Mostrando entradas con la etiqueta High-Resolution Imaging Science Experiment (HiRISE). Mostrar todas las entradas
Mostrando entradas con la etiqueta High-Resolution Imaging Science Experiment (HiRISE). Mostrar todas las entradas

miércoles, 11 de noviembre de 2015

NASA : Layers and Fractures in Ophir Chasma, Mars .- Capas y fracturas en Ophir Chasma, Marte

Hola amigos : A VUELO DE UN QUINDE EL BLOG., Ophir Chasma forma la porción norte de la gran sistema Valles Marineris, de cañones de Marte, y esta imagen, adquirida el 10 de agosto de 2015, por the High Resolution Imaging Science Experiment (HiRISE) de la cámara del NASA's Mars Reconnaissance Orbiter, , cuenta con una pequeña parte de su pared y el suelo.
La roca de la pared muestra muchas capas sedimentarias y el suelo está cubierto de cantos por el viento, que son de tamaño intermedio entre ondas de arena y dunas de arena. Las rocas que sobresalen en el suelo podrían ser intrusiones volcánicas de magma de una vez fundida que hizo a un lado las capas sedimentarias de los alrededores y "congeló" en su lugar.
More information....
http://www.nasa.gov/image-feature/layers-and-fractures-in-ophir-chasma-mars

Sedimentary layers on Mars surface in blue tones on left half of image and white on right
Ophir Chasma forms the northern portion of the vast Mars canyon system Valles Marineris, and this image, acquired on Aug. 10, 2015, by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter, features a small part of its wall and floor.
The wall rock shows many sedimentary layers and the floor is covered with wind-blown ridges, which are intermediate in size between sand ripples and sand dunes. Rocks protruding on the floor could be volcanic intrusions of once-molten magma that pushed aside the surrounding sedimentary layers and “froze” in place.
Images like this can help geologists study the formation mechanisms of large tectonic systems like Valles Marineris. (The word “tectonics” does not mean the same thing as “plate tectonics.” Tectonics simply refers to large stresses and strains in a planet’s crust. Plate tectonics is the main type of tectonics that Earth has; Mars does not have plate tectonics.)
The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter Project and Mars Science Laboratory Project for NASA's Science Mission Directorate, Washington.
Image Credit: NASA/JPL/University of Arizona
Caption: Kirby Runyon
Last Updated: Nov. 9, 2015
Editor: Sarah Loff
Tags:  Image of the Day, Mars, Mars Reconnaissance Orbiter (MRO), Solar System,
NASA
Guillermo Gonzalo Sánchez Achutegui
Incríbete en el Foro del blog y participa : A Vuelo De Un Quinde - El Foro!

lunes, 6 de agosto de 2012

MARS: NASA's Curiosity Rover Caught in the Act of Landing

 

Download Image

› Full Size

 NASA

 NASA's Curiosity Rover Caught in the Act of Landing
 
 PASADENA, Calif. -- An image from the High Resolution Imaging Science Experiment (HiRISE) camera aboard NASA's Mars Reconnaissance Orbiter (MRO) captured the Curiosity rover still connected to its 51-foot (almost 16 meter)-wide parachute as it descended toward its landing site at Gale Crater Sunday.

"If HiRISE took the image one second before or one second after, we probably would be looking at an empty Martian landscape," said Sarah Milkovich, HiRISE investigation scientist at the Jet Propulsion Laboratory (JPL) in Pasadena, Calif. "When you consider that we have been working on this sequence since March and had to upload commands to the spacecraft about 72 hours prior to the image being taken, you begin to realize how challenging this picture was to obtain."

The image of Curiosity on its parachute can be found at:

The image was taken while MRO was 211 miles (340 kilometers) away from the parachuting rover. Curiosity and its rocket-propelled backpack, contained within the conical-shaped back shell, had not deployed yet. At the time, Curiosity was about two miles (three kilometers) above the Martian surface.

"Guess you could consider us the closest thing to paparazzi on Mars," said Milkovich. "We definitely caught NASA's newest celebrity in the act."

Curiosity, NASA's latest contribution to the Martian landscape, landed at 10:32 p.m. PDT Aug. 5 (1:32 a.m. EDT Aug. 6) near the foot of a three-mile tall mountain inside Gale Crater, which is 96 miles in diameter.

In other Curiosity news, one part of the rover team at JPL continues to review the data from Sunday night's landing while another continues to prepare the 1-ton mobile laboratory for its future explorations of Gale Crater. One key assignment given to Curiosity for its first full day on Mars is to raise its high-gain antenna. Using this antenna will increase the data rate the rover can communicate directly with Earth. The mission will use relays to orbiters as the primary method for sending data home because that method is much more energy efficient for the rover.

Curiosity carries 10 science instruments with a total mass 15 times as large as the science payloads on the Mars rovers Spirit and Opportunity. Some of the tools, such as a laser-firing instrument for checking rocks' elemental composition from a distance, are the first of their kind on Mars. Curiosity will use a drill and scoop which is located at the end of its robotic arm to gather soil and powdered samples of rock interiors, then sieve and parcel out these samples into the rover's analytical laboratory instruments.

To handle this science toolkit, Curiosity is twice as long and five times as heavy as Spirit or Opportunity. The Gale Crater landing site places the rover within driving distance of layers of the crater's interior mountain. Observations from orbit have identified clay and sulfate minerals in the lower layers, indicating a wet history.

The Mars Science Laboratory Curiosity mission is managed by JPL for NASA's Science Mission Directorate in Washington. The rover was designed, developed and assembled at JPL. For more information on the mission, visit:
and

Follow the mission on Facebook and Twitter at:  
and

HiRISE is operated by the University of Arizona in Tucson. The instrument was built by Ball Aerospace & Technologies Corp. in Boulder, Colo. The Mars Reconnaissance Orbiter and Mars Exploration Rover projects are managed by JPL for NASA's Science Mission Directorate. JPL is a division of the California Institute of Technology in Pasadena. Lockheed Martin Space Systems in Denver, built the orbiter.

For more about the Mars Reconnaissance Orbiter, visit:  
 
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
 Inscríbete en el Foro del blog y participa : A Vuelo De Un Quinde - El Foro!

Mi lista de blogs