Systems. for providing the images used in this video.
http://www.nasa.gov/
http://www.jpl.nasa.gov/
http://www.msss.com/
wn.com/Plan Your Next Holiday To Mars (1)
Plan your next holiday to Mars - part 1
PIA17928: Shapes and Spots on a Polar Sand Dune
http://photojournal.jpl.nasa.gov/catalog/PIA17928
PIA17981: Dunes Flying in Formation
http://photojournal.jpl.nasa.gov/catalog/PIA17981
PIA17986: Fall Frost Accumulation on Russell Crater Dunes
http://photojournal.jpl.nasa.gov/catalog/PIA17986
PIA18244: The Active Dunes of Nili Patera
http://photojournal.jpl.nasa.gov/catalog/PIA18244
PIA18512: Touring a Dusty Region
http://photojournal.jpl.nasa.gov/catalog/PIA18512
PIA18586: Blockfall on the North Polar Layered Deposits
http://photojournal.jpl.nasa.gov/catalog/PIA18586
PIA18632: Water-Bearing Rocks in Noctis Labyrinthus
http://photojournal.jpl.nasa.gov/catalog/PIA18632
PIA18634: Frosty Gullies
http://photojournal.jpl.nasa.gov/catalog/PIA18634
PIA18646: The Side of Chasma Boreale
http://photojournal.jpl.nasa.gov/catalog/PIA18646
PIA18771: At the Edge of a Polar Cap
http://photojournal.jpl.nasa.gov/catalog/PIA18771
PIA18806: Banded TARs in Iapygia
http://photojournal.jpl.nasa.gov/catalog/PIA18806
PIA18818: Continual Dune and Ripple Migration in Nili Patera
http://photojournal.jpl.nasa.gov/catalog/PIA18818
PIA18819: Bright Slope Streaks in Arabia Terra
http://photojournal.jpl.nasa.gov/catalog/PIA18819
PIA18820: Dome and Barchan Dunes in Newton Crater
http://photojournal.jpl.nasa.gov/catalog/PIA18820
PIA18832: Perennial Frost in a Crater on the Northern Plains
http://photojournal.jpl.nasa.gov/catalog/PIA18832
PIA19116: Seeing Beneath the Surface in Morava Valles
http://photojournal.jpl.nasa.gov/catalog/PIA19116
PIA19117: Frosted Gullies in a Central Pit
http://photojournal.jpl.nasa.gov/catalog/PIA19117
PIA19118: Recurring Slope Lineae in Juventae Chasma
http://photojournal.jpl.nasa.gov/catalog/PIA19118
PIA19120: Polar Layered Deposit Slopes
http://photojournal.jpl.nasa.gov/catalog/PIA19120
PIA19122: Frosty Slopes in Late Spring
http://photojournal.jpl.nasa.gov/catalog/PIA19122
PIA19139: Crater Slopes: The Power of a Repeat Image
http://photojournal.jpl.nasa.gov/catalog/PIA19139
PIA19289: Pits in Hale Crater Ejecta
http://photojournal.jpl.nasa.gov/catalog/PIA19289
PIA19291: Yardangs in Arsinoes Chaos, Mars
http://photojournal.jpl.nasa.gov/catalog/PIA19291
PIA19292: Icy Wonderland
http://photojournal.jpl.nasa.gov/catalog/PIA19292
PIA19294: Gullies and Bedrock in Nirgal Vallis
http://photojournal.jpl.nasa.gov/catalog/PIA19294
PIA17636: Polygonal Surface Patterns at the South Pole
http://photojournal.jpl.nasa.gov/catalog/PIA17636
PIA17723: Mawrth Vallis Geodiversity
http://photojournal.jpl.nasa.gov/catalog/PIA17723
PIA17876: Fissure near Cerberus Fossae with Tectonic Morphologies
http://photojournal.jpl.nasa.gov/catalog/PIA17876
PIA17879: Raindrops of Sand in Copernicus Crater
http://photojournal.jpl.nasa.gov/catalog/PIA17879
PIA17919: Two-Color Dunes in Meridiani Terra
http://photojournal.jpl.nasa.gov/catalog/PIA17919
All thanks go to NASA/JPL/Malin Space Science Systems. for providing the images used in this video.
http://www.nasa.gov/
http://www.jpl.nasa.gov/
http://www.msss.com/
- published: 22 Feb 2015
- views: 206
Plan your next holiday to Mars (2)
- Order: Reorder
- Duration: 4:22
- Updated: 25 Mar 2015
- views: 101
Plan your next holiday to Mars - part 2
PIA12956: Cerberus Fossae East of the Head of Athabasca Valles
PIA13076: Proctor Crater Dune Field
PIA17573: Colorful ...
Plan your next holiday to Mars - part 2
PIA12956: Cerberus Fossae East of the Head of Athabasca Valles
PIA13076: Proctor Crater Dune Field
PIA17573: Colorful Dunes
PIA17628: Two Generations of Windblown Sediments
PIA17629: Martian Glaciers and Brain Terrain
PIA17630: Layers, Bedrock Ridges, and Dark Sand in Schiaparelli Crater
PIA17633: Utopia Planitia's Surface
PIA17638: Bright Dunes in Syria Planum
PIA17640: Lava Against an Impact Crater in Elysium Planitia
PIA17641: Frosted Impact Crater in Late Northern Winter
PIA17643: Basin in the West Candor Chasma Layered Deposits
PIA17699: Colorful Sediments near Hellas Basin
PIA17857: Rippled Surfaces on a Slope in Coloe Fossae
PIA17875: Looking for Salts on Mars
PIA17878: Bright Tracks from Bouncing and Rolling Boulders
PIA17910: An Unusual Mound
PIA17980: Bright Sediments on the Floor of Ladon Basin
PIA17984: Squiggly Sand Dunes
PIA17985: Channels in Phlegra Montes
PIA18225: Equatorial Gullies on Mars
PIA18241: Yardangs Forming Near Gordii Dorsum
PIA18242: Sunken and Pitted Ejecta
PIA18635: Layers and Sand on the Floor of Schiaparelli Crater
PIA18645: Strange Cones and Flows
PIA18648: What Gullies Can Say
PIA18774: Weird Crater
PIA18829: Perennial Frost in a Crater on the Northern Plains
PIA18930: Braided TARs in Syrtis Major
PIA19293: A Large, Longitudinal Dune
PIA19295: Boulders in Gully Alcoves
All thanks go to NASA/JPL/Malin Space Science Systems. for providing the images used in this video.
http://www.nasa.gov/
http://www.jpl.nasa.gov/
http://www.msss.com/
wn.com/Plan Your Next Holiday To Mars (2)
Plan your next holiday to Mars - part 2
PIA12956: Cerberus Fossae East of the Head of Athabasca Valles
PIA13076: Proctor Crater Dune Field
PIA17573: Colorful Dunes
PIA17628: Two Generations of Windblown Sediments
PIA17629: Martian Glaciers and Brain Terrain
PIA17630: Layers, Bedrock Ridges, and Dark Sand in Schiaparelli Crater
PIA17633: Utopia Planitia's Surface
PIA17638: Bright Dunes in Syria Planum
PIA17640: Lava Against an Impact Crater in Elysium Planitia
PIA17641: Frosted Impact Crater in Late Northern Winter
PIA17643: Basin in the West Candor Chasma Layered Deposits
PIA17699: Colorful Sediments near Hellas Basin
PIA17857: Rippled Surfaces on a Slope in Coloe Fossae
PIA17875: Looking for Salts on Mars
PIA17878: Bright Tracks from Bouncing and Rolling Boulders
PIA17910: An Unusual Mound
PIA17980: Bright Sediments on the Floor of Ladon Basin
PIA17984: Squiggly Sand Dunes
PIA17985: Channels in Phlegra Montes
PIA18225: Equatorial Gullies on Mars
PIA18241: Yardangs Forming Near Gordii Dorsum
PIA18242: Sunken and Pitted Ejecta
PIA18635: Layers and Sand on the Floor of Schiaparelli Crater
PIA18645: Strange Cones and Flows
PIA18648: What Gullies Can Say
PIA18774: Weird Crater
PIA18829: Perennial Frost in a Crater on the Northern Plains
PIA18930: Braided TARs in Syrtis Major
PIA19293: A Large, Longitudinal Dune
PIA19295: Boulders in Gully Alcoves
All thanks go to NASA/JPL/Malin Space Science Systems. for providing the images used in this video.
http://www.nasa.gov/
http://www.jpl.nasa.gov/
http://www.msss.com/
- published: 25 Mar 2015
- views: 101
Surfing Black Mt. volcano in Tucson AZ
- Order: Reorder
- Duration: 1:57
- Updated: 08 Oct 2013
- views: 567
Windy day on Ms. Black Volcano
Windy day on Ms. Black Volcano
wn.com/Surfing Black Mt. Volcano In Tucson Az
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close fullscreen
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4:18
Cerberus Fossae, Mars
Mars Reconnaissance Orbiter
Fissure near Cerberus Fossae with Tectonic Morphologies
Look...
published: 15 Jan 2014
Cerberus Fossae, Mars
Cerberus Fossae, Mars
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- published: 15 Jan 2014
- views: 143
2:18
Mars Geology: The Eastern Portion of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meter...
published: 11 Aug 2015
Mars Geology: The Eastern Portion of Cerberus Fossae
Mars Geology: The Eastern Portion of Cerberus Fossae
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- published: 11 Aug 2015
- views: 39
0:56
Mars Geology: Fissure near Cerberus Fossae with Tectonic Morphologies
The linearity of the volcanic vent shown in this HiRISE image (http://static.uahirise.org/...
published: 15 Jan 2014
Mars Geology: Fissure near Cerberus Fossae with Tectonic Morphologies
Mars Geology: Fissure near Cerberus Fossae with Tectonic Morphologies
- Report rights infringement
- published: 15 Jan 2014
- views: 358
2:18
The Eastern Portion of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meter...
published: 07 Jan 2015
The Eastern Portion of Cerberus Fossae
The Eastern Portion of Cerberus Fossae
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- published: 07 Jan 2015
- views: 212
3:56
The Cerberus Fossae, Woodford
published: 15 Aug 2012
The Cerberus Fossae, Woodford
The Cerberus Fossae, Woodford
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- published: 15 Aug 2012
- views: 27
1:01
Cerberus Fossae: In the Relay Zone
These trenches or "fossae" are about a kilometer (0.62 miles) across. This area shows wher...
published: 18 Feb 2015
Cerberus Fossae: In the Relay Zone
Cerberus Fossae: In the Relay Zone
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- published: 18 Feb 2015
- views: 238
2:35
Geología de Marte: La Parte Oriental de Cerberus Fossae
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conju...
published: 04 Oct 2015
Geología de Marte: La Parte Oriental de Cerberus Fossae
Geología de Marte: La Parte Oriental de Cerberus Fossae
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- published: 04 Oct 2015
- views: 90
0:44
Mars Geology: Small Floral-Shaped Volcano on Cerberus Fossae
This is a small volcano superposed on the flanks of a larger one of the Cerberus Tholi. Th...
published: 09 Aug 2015
Mars Geology: Small Floral-Shaped Volcano on Cerberus Fossae
Mars Geology: Small Floral-Shaped Volcano on Cerberus Fossae
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- published: 09 Aug 2015
- views: 19
2:18
Mars: The Eastern Portion of Cerberus Fossae
Visible in this observation is a section of Cerberus Fossae (width approximately 250 meter...
published: 09 Jan 2015
Mars: The Eastern Portion of Cerberus Fossae
Mars: The Eastern Portion of Cerberus Fossae
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- published: 09 Jan 2015
- views: 15
2:35
La parte oriental de Cerberus Fossae
Visible en esta observación hay una parte de Cerberus Fossae que está formada por un conju...
published: 04 Feb 2015
La parte oriental de Cerberus Fossae
La parte oriental de Cerberus Fossae
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- published: 04 Feb 2015
- views: 12
0:40
Mars News: "Batman's Fortress" on Cerberus
Cerberus is a large "dark spot" (an albedo feature) located on Mars and named after the my...
published: 14 Feb 2015
Mars News: "Batman's Fortress" on Cerberus
Mars News: "Batman's Fortress" on Cerberus
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- published: 14 Feb 2015
- views: 469
0:40
Eroded Terrain Near Volcanic Fissures [720p]
This observation was taken to investigate the topography near the source of fluids from th...
published: 12 Apr 2012
Eroded Terrain Near Volcanic Fissures [720p]
Eroded Terrain Near Volcanic Fissures [720p]
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- published: 12 Apr 2012
- views: 1479
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4:28
Cerberus Fossae, Mars
Mars Reconnaissance Orbiter
The Eastern Portion of Cerberus Fossae
A Recent Impact in Elys...
published: 11 Jan 2015
Cerberus Fossae, Mars
Cerberus Fossae, Mars
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- published: 11 Jan 2015
- views: 64
4:11
Marte: Paseo turístico por lo desconocido / Travel guide to Mars [IGEO.TV]
Colabora con nosotros: http://igeo.tv/contribuye-al-proyecto/
Vamos a dar una vuelta por ...
published: 16 May 2014
Marte: Paseo turístico por lo desconocido / Travel guide to Mars [IGEO.TV]
Marte: Paseo turístico por lo desconocido / Travel guide to Mars [IGEO.TV]
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- published: 16 May 2014
- views: 3443
4:22
Plan your next holiday to Mars (1)
Plan your next holiday to Mars - part 1
PIA17928: Shapes and Spots on a Polar Sand Dune ...
published: 22 Feb 2015
Plan your next holiday to Mars (1)
Plan your next holiday to Mars (1)
- Report rights infringement
- published: 22 Feb 2015
- views: 206
4:22
Plan your next holiday to Mars (2)
Plan your next holiday to Mars - part 2
PIA12956: Cerberus Fossae East of the Head of Ath...
published: 25 Mar 2015
Plan your next holiday to Mars (2)
Plan your next holiday to Mars (2)
- Report rights infringement
- published: 25 Mar 2015
- views: 101
1:57
Surfing Black Mt. volcano in Tucson AZ
Windy day on Ms. Black Volcano
published: 08 Oct 2013
Surfing Black Mt. volcano in Tucson AZ
Surfing Black Mt. volcano in Tucson AZ
- Report rights infringement
- published: 08 Oct 2013
- views: 567
Cerberus Fossae, Mars...
Marte: Paseo turístico por lo desconocido / Travel...
Plan your next holiday to Mars (1)...
Plan your next holiday to Mars (2)...
