Mostrando entradas con la etiqueta NASA's Mars Reconnaissance Orbiter. Mostrar todas las entradas
Mostrando entradas con la etiqueta NASA's Mars Reconnaissance Orbiter. Mostrar todas las entradas

domingo, 13 de noviembre de 2016

NASA : Wind Carved Rock on Mars .- Roca tallada por el viento en Marte

Windswept elongated hills in closeup on Mars surface

 

      











The distinctively fluted surface and elongated hills in this image in Medusae Fossae on Mars are caused by wind erosion of a soft fine-grained rock. Called yardangs, these features are aligned with the prevailing wind direction. This wind direction would have dominated for a very long time to carve these large-scale features into the exposed rock we see today. The image was acquired at 15:25 local Mars time on June 28, 2016, by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.
Yardangs not only reveal the strength and direction of historic winds, but also reveal something of the host rock itself. Close inspection by HiRISE shows an absence of boulders or rubble, especially along steep yardang cliffs and buttresses. The absence of rubble and the scale of the yardangs tells us that the host rock consists only of weakly cemented fine granules in tens of meters or more thick deposits. Such deposits could have come from extended settling of volcanic ash, atmospheric dust, or accumulations of wind deposited fine sands. After a time these deposits became cemented and cohesive, illustrated by the high standing relief and exposed cliffs. 
The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.
Image Credit: NASA/JPL/University of Arizona
Caption: Michael Mellon
Last Updated: Nov. 9, 2016
Editor: Sarah Loff

NASA
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!

jueves, 14 de enero de 2016

NASA : Starburst Spider .- Starburst araña

Hola amigos: A VUELO DE UN QUINDE EL BLOG., Casquillo estacional de Marte de hielo de dióxido de carbono ha erosionado muchos terrenos hermosas, ya que sublima (pasa directamente de hielo a vapor) cada primavera. En la región donde la cámara Experimento Imágenes de Alta Resolución Science (HiRISE) de Mars Reconnaissance Orbiter de la NASA tomó esta imagen, vemos valles que forman un patrón de estallido estelar. En otras áreas de estos canales radiales se han referido como arañas, simplemente debido a su forma. En esta región el patrón se ve más dendríticas como canales ramifican varias veces a medida que más lejos del centro.
More information......

Dark spidery bedforms imaged from Mars orbit
Mars' seasonal cap of carbon dioxide ice has eroded many beautiful terrains as it sublimates (goes directly from ice to vapor) every spring. In the region where the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter took this image, we see troughs that form a starburst pattern. In other areas these radial troughs have been refered to as spiders, simply because of their shape. In this region the pattern looks more dendritic as channels branch out numerous times as they get further from the center.
 
The troughs are believed to be formed by gas flowing beneath the seasonal ice to openings where the gas escapes, carrying along dust from the surface below. The dust falls to the surface of the ice in fan-shaped deposits.
This image, covering an area about 1 kilometer (0.6 mile) across, is a portion of the HiRISE observation catalogued as ESP_011842_0980, taken on Feb. 4, 2009. The observation is centered at 81.8 degrees south latitude, 76.2 degrees east longitude. The image was taken at a local Mars time of 4:56 p.m. and the scene is illuminated from the west with a solar incidence angle of 78 degrees, thus the sun was about 12 degrees above the horizon. At a solar longitude of 203.6 degrees, the season on Mars is northern autumn.
NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, is the prime contractor for the project and built the spacecraft. The High Resolution Imaging Science Experiment is operated by the University of Arizona, Tucson, and the instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo.

Image Credit: NASA/JPL-Caltech/University of Arizona
Last Updated: Jan. 11, 2016
Editor: NASA Administrator
NASA
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!

viernes, 2 de mayo de 2014

NASA : Active Dune Field on Mars


Active Dune Field on Mars
Nili Patera is one of the most active dune fields on Mars. As such, it is continuously monitored with the HiRISE (High Resolution Imaging Science Experiment) camera, a science instrument aboard NASA's Mars Reconnaissance Orbiter, with a new image acquired about every six weeks.
By monitoring the sand dune changes, we can determine how winds vary seasonally and year-to-year. This observation is one of the more recent Nili images, acquired on March 1, 2014. Compared to an image acquired on Nov. 22, 2012, changes are obvious. The ripples on the dunes have moved, as well some of the dune boundaries, such as the one at upper left. New landslides on the central dune's lee face are apparent.
Such changes, in just 16 months (and finer scale changes have been seen in just a couple of weeks), demonstrate the effectiveness of wind in modifying the Martian landscape.
HiRISE is one of six instruments on NASA's Mars Reconnaissance Orbiter. The University of Arizona, Tucson, operates the orbiter's HiRISE camera, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter Project for the NASA Science Mission Directorate, Washington.
Image Credit: NASA/JPL-Caltech/Univ. of Arizona
Caption: Nathan Bridges
NASA
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!

viernes, 26 de julio de 2013

NASA - View From Mars Orbiter Showing Curiosity Rover at 'Shaler'


View From Mars Orbiter Showing Curiosity Rover at 'Shaler'
NASA's Mars Science Laboratory rover Curiosity appears as a bluish dot near the lower right corner of this enhanced-color view from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter. The rover's tracks are visible extending from the landing site, "Bradbury Landing," in the left half of the scene. Two bright, relatively blue spots surrounded by darker patches are where the Mars Science Laboratory spacecraft's landing jets cleared away reddish surface dust at the landing site. North is toward the top. For scale, the two parallel lines of the wheel tracks are about 10 feet (3 meters) apart.
HiRISE shot this image on June 27, 2013, when Curiosity was at an outcrop called "Shaler" in the "Glenelg" area of Gale Crater. Subsequently the rover drove away from Glenelg toward the southwest.
When HiRISE captured this view, the Mars Reconnaissance Orbiter was rolled for an eastward-looking angle rather than straight downward. The afternoon sun illuminated the scene from the western sky, so the lighting was nearly behind the camera. Specifically, the angle from sun to orbiter to rover was just 5.47 degrees. This geometry hides shadows and reveals subtle color variations.
The image is one product from HiRISE observation ESP_032436_1755. Other image products from this observation are available at
HiRISE is one of six instruments on NASA's Mars Reconnaissance Orbiter. The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter and Mars Science Laboratory projects for NASA's Science Mission Directorate, Washington.
Image credit: NASA/JPL-Caltech/Univ. of Arizona
NASA
Guillermo Gonzalo Sánchez Achutegui

miércoles, 12 de junio de 2013

NASA - Marks on Martian Dunes May Reveal Tracks of Dry Ice Sleds


Several types of downhill flow features have been observed on Mars. This image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter is an example of a type called 'linear gullies.' 
 Several types of downhill flow features have been observed on Mars. This image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter is an example of a type called "linear gullies." Image credit: NASA/JPL-Caltech/Univ. of Arizona › Full image and caption    
 
This graphic compares seven different types of features observed on Mars that appear to result from material flowing or sliding or rolling down slopes. 
 As on the Earth, many processes can move material down a Martian slope. This graphic compares seven different types of features observed on Mars that appear to result from material flowing or sliding or rolling down slopes. Image credit: NASA/JPL-Caltech/ASA/MSSS/UA
› Full image and caption

These examples of one distinctive type of Martian gullies, called 'linear gullies,' are on a dune in Matara Crater, seen at different times of year to observe changes. 
 These examples of one distinctive type of Martian gullies, called "linear gullies," are on a dune in Matara Crater, seen at different times of year to observe changes. Image credit: NASA/JPL-Caltech/Univ. of Arizona
› Full image and caption

PASADENA, Calif. -- NASA research indicates hunks of frozen carbon dioxide -- dry ice -- may glide down some Martian sand dunes on cushions of gas similar to miniature hovercraft, plowing furrows as they go.
Researchers deduced this process could explain one enigmatic class of gullies seen on Martian sand dunes by examining images from NASA's Mars Reconnaissance Orbiter (MRO) and performing experiments on sand dunes in Utah and California.
"I have always dreamed of going to Mars," said Serina Diniega, a planetary scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and lead author of a report published online by the journal Icarus. "Now I dream of snowboarding down a Martian sand dune on a block of dry ice."
The hillside grooves on Mars, called linear gullies, show relatively constant width -- up to a few yards, or meters, across -- with raised banks or levees along the sides. Unlike gullies caused by water flows on Earth and possibly on Mars, they do not have aprons of debris at the downhill end of the gully. Instead, many have pits at the downhill end.
"In debris flows, you have water carrying sediment downhill, and the material eroded from the top is carried to the bottom and deposited as a fan-shaped apron," said Diniega. "In the linear gullies, you're not transporting material. You're carving out a groove, pushing material to the sides."
Images from MRO's High Resolution Imaging Science Experiment (HiRISE) camera show sand dunes with linear gullies covered by carbon-dioxide frost during the Martian winter. The location of the linear gullies is on dunes that spend the Martian winter covered by carbon-dioxide frost. By comparing before-and-after images from different seasons, researchers determined that the grooves are formed during early spring. Some images have even caught bright objects in the gullies.
Scientists theorize the bright objects are pieces of dry ice that have broken away from points higher on the slope. According to the new hypothesis, the pits could result from the blocks of dry ice completely sublimating away into carbon-dioxide gas after they have stopped traveling.
"Linear gullies don't look like gullies on Earth or other gullies on Mars, and this process wouldn't happen on Earth," said Diniega. "You don't get blocks of dry ice on Earth unless you go buy them."
That is exactly what report co-author Candice Hansen, of the Planetary Science Institute in Tucson, Ariz., did. Hansen has studied other effects of seasonal carbon-dioxide ice on Mars, such as spider-shaped features that result from explosive release of carbon-dioxide gas trapped beneath a sheet of dry ice as the underside of the sheet thaws in spring. She suspected a role for dry ice in forming linear gullies, so she bought some slabs of dry ice at a supermarket and slid them down sand dunes.
That day and in several later experiments, gaseous carbon dioxide from the thawing ice maintained a lubricating layer under the slab and also pushed sand aside into small levees as the slabs glided down even low-angle slopes.
The outdoor tests did not simulate Martian temperature and pressure, but calculations indicate the dry ice would act similarly in early Martian spring where the linear gullies form. Although water ice, too, can sublimate directly to gas under some Martian conditions, it would stay frozen at the temperatures at which these gullies form, the researchers calculate.
"MRO is showing that Mars is a very active planet," Hansen said. "Some of the processes we see on Mars are like processes on Earth, but this one is in the category of uniquely Martian."
Hansen also noted the process could be unique to the linear gullies described on Martian sand dunes.
"There are a variety of different types of features on Mars that sometimes get lumped together as 'gullies,' but they are formed by different processes," she said. "Just because this dry-ice hypothesis looks like a good explanation for one type doesn't mean it applies to others."
The University of Arizona Lunar and Planetary Laboratory operates the HiRISE camera, which was built by Ball Aerospace & Technologies Corp. of Boulder, Colo. JPL, a division of the California Institute of Technology in Pasadena, manages MRO for NASA's Science Mission Directorate in Washington. Lockheed Martin Space Systems, Denver, built the orbiter.
To see images of the linear gullies and obtain more information about MRO, visit: http://www.nasa.gov/mro .
For more about HiRISE,
 
 
Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov
NASA
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!

sábado, 15 de diciembre de 2012

NASA Makes Unprecedented Return to Mars, Advances Commercial Spaceflight and Adds to its Amazing Research and Discoveries in 2012

WASHINGTON -- In 2012, NASA continued to implement America's ambitious space exploration program, landing the most sophisticated rover on the surface of Mars, carrying out the first-ever commercial mission to the International Space Station and advancing the systems needed to send humans deeper into space.

"NASA achieved historic milestones this year landing the most sophisticated rover on the surface of Mars, carrying out the first ever commercial mission to the space station and continuing to advance the systems needed to send humans deeper into space -- beyond the moon, to an asteroid and on to Mars," NASA Administrator Charles Bolden said. "We are able to keep the United States the world leader in space exploration -- and continue to implement America's bipartisan space plan -- because of our talented and dedicated work force."

The following are some of NASA's top stories this year:

NASA LANDS CAR-SIZE ROVER BESIDE MARTIAN MOUNTAIN

Undertaking the most complex landing ever attempted in planetary exploration, NASA successfully placed the most advanced robotic rover on Mars. The Mars Science Laboratory mission carrying the one-ton rover named Curiosity, touched down in August. Almost immediately, Curiosity sent back pictures of its landing site at Gale Crater with the eventual destination of Mount Sharp in the background. Since then, Curiosity has checked out its 10 science instruments, sent back detailed photos and weather observations and "tasted" Martian soil.

Key mission findings during the first three months after the landing include conglomerate rocks bearing rounded pebbles as evidence of vigorous ancient stream flow right in the area where Curiosity landed; mineral composition of Martian soil similar to soils in Hawaii that contain volcanic glass; and the first assessment of the natural radiation environment that future astronauts will encounter on the surface of Mars.

Curiosity's planned two-year prime mission will be to explore and assess a local region on the surface of Mars as a potential habitat for life, past or present. In addition, the landing technology for putting such a large payload safely on the Martian surface could help with plans for future human Mars missions.

On Dec. 4, NASA announced plans for a robust multi-year Mars program, including a new robotic science rover based on the Curiosity design set to launch in 2020. The planned portfolio includes the Curiosity and Opportunity rovers; two NASA spacecraft and contributions to one European spacecraft currently orbiting Mars; the 2013 launch of the Mars Atmosphere and Volatile EvolutioN (MAVEN) orbiter to study the Martian upper atmosphere; the Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) mission, which will take the first look into the deep interior of Mars; and participation in ESA's 2016 and 2018 ExoMars missions, including providing "Electra" telecommunication radios to ESA's 2016 mission and a critical element of the premier astrobiology instrument on the 2018 ExoMars rover. With InSight, there will be a total of seven NASA missions operating or being planned to study and explore our Earth-like neighbor.

The 2020 mission will constitute another step toward being responsive to high-priority science goals and the president's challenge of sending humans to Mars orbit in the 2030s.


NASA ADVANCES COMMERCIAL SPACEFLIGHT, HELPS MAKE HISTORY

A Space Exploration Technologies Corp. (SpaceX) Dragon spacecraft successfully resupplied the International Space Station and returned cargo back to Earth in October, completing NASA's first contracted cargo delivery flight.

Under NASA's Commercial Resupply Services contract, SpaceX will fly at least 12 cargo missions to the space station through 2016. The Dragon launched on a SpaceX Falcon 9 rocket carrying 882 pounds of cargo, including crew supplies, scientific research and hardware. Dragon returned almost twice that amount of cargo, including a freezer packed with research samples collected in the orbiting laboratory's unique microgravity environment. These samples will help advance multiple scientific disciplines on Earth and provide critical data on the effects of long-duration spaceflight on the human body. The ability to return frozen samples is a first for this flight and will be tremendously beneficial to the station's research community. Not since the space shuttle have NASA and its international partners been able to return considerable amounts of research and samples for analysis.

SpaceX is one of two companies that built and tested new cargo spacecraft under NASA's Commercial Orbital Transportation Services (COTS) program. SpaceX completed its final demonstration test flight in May, becoming the first commercial company ever to launch, rendezvous and be docked to the International Space Station. Orbital Sciences is the other company participating in COTS. Orbital's Antares launch vehicle is on the launch pad at Wallops Flight Facility in Virginia in advance of a hot fire test of the Antares first-stage engines. A flight test of the Antares with a simulated Cygnus spacecraft and a demonstration flight of Cygnus to the space station are planned for 2013.

With commercial cargo flights to the space station under way in 2012, NASA took the next steps in the effort to launch Americans from U.S. soil again. The agency announced in August new agreements with three American commercial companies to design and develop the next generation of U.S. human spaceflight capabilities, enabling a launch of astronauts from the United States in the next five years.

Advances made by these companies under Space Act Agreements through the agency's Commercial Crew Integrated Capability (CCiCap) initiative are intended to ultimately lead to the availability of commercial human spaceflight services for government and commercial customers. The CCiCap partners are the Sierra Nevada Corporation, Space Exploration Technologies (SpaceX), and The Boeing Company.

CCiCap is an initiative of NASA's Commercial Crew Program (CCP) and an administration priority. The objective of the CCP is to facilitate the development of a U.S. commercial crew space transportation capability with the goal of achieving safe, reliable and cost-effective access to and from the International Space Station and low-Earth orbit. Between now and May 31, 2014, NASA's partners will perform tests and mature integrated designs. This would then set the stage for a future activity that will launch crewed orbital demonstration missions to low-Earth orbit by the middle of the decade.

SPACE STATION FULLY OPERATIONAL WITH NEW RESEARCH AND TECHNOLOGY TESTING

NASA and its international partners celebrated 12 years of permanent human habitation on the International Space Station on Nov. 2. More than 1,500 research and technology development experiments have been conducted aboard the orbiting lab -- more than 200 of them this year alone -- many of which are producing advances in medicine, environmental systems and our understanding of the universe.

Human research studies, including new research announced in August, have shown that using the Advanced Resistive Exercise Device for high-intensity workouts aboard the orbiting laboratory, in combination with proper diets, helps astronauts lose less bone density during their stay. This could have profound effects on future space exploration, as well as the aging population on Earth. Plant-growth studies are often on the menu, as the ability to grow plants in microgravity would allow for fresh food, oxygen generation and carbon dioxide removal. This research also could help improve crop production on the ground.

Several new facilities delivered to the space station this year allow for an array of new research projects. The Japanese Experiment Module Small Satellite Orbital Deployer changes the way mini satellites now can be deployed to their optimal orbit, allowing for greater flexibility, operational control and significant monetary savings. The Aquatic Habitat received its first inhabitants, translucent Medaka fish, allowing for easy observation of their skeletal systems, which gives more insight into bone and muscle atrophy, which are medical issues for astronauts and the aging population, and radiation effects. A Gravitational Biology Lab also was delivered to station. The centrifuge allows for biological experimentation in artificial gravity -- from zero gravity to twice Earth's normal gravity -- for prolonged periods of time. This facility provides environmental control, lighting, data transfer, commanding and observation of experiments in Mars and moon gravity conditions, as well as mimicking Earth's gravity. The centrifuge is useful for biological organism research and could lead to advances in medications and vaccines, agricultural controls and discoveries in genetics -- all beneficial to people on Earth.

WORK UNDER WAY FOR FIRST LAUNCHES OF NASA'S NEW SPACECRAFT AND ROCKET

In July, NASA's Kennedy Space Center in Florida welcomed the arrival of the agency's first space-bound Orion capsule, marking a major milestone in the construction of the spacecraft that will carry astronauts farther into space than ever before. Orion will be the most advanced spacecraft ever designed, sustaining astronauts during space travel, providing safe re-entry from deep space and emergency abort capability.

The Orion at Kennedy will launch on Exploration Flight Test-1, an uncrewed mission planned for 2014. The spacecraft will travel 3,600 miles above the Earth's surface, 15 times farther than the International Space Station's orbital position. The primary flight objective is to understand Orion's heat shield performance at speeds generated during a return from deep space.

NASA and its industry partners around the country also made swift progress on the Space Launch System (SLS) this year, testing and developing new components and improving on existing hardware. New construction on the largest rocket ever built is enabled by existing, proven technology, like the space shuttle main engines that will power the first stage of the rocket. The new J-2X engine, which is targeted to power the upper stage of the rocket, underwent a battery of tests that broke duration records and pushed the engine design to its limits.

The Orion, SLS, and Ground Systems Development and Operations programs also reached their critical milestones this year each with an approved system requirement review and system definition review. Those pivotal steps allowed these programs to move from concept into its preliminary design phase and all remain on target for its first flight test in 2017.

NASA'S HUBBLE PROVIDES FIRST CENSUS OF GALAXIES NEAR COSMIC DAWN

Using NASA's Hubble Space Telescope, astronomers announced Dec. 12 they have seen further back in time than ever before and have uncovered a previously unseen population of seven primitive galaxies that formed more than 13 billion years ago, when the universe was less than 3 percent of its present age. The deepest images to date from Hubble yield the first statistically robust sample of galaxies that tells how abundant they were close to the era when galaxies first formed.

The greater depth of the new Hubble images, together with a carefully designed survey strategy, allows this work to go further than previous studies, thereby providing what researchers say is the first reliable galaxy census of this epoch. Notably, one of the galaxies may be a distance record breaker, observed 380 million years after the birth of our universe in the theorized big bang.

Looking deeper into the universe also means peering further back in time. The universe is estimated to be 13.7 billion years old. The newly discovered galaxies are seen as they looked 350 to 600 million years after the big bang. Their light is just arriving at Earth now.

ICE SHEET LOSS AT BOTH POLES INCREASING

An international team of experts supported by NASA and the European Space Agency combined data from multiple satellites and aircraft to produce the most comprehensive and accurate assessment to date of ice sheet losses in Greenland and Antarctica and their contributions to sea level rise.

The combined rate of melting for the ice sheets covering Greenland and Antarctica increased during the last 20 years. Together, these ice sheets are losing more than three times as much ice each year as they were in the 1990s. About two-thirds of the loss is coming from Greenland, with the rest from Antarctica.

The study announced in November was produced by an international collaboration -- the Ice Sheet Mass Balance Inter-comparison Exercise -- that combined observations from 10 satellite missions to develop the first consistent measurement of polar ice sheet changes. Satellite data from NASA's Ice, Cloud and land Elevation Satellite (ICESat) and the NASA/German Aerospace Center's Gravity Recovery and Climate Experiment (GRACE) missions were included in the study.

This activity was a major challenge involving cutting-edge, difficult research to produce the most rigorous and detailed estimates of ice loss from Greenland and Antarctica to date.

NASA'S AERONAUTICS RESEARCH WORKS TO MAKE A SILENT SONIC BOOM

NASA is continuing to learn more about how sound waves created by supersonic aircraft move through the atmosphere, all with an eye towards designing aircraft that generate sonic booms you can barely hear -- or can't hear at all -- on the ground below. This work could open a whole new segment of the economy for commercial aviation by making supersonic flight over land acceptable.

Following a series of research flights last year, NASA engineers in 2012 poured over information they gathered from residents near Edwards Air Force Base in California to see how well they did in generating sonic booms with NASA's F/A-18 jet that could barely be heard on the ground. The Waveforms and Sonic boom Perception and Response, or WSPR, project gathered data from a select group of more than 100 volunteers. A final report on the study is due soon.

Another phase of this research began in 2012 with the Farfield Investigation of No Boom Threshold, or FaINT. Using NASA's F/A-18 supersonic jet, project researchers will try to better understand what's happening at the very edge of the sonic boom, or just beyond.

and


SPACE TECHNOLOGY PROGRAM SHARPENS CUTTING-EDGE TECHNOLOGIES

With a new set of Space Technology Roadmaps as a guide, NASA's Office of the Chief Technologist and the Space Technology Program continued to make great strides in creating the new knowledge and capabilities needed for NASA's current and future missions in 2012. NASA's Space Technology Program is innovating, developing, testing, and flying technology for use in NASA's future missions and by the greater aerospace community. With more than 800 projects under way, many of which are partnering with universities and industry, the program continues to meet milestones and advance NASA's technology capabilities.

This year, NASA's Space Technology Program launched and successfully demonstrated a hypersonic inflatable reentry vehicle, proving that inflatable heat shields are viable for safely slowing large-mass payloads during their fiery entry through planetary atmospheres, like those of Earth or Mars.

NASA continues to invest in and create new enabling robotic technologies that aid in future exploration while also having applications here one Earth, potentially helping paraplegics walk and aiding in other medical rehabilitation efforts. Investments in improved woven thermal protection systems also made strides this year using commercially available 3-D weaving techniques, reducing life cycle costs and allowing for sustainable and scalable space missions.

Rebuilding the bridge to new ideas and the nation's top talent, Space Technology is engaging in more than 350 activities with approximately 100 universities and academic institutions through fellowships, direct competitive awards and partnerships with NASA centers, and commercial contractors for its technology developments and demonstrations.

In addition, NASA technologies continue to create thousands of jobs and revenue while significantly improving the quality of life for millions of people here on Earth.

NASA EDUCATION PROVIDES HANDS-ON LEARNING OPPORTUNITIES

NASA's 2012 Summer of Innovation program continued to offer a variety of programs to provide summer learning opportunities to students and teachers. The program reached approximately 42,000 students in grades 4-9 across the country, many of whom fell within the agency's target audience of underrepresented and underserved students. The program also provided professional development for more than 3,200 middle school teachers nationwide to help them improve their ability to teach STEM content in the classroom.

SPACECRAFT FINDS NEW EVIDENCE FOR ICE ON MERCURY

NASA's MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft provided compelling support for the long-held hypothesis the planet harbors abundant water ice and other frozen volatile materials within its permanently shadowed polar craters.

The spacecraft's onboard instruments have been studying Mercury in unprecedented detail since its historic arrival there in March 2011. Scientists are seeing clearly for the first time a chapter in the story of how the inner planets, including Earth, acquired their water and some of the chemical building blocks for life.

The new data announced in December indicated the water ice in Mercury's polar regions, if spread over an area the size of Washington, D.C., would be more than 2 miles thick. Given its proximity to the sun, Mercury would seem to be an unlikely place to find ice, however, there are pockets at the planet's poles that never see sunlight.

IBEX SPACECRAFT REVEALS NEW OBSERVATIONS OF INTERSTELLAR MATTER

NASA announced in January its Interstellar Boundary Explorer (IBEX) spacecraft captured the best and most complete glimpse yet of what lies beyond the solar system -- observations that show our solar system is different than the space right outside it. The new measurements give clues about how and where our solar system formed, the forces that physically shape our solar system, and the history of other stars in the Milky Way.

The spacecraft observed four separate types of atoms, including hydrogen, oxygen, neon and helium. These interstellar atoms are the byproducts of older stars, which spread across the galaxy and fill the vast space between stars. IBEX determined the distribution of these elements outside the solar system that are flowing charged and neutral particles, which blow through the galaxy.

IBEX also measured the interstellar wind traveling at a slower speed than previously measured by the Ulysses spacecraft, and from a different direction. The improved measurements from IBEX show a 20 percent difference in how much pressure the interstellar wind exerts on our heliosphere. Measuring the pressure on our heliosphere from the material in the galaxy and from the magnetic fields out there will help determine the size and shape of our solar system as it travels through the galaxy.

WISE MISSION SEES SKIES ABLAZE WITH BLAZARS

Astronomers announced in April they were actively hunting a class of supermassive black holes throughout the universe called blazars thanks to data collected by NASA's Wide-field Infrared Survey Explorer. The mission revealed more than 200 blazars to date with the potential for finding thousands more.

Blazars are among the most energetic objects in the universe. They consist of supermassive black holes actively "feeding," or pulling matter onto them, at the cores of giant galaxies. As the matter is dragged toward the supermassive hole, some of the energy is released in the form of jets traveling at nearly the speed of light. The findings ultimately will help researchers understand the extreme physics behind super-fast jets and the evolution of supermassive black holes in the early universe.

SPACE SHUTTLES ARRIVE AT NEW HOMES

With the final flight of the Space Shuttle Program in 2011, the shuttles themselves were delivered in 2012 to their new homes, where they will begin a new chapter in their careers: inspiring museum-goers of all ages to reach for the stars.
Discovery arrived at the Smithsonian Institution's National Air and Space Museum in Dulles, Virginia, in April; Enterprise was unveiled at the Intrepid Sea, Air and Space Museum in New York in July; Endeavour was moved to the California Science Center in Los Angeles in October; and Atlantis was relocated to the Kennedy Space Center Visitor Complex in Florida in November.

NASA'S SOCIAL MEDIA AND INTERNET TEAMS CONNECT WITH THE PUBLIC

NASA's social media activities continued to evolve in 2012. With more than 3.2 million Twitter followers on the agency's flagship account @NASA, more than a million on Facebook, and a growing audience of hundreds of thousands on Google+, NASA is connecting directly with more people to share the agency's activities, people and mission.

NASA's online media teams provided live coverage of several major agency events and milestones, including this year's historic SpaceX launches to the International Space Station, the Transit of Venus and the landing of the Curiosity rover on Mars. In each event, the agency shattered records for new levels of online engagement with live updates of each event that reached millions, and in the case of Curiosity -- billions, of people.

During the August Mars Curiosity rover landing, NASA's website received 15 million visits and sent out 36 million webcast streams of NASA TV, breaking records that had just been set during the Venus Transit (4.2 million website visits, 7.7 million webcast streams). In October, Curiosity checked-in on Foursquare from Gale Crater, making it the first time a check-in has happened on another planet. The two events contributed to record traffic to the site, 185 million visits through Nov. 30, up from 151 million for 2011.

For the first time, visits to NASA.gov from mobile devices contributed a significant amount of traffic, totaling more than 10 percent of all visits. The site was honored with its fifth People's Voice Webby for best government site, and for the first time received the judges' Webby award as well. NASA.gov also was chosen by Time magazine as one of the 50 Best Websites of 2012.

NASA transitioned our in-person social media events from NASA Tweetups to NASA Socials, included more social media platforms and held the agency's first multi-NASA center social for Curiosity's landing. NASA's social media teams held 16 events, bringing more than 1,000 people into NASA and other facilities.

The agency also worked to integrated social media into more daily news processes than ever before. From inviting social media followers to participate in NASA news briefings and events to being able to virtually attend events held for news media, such as the Orion capsule arrival at Kennedy Space Center in July. NASA also offered more than a dozen opportunities to ask questions of agency officials using #askNASA, including in several Google+ Hangouts, providing additional direct interaction points between the public and NASA.

and

   
A little more than a year after the final shuttle mission, NASA helped return cargo flights to the International Space Station from U.S. soil, furthered the development of U.S. commercial spaceflight systems to transport astronauts to the space station and made progress toward the first launches of NASA's new deep-space spacecraft and heavy-lift rocket. Complemented by key research and technology products to enable long journeys into space, NASA continued making the investments in 2012 required to undertake this new era of deep space exploration.

NASA Television's Video File newsfeed will include items featuring these top stories beginning at noon EST, Dec. 17. For NASA TV streaming video, schedules and downlink information, visit:

NASA's website will highlight these stories and more also starting at noon on Dec. 17. Visit:

Download Image

› Full Size 

The NASA Mars rover Curiosity used its Mast Camera (Mastcam) during the mission's 120th Martian day, or sol (Dec. 7, 2012), to record this view of a rock outcrop informally named "Shaler." Image credit: NASA/JPL-Caltech/MSSS
› Full image and caption       › Latest images       › Curiosity gallery       › Curiosity videos

Download Image

› Full Size 


PASADENA, Calif. -- The NASA Mars rover Curiosity drove 63 feet (19 meters) northeastward early Monday, Dec. 10, approaching a step down into a slightly lower area called "Yellowknife Bay," where researchers intend to choose a rock to drill.
The drive was Curiosity's fourth consecutive driving day since leaving a site near an outcrop called "Point Lake," where it arrived last month. These drives totaled 260 feet (79 meters) and brought the mission's total odometry to 0.37 mile (598 meters).
The route took the rover close to an outcrop called "Shaler," where scientists used Curiosity's Chemistry and Camera (ChemCam) instrument and Mast Camera (Mastcam) to assess the rock's composition and observe its layering. Before departure from Point Lake, a fourth sample of dusty sand that the rover had been carrying from the "Rocknest" drift was ingested and analyzed by Curiosity's Sample Analysis at Mars (SAM) instrument.
Curiosity ended Monday's drive about 30 percent shorter than planned for the day when it detected a slight difference between two calculations of its tilt, not an immediate risk, but a trigger for software to halt the drive as a precaution. "The rover is traversing across terrain different from where it has driven earlier, and responding differently," said Rick Welch, mission manager at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "We're making progress, though we're still in the learning phase with this rover, going a little slower on this terrain than we might wish we could."
Curiosity is approaching a lip where it will descend about 20 inches (half a meter) to Yellowknife Bay. The rover team is checking carefully for a safe way down. Yellowknife Bay is the temporary destination for first use of Curiosity's rock-powdering drill, before the mission turns southwestward for driving to its main destination on the slope of Mount Sharp.
JPL, a division of the California Institute of Technology, Pasadena, manages the Mars Science Laboratory Project and the mission's Curiosity rover for NASA's Science Mission Directorate, Washington. JPL designed and built the rover.
More information about Curiosity is online 
You can follow the mission on Facebook 
Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov
NASA
Guillermo Gonzalo Sánchez Achuteguui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
Inscríbete en el Foro del blog y participa : A Vuelo De Un Quinde - El Foro!

domingo, 23 de septiembre de 2012

Astronomy: NASA Dawn Spacecraft Sees Hydrated Minerals on Giant Asteroid


Download Image

› Full Size

 The animation from NASA's Dawn mission shows abundances of hydrogen in a wide swath around the equator of the giant asteroid Vesta. › Download video

Download Image

› Full Size


 NASA Dawn Spacecraft Sees Hydrated Minerals on Giant Asteroid
 
 
WASHINGTON -- NASA's Dawn spacecraft has revealed the giant asteroid Vesta has its own version of ring around the collar. Two new papers, based on observations from the low-altitude mapping orbit of the Dawn mission, show volatile, or easily evaporated, materials have colored Vesta's surface in a broad swath around its equator.

The volatiles were released from minerals likely containing water. Pothole-like features mark some of the asteroid's surface where the volatiles boiled off. Dawn did not find actual water ice at Vesta. However, it found evidence of hydrated minerals delivered by meteorites and dust in the giant asteroid's chemistry and geology. The findings appear Thursday in the journal Science.

One paper, led by Thomas Prettyman, the lead scientist for Dawn's gamma ray and neutron detector (GRaND) at the Planetary Science Institute in Tucson, Ariz., describes how the instrument found signatures of hydrogen, likely in the form of hydroxyl or water bound to minerals in Vesta's surface.

"The source of the hydrogen within Vesta's surface appears to be hydrated minerals delivered by carbon-rich space rocks that collided with Vesta at speeds slow enough to preserve their volatile content," said Prettyman.

A complementary paper, led by Brett Denevi, a Dawn participating scientist at the Johns Hopkins University Applied Physics Laboratory in Laurel, Md., describes the presence of pitted terrain created by the release of the volatiles.

Vesta is the second most massive member of our solar system's main asteroid belt. Dawn was orbiting at an average altitude of about 130 miles (210 kilometers) above the surface when it obtained the data. Dawn left Vesta on Sept. 5 EDT (Sept. 4) and is on its way to a second target, the dwarf planet Ceres.

Scientists thought it might be possible for water ice to survive near the surface around the giant asteroid's poles. Unlike Earth's moon, however, Vesta has no permanently shadowed polar regions where ice might survive. The strongest signature for hydrogen in the latest data came from regions near the equator, where water ice is not stable.

In some cases, space rocks crashed into these deposits at high speed. The heat from the collisions converted the hydrogen bound to the minerals into water, which evaporated. Escaping water left holes as much as six-tenths of a mile (1 kilometer) wide and as deep as 700 feet (200 meters). Seen in images from Dawn's framing camera, this pitted terrain is best preserved in sections of Marcia crater.

"The pits look just like features seen on Mars, and while water was common on Mars, it was totally unexpected on Vesta in these high abundances," said Denevi. "These results provide evidence that not only were hydrated materials present, but they played an important role in shaping the asteroid's geology and the surface we see today."

GRaND's data are the first direct measurements describing the elemental composition of Vesta's surface. Dawn's elemental investigation by the instrument determined the ratios of iron to oxygen and iron to silicon in the surface materials. The new findings solidly confirm the connection between Vesta and a class of meteorites found on Earth called the Howardite, Eucrite and Diogenite meteorites, which have the same ratios for these elements. In addition, more volatile-rich fragments of other objects have been identified in these meteorites, which supports the idea the volatile-rich material was deposited on Vesta.

The Dawn mission is managed by NASA's Jet Propulsion Laboratory for the Science Mission Directorate in Washington. The spacecraft is as a project of the Discovery Program managed by NASA's Marshall Space Flight Center in Huntsville, Ala. The University of California, Los Angeles, is responsible for overall mission science. Orbital Sciences Corporation of Dulles, Va., designed and built the spacecraft.

The framing cameras that saw the pitted terrain were developed and built under the leadership of the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, with contributions by the German Aerospace Center (DLR) Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig. The framing camera project is funded by NASA, the Max Planck Society and DLR. The gamma ray and neutron detector instrument was built by Los Alamos National Laboratory, N.M., and is operated by the Planetary Science Institute.

To view new images and for more information about Dawn, visit:
http://www.nasa.gov/dawn 
NASA
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!

martes, 14 de agosto de 2012

MARS: Curiosity in Exaggerated Color

 

Download Image

› Full Size 

NASA
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!

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!

martes, 12 de junio de 2012

Astronomy: NASA Mars Rover Team Aims for Landing Closer to Prime Science Site

Hi My Friends: A VUELO DE UN QUINDE EL BLOG., NASA has narrowed the target for its most advanced Mars rover, Curiosity, which will land on the Red Planet in August. The car-sized rover will arrive closer to its ultimate destination for science operations, but also closer to the foot of a mountain slope that poses a landing hazard.

Download Image

› Full Size 


PASADENA, Calif. -- NASA has narrowed the target for its most advanced Mars rover, Curiosity, which will land on the Red Planet in August. The car-sized rover will arrive closer to its ultimate destination for science operations, but also closer to the foot of a mountain slope that poses a landing hazard.
"We're trimming the distance we'll have to drive after landing by almost half," said Pete Theisinger, Mars Science Laboratory project manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "That could get us to the mountain months earlier."
It was possible to adjust landing plans because of increased confidence in precision landing technology aboard the Mars Science Laboratory spacecraft, which is carrying the Curiosity rover. That spacecraft can aim closer without hitting Mount Sharp at the center of Gale crater. Rock layers located in the mountain are the prime location for research with the rover.
Curiosity is scheduled to land at approximately 10:31 p.m. PDT Aug. 5 (1:31 a.m. EDT, Aug. 6). Following checkout operations, Curiosity will begin a two-year study of whether the landing vicinity ever offered an environment favorable for microbial life.
Theisinger and other mission leaders described the target adjustment during an update to reporters on Monday, June 11, about preparations for landing and for operating Curiosity on Mars.
The landing target ellipse had been approximately 12 miles wide and 16 miles long (20 kilometers by 25 kilometers). Continuing analysis of the new landing system's capabilities has allowed mission planners to shrink the area to approximately 4 miles wide and 12 miles long (7 kilometers by 20 kilometers), assuming winds and other atmospheric conditions are as predicted.
Even with the smaller ellipse, Curiosity will be able to touch down at a safe distance from steep slopes at the edge of Mount Sharp.
"We have been preparing for years for a successful landing by Curiosity, and all signs are good," said Dave Lavery, Mars Science Laboratory program executive at NASA. "However, landing on Mars always carries risks, so success is not guaranteed. Once on the ground we'll proceed carefully. We have plenty of time since Curiosity is not as life-limited as the approximate 90-day missions like NASA’s Mars Exploration Rovers and the Phoenix lander.”
Since the spacecraft was launched in November 2011, engineers have continued testing and improving its landing software. Mars Science Laboratory will use an upgraded version of flight software installed on its computers during the past two weeks. Additional upgrades for Mars surface operations will be sent to the rover about a week after landing.
Other preparations include upgrades to the rover's software and understanding effects of debris coming from the drill the rover will use to collect samples from rocks on Mars. Experiments at JPL indicate that Teflon from the drill could mix with the powdered samples. Testing will continue past landing with copies of the drill. The rover will deliver the samples to onboard instruments that can identify mineral and chemical ingredients.
"The material from the drill could complicate, but will not prevent analysis of carbon content in rocks by one of the rover's 10 instruments. There are workarounds,” said John Grotzinger, the mission’s project scientist at the California Institute of Technology in Pasadena. "Organic carbon compounds in an environment are one prerequisite for life. We know meteorites deliver non-biological organic carbon to Mars, but not whether it persists near the surface. We will be checking for that and for other chemical and mineral clues about habitability."
Curiosity will be in good company as it nears landing. Two NASA Mars orbiters, along with a European Space Agency orbiter, will be in position to listen to radio transmissions as Mars Science Laboratory descends through Mars' atmosphere.
The mission is managed by JPL for NASA's Science Mission Directorate in Washington. Curiosity was designed, developed and assembled at JPL. Caltech manages JPL for NASA.
Follow the mission on Facebook and Twitter at:
http://www.facebook.com/marscuriosity
http://www.twitter.com/marscuriosity
For more information on the Mars Science Laboratory/Curiosity mission, visit:
http://www.nasa.gov/msl
NASA
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