Mostrando entradas con la etiqueta NASA’s MErcury Surface Space ENvironment GEochemistry and Ranging (MESSENGER). Mostrar todas las entradas
Mostrando entradas con la etiqueta NASA’s MErcury Surface Space ENvironment GEochemistry and Ranging (MESSENGER). Mostrar todas las entradas

domingo, 2 de octubre de 2016

NASA : Tectonically Active Planet Mercury .- Tectónicamente el Planeta Mercurio está activo...

http://www.nasa.gov/image-feature/tectonically-active-planet-mercury


Surprising new NASA-funded research suggests that Mercury is contracting even today
It’s small, it’s hot, and it’s shrinking. New NASA-funded research suggests that Mercury is contracting even today, joining Earth as a tectonically active planet.
Images obtained by NASA’s MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft reveal previously undetected small fault scarps— cliff-like landforms that resemble stair steps. These scarps are small enough that scientists believe they must be geologically young, which means Mercury is still contracting and that Earth is not the only tectonically active planet in our solar system, as previously thought.
Managed by the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland, MESSENGER launched Aug. 3, 2004 and began orbiting Mercury March 18, 2011. The mission ended with a planned impact on the surface of Mercury on April 30, 2015.
Image Credit: NASA/JHUAPL/Carnegie Institution of Washington/USGS/Arizona State University
Last Updated: Sept. 26, 2016
Editor: Sarah Loff
Tags:  Image of the Day, Mercury (Planet), MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging),
NASA
Guillermo Gonzalo Sánchez Achutegui

domingo, 3 de mayo de 2015

NASA : Overview of MESSENGER Spacecraft's Impact Region on Mercury .- Descripción general de la Región de Impacto de la nave espacial MESSENGER en Mercurio

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, sobre como será el impacto del: NASA’s MErcury Surface Space ENvironment GEochemistry and Ranging (MESSENGER), en la superficie de Mercurio. probablemente ...El 30 de abril, esta región de la superficie de Mercurio tendrá un nuevo cráter! Viajando a 3,91 kilometros por segundo (más de 8700 millas por hora), la nave espacial MESSENGER chocará con la superficie de Mercurio, creando un cráter estimado en 16 metros (52 pies) de diámetro.

More information...
Topography color coded image of section of Mercury's surface
On April 30th, this region of Mercury's surface will have a new crater! Traveling at 3.91 kilometers per second (over 8,700 miles per hour), the MESSENGER spacecraft will collide with Mercury's surface, creating a crater estimated to be 16 meters (52 feet) in diameter.
The large, 400-kilometer-diameter (250-mile-diameter), impact basin "Shakespeare" occupies the bottom left quarter of this image, acquired by the Mercury Dual Imaging System (MDIS) and Mercury Laser Altimeter (MLA) instruments aboard the spacecraft. The image is coded by topography. The tallest regions are colored red and are roughly 3 kilometers (1.9 miles) higher than low-lying areas such as the floors of impact craters, colored blue. The large crater on the left side of the image is "Janacek," with a diameter of 48 kilometers (30 miles). The Shakespeare impact basin is filled with smooth plains material, likely due to extensive lava flooding in the past. As of 24 hours before the impact, the current best estimates predict that the spacecraft will strike a ridge slightly to the northeast of Shakespeare. View this image to see more details of the predicted impact site and time.
The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. In the mission's more than four years of orbital operations, MESSENGER has acquired over 250,000 images and extensive other data sets. MESSENGER's highly successful orbital mission is about to come to an end, as the spacecraft runs out of propellant and the force of solar gravity causes it to impact the surface of Mercury on April 30, 2015.
Image Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
Last Updated: May 3, 2015
Editor: Sarah Loff
Tags:  Image of the Day, Mercury, MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging), Solar System,

Desenmascarando los Secretos de Mercurio


28.04.15.- El Espectrómetro MASCS a bordo de la nave espacial MESSENGER de la NASA fue diseñado para estudiar tanto la exosfera como la superficie del planeta Mercurio. Para aprender más acerca de los minerales y los procesos de la superficie de Mercurio, el espectrómetro visual e infrarrojo (VIRS) ha estado recogiendo diligentemente pistas individuales de mediciones espectrales de la superficie desde que MESSENGER entró en la órbita de Mercurio el 17 de Marzo de 2011.
La cobertura de las pista es ahora lo suficientemente extensa para que las propiedades espectrales de los dos amplios terrenos y las características pequeñas, tales como rejillas de ventilación piroclásticas y cráteres frescos puedan ser estudiados. Para acentuar el contexto geológico de las mediciones espectrales, los datos de MASCS se han superpuesto en el mosaico monocromo del MDIS, un instrumento con cámaras de ángulo ancho y estrecho para mapear los relieves abruptos y las variaciones espectrales en la superficie de Mercurio.
La sonda MESSENGER ha estado realizando mediciones espectrales de la superficie desde que MESSENGER entró en la órbita de Mercurio el 17 de Marzo de 2011
La sonda MESSENGER ha estado realizando mediciones espectrales de la superficie desde que MESSENGER entró en la órbita de Mercurio el 17 de Marzo de 2011. Image Credit: NASA
 
La nave espacial MESSENGER es la primera en orbitar el planeta Mercurio, y los siete instrumentos científicos de la nave espacial y la investigación científica de radio están desentrañando la historia y evolución del planeta más interior del Sistema Solar. Durante la misión, de más de cuatro años de operaciones orbitales, MESSENGER ha adquirido más de 250.000 imágenes y otros conjuntos de datos extensos. La misión orbital de gran éxito de MESSENGER está a punto de llegar a su fin, ya que la nave espacial se queda sin propelente y la fuerza de la gravedad solar provocará que impacte en la superficie de Mercurio a finales de Abril de 2015.
NASA
Guillermo Gonzalo Sánchez Achutegui
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domingo, 19 de abril de 2015

NASA : NASA Spacecraft Achieves Unprecedented Success Studying Mercury .- Nave espacial de NASA alcanza el éxito sin precedentes Estudiar Mercurio

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia espacial NASA, sobre el éxito logrado por la sonda NASA’s MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER), en sus investigaciones sobre el Planeta Mercurio, esta nave impactará  en el planeta a más de 8.750 millas por hora (3,91 kilometros por segundo) en el lado del planeta alejado de la Tierra. Debido a la ubicación esperada, los ingenieros no serán capaces de ver en tiempo real la ubicación exacta de impacto.

Messenger in orbit
NASA’s MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft traveled more than six and a half years before it was inserted into orbit around Mercury on March 18, 2011.
Credits: NASA/JHU APL/Carnegie Institution of Washington
 
After extraordinary science findings and technological innovations, a NASA spacecraft launched in 2004 to study Mercury will impact the planet’s surface, most likely on April 30, after it runs out of propellant.
NASA’s MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft will impact the planet at more than 8,750 miles per hour (3.91 kilometers per second) on the side of the planet facing away from Earth. Due to the expected location, engineers will be unable to view in real time the exact location of impact.
On Tuesday, mission operators in mission control at the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Maryland, completed the fourth in a series of orbit correction maneuvers designed to delay the spacecraft’s impact into the surface of Mercury. The last maneuver is scheduled for Friday, April 24.
"Following this last maneuver, we will finally declare the spacecraft out of propellant, as this maneuver will deplete nearly all of our remaining helium gas,” said Daniel O’Shaughnessy, mission systems engineer at APL. “At that point, the spacecraft will no longer be capable of fighting the downward push of the sun's gravity.”
Although Mercury is one of Earth’s nearest planetary neighbors, little was known about the planet prior to the MESSENGER mission.
“For the first time in history we now have real knowledge about the planet Mercury that shows it to be a fascinating world as part of our diverse solar system,” said John Grunsfeld, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington. “While spacecraft operations will end, we are celebrating MESSENGER as more than a successful mission. It’s the beginning of a longer journey to analyze the data that reveals all the scientific mysteries of Mercury.” 
The spacecraft traveled more than six and a half years before it was inserted into orbit around Mercury on March 18, 2011. The prime mission was to orbit the planet and collect data for one Earth year. The spacecraft’s healthy instruments, remaining fuel, and new questions raised by early findings resulted in two approved operations extensions, allowing the mission to continue for almost four years and resulting in more scientific firsts.
One key science finding in 2012 provided compelling support for the hypothesis that Mercury harbors abundant frozen water and other volatile materials in its permanently shadowed polar craters.
Data indicated the ice in Mercury's polar regions, if spread over an area the size of Washington, would be more than two miles thick. For the first time, scientists began seeing clearly a chapter in the story of how the inner planets, including Earth, acquired water and some of the chemical building blocks for life.
A dark layer covering most of the water ice deposits supports the theory that organic compounds,  as well as water, were delivered from the outer solar system to the inner planets and may have led to prebiotic chemical synthesis and, thusly, life on Earth.
“The water now stored in ice deposits in the permanently shadowed floors of impact craters at Mercury’s poles most likely was delivered to the innermost planet by the impacts of comets and volatile-rich asteroids,” said Sean Solomon, the mission’s principal investigator, and director of Columbia University's Lamont-Doherty Earth Observatory in Palisades, New York. “Those same impacts also likely delivered the dark organic material.”
In addition to science discoveries, the mission provided many technological firsts, including the development of a vital heat-resistant and highly reflective ceramic cloth sunshade that isolated the spacecraft’s instruments and electronics from direct solar radiation – vital to mission success given Mercury’s proximity to the sun. The technology will help inform future designs for planetary missions within our solar system.
“The front side of the sunshade routinely experienced temperatures in excess of 300° Celsius (570° Fahrenheit), whereas the majority of components in its shadow routinely operated near room temperature (20°C or 68°F),” said Helene Winters, mission project manager at APL. “This technology to protect the spacecraft’s instruments was a key to mission success during its prime and extended operations.”
The spacecraft was designed and built by APL. The lab manages and operates the mission for NASA's Science Mission Directorate. The mission is part of NASA's Discovery Program, managed for the directorate by the agency's Marshall Space Flight Center in Huntsville, Alabama.
For a complete listing of science findings and technological achievements of the mission visit:

NASA
Guillermo Gonzalo Sánchez Achutegui
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