domingo, 19 de abril de 2015

NASA : White Dwarf May Have Shredded Passing Planet .- Un planeta enano que puede hacer sido destrozado...

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibo información de la Agencia Espacial NASA, sobre el paso de un planeta enano que puede hacer sido destruido por un estrella enana, esto sucedió en el Cúmulo globular NGC 6388.
NASA, así lo describe: " En esta imagen de Chandra de NGC 6388, los investigadores han encontrado pruebas de que una estrella enana blanca puede haber desgarrado un planeta a medida que se acercaba demasiado. Cuando una estrella alcanza su etapa de enana blanca, casi todo el material de la estrella está lleno dentro de un radio de centésimas de que la estrella original.
La destrucción de un planeta puede sonar como algo de ciencia ficción, pero un equipo de astrónomos ha encontrado evidencia de que esto puede haber sucedido en un clúster antiguo de estrellas en el borde de la galaxia de la Vía Láctea.....

chandra ngc6388
In this Chandra image of ngc6388, researchers have found evidence that a white dwarf star may have ripped apart a planet as it came too close. When a star reaches its white dwarf stage, nearly all of the material from the star is packed inside a radius one hundredth that of the original star.
The destruction of a planet may sound like the stuff of science fiction, but a team of astronomers has found evidence that this may have happened in an ancient cluster of stars at the edge of the Milky Way galaxy.

Using several telescopes, including NASA’s Chandra X-ray Observatory, researchers have found evidence that a white dwarf star – the dense core of a star like the Sun that has run out of nuclear fuel – may have ripped apart a planet as it came too close.
Image Credit: NASA
Last Updated: April 19, 2015
Editor: Steve Fox
NASA
Guillermo Gonzalo Sánchez Achutegui
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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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NASA : NASA Awards Radiation Challenge Winners, Launches Next Round to Seek Ideas for Protecting Humans on the Journey to Mars .- NASA Premios radiación Ganadores del Concurso, lanzamientos Siguiente Ronda se debe buscar ideas para proteger a las personas en el viaje a Marte

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial  NASA, sobre el otorgamiento de premios, para investigadores que permiten diseñar modelos de artefactos y evitar la radiación solar.  NASA otorgó $ 12,000 a cinco ganadores de un desafío de mitigar la exposición a radiación en misiones de espacio profundo y puso en marcha un nuevo seguimiento en el desafío de identificar formas innovadoras de proteger a las tripulaciones en el viaje a Marte.

Illustration of heliosphere
This illustration depicts our heliosphere, showing the approximate locations of Voyager 1 and Voyager 2 spacecraft. Galactic cosmic rays originate outside the heliosphere and stream in uniformly from all directions.
Credits: NASA
 
NASA awarded $12,000 to five winners of a challenge to mitigate radiation exposure on deep space missions and launched a new follow-on challenge to identify innovative ways of protecting crews on the journey to Mars.
The follow-on challenge offers an award of up to $30,000 for design ideas to protect the crew on long-duration space missions. Anyone can participate in the challenge, which will be open Wednesday, April 29 through Monday, June 29, 2015.
"We are very impressed with the enthusiasm and sheer number of people from the public who showed interest in solving this very difficult problem for human space exploration,” said Steve Rader, deputy manager of the Center of Excellence for Collaborative Innovation. "We look forward to seeing what people will come up with in this next challenge to find the optimal configuration for these different protection approaches.”
Galactic cosmic rays (GCRs), high-energy radiation that originates outside the solar system are a major issue facing future space travelers venturing beyond low-Earth orbit. These charged particles permeate the universe and exposure to them is inevitable during space exploration. Because missions to Mars will require crews to remain beyond the protection of Earth’s magnetic field and atmosphere for approximately 500 days and potentially more than 1,000 days, learning how to protect human explorers from the effect of exposure to GCRs is a high priority.
While the five winners selected in the first challenge did not identify a solution that ultimately solves the problem of GCR risk to human crews, the first place idea did provide a novel approach to using and configuring known methods of protection to save substantial launch mass and lower launch costs over multiple missions. The other winning submissions all provided solid proposed configurations on known approaches and were supported with sound engineering and mathematics.
NASA received 136 submissions. The five selected winners are:
  • 1st place ($5,000): George Hitt, assistant professor of Physics and Nuclear Engineering at Khalifa University, United Arab Emirates, for his novel idea on reusing a shield that could be placed in a Mars Transfer Orbit.
  • 2nd Place ($3,000): Ian Gallon, retired researcher in electro-magnetics of Bridport, England, for his mathematical details on what it would take for an active radiation mitigation system to function well.
  • 3rd Place ($2,000): Olivier Loido, freelance engineer of Toulouse, France, for his concepts for a launch configuration and deploying an array of magnets.
  • 4th Place ($1,000 each): Markus Novak, recent graduate from Ohio State University of Dublin, Ohio, for his creation of safe areas through particle trajectory simulations, and Mikhail Petrichenkov of Russia for his concept of operations making use of NASA Storm Shelter work.
NASA’s goal is to identify key solutions that will reduce crew members’ total radiation dose from exposure to GCRs on long duration deep space missions by at least a factor of four.
In a continued effort to achieve that goal, the agency has developed a second challenge that asks the public for ideas on optimal configurations of active and passive solutions to provide crew members maximum protection. Active protection uses magnetic or electrostatic fields to deflect the harmful radiation, while passive protection uses material layering to shield the crew from the GCRs.
These challenges are managed by the Center of Excellence for Collaborative Innovation (CoECI). CoECI is a multi-center organization established at the request of the White House Office of Science and Technology Policy to advance NASA’s open innovation efforts and extend that expertise to other federal agencies. CoECI is directly supported by the Human Health and Performance Directorate at NASA’s Johnson Space Center in Houston. The challenges are hosted on the NASA Innovation Pavilion through its contract with InnoCentive, Inc.
To participate in the challenge beginning April 29, visit:
For additional information about the galactic cosmic ray challenges, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui
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NASA : Multi-Utility Technology Testbed Aircraft On the Runway .- Multi-Utility Tecnología Testbed avión en la pista

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido la información de la Agencia Espacial NASA, sobre The X-56A Multi-Utility Technology Testbed (MUTT), que es un pequeño avión a control remoto, cuya misión es investigar con alta tecnología, que la NASA, denomina : aeroservoelastic; para bajar costos y producir un diseño barato para múltiples misiones que se pueda emplearlo.

Small white test aircraft with eyes painted on it facing forward, while U.S. Air Force team member in uniform stands to the left
The X-56A Multi-Utility Technology Testbed (MUTT) is greeted on an Edwards Air Force Base runway by a U.S. Air Force Research Laboratory (AFRL) team member. NASA’s Armstrong Flight Research Center and the AFRL, along with participants from Langley Research Center and Glenn Research Center, and support from Lockheed Martin, are using the second X-56A (dubbed “Buckeye”) to check out aircraft systems, evaluate handling qualities, characterize and expand the airplane’s performance envelope, and verify pre-flight predictions regarding aircraft behavior. The 20-minute flight marked the beginning of a research effort designed to yield significant advances in aeroservoelastic technology using a low-cost, modular, remotely piloted aerial vehicle.
Image Credit: NASA/Ken Ulbrich
Last Updated: April 19, 2015
Editor: Sarah Loff
NASA
Guillermo Gonzalo Sánchez Achutegui
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NASA : SpaceX Launches NASA Cargo and Research To International Space Station.- NASA lanza CargoSpaceX y la investigación para la Estación Espacial Internacional

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, sobre el envío del SpaceX Falcon 9 rocket , que impulsa a la nave Dragón que lleva abastecimiento para la Estación Espacial Internacional y materiales de investigación para exploraciones robóticas para  las futuras misiones en Marte.
Liftoff of SpaceX rocket with spacecraft
The mission is the company's sixth cargo delivery flight to the station through NASA’s Commercial Resupply Services contract. Dragon's cargo will support approximately 40 of the more than 250 science and research investigations that will be performed during Expeditions 43 and 44, including numerous human research investigations for NASA astronaut Scott Kelly's one-year mission in space.
Image Credit: NASA/Kim Shiflett
Last Updated: April 19, 2015
Editor: Sarah Loff
NASA
Guillermo Gonzalo Sánchez Achutegui
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nsf.gov - National Science Foundation - Earth Day is on the horizon. But is 'greener' always better? .- Día de la Tierra está en el horizonte. Pero es más "verde" siempre mejor?

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Fundación Nacional de Ciencias de Los Estados Unidos, sobre los próximos acontecimientos sobre el Día de La tierra y ellos se hacen la pregunta "ser mas verde" es mejor?
Y ellos se contestan así: "Ir verde. En el Día de la Tierra y cada día, siendo más "verde" está vinculado con las cosas buenas, como la reducción de su huella de carbono y el consumo de alimentos cultivados localmente....... Pero no cuando se trata de beber o nadar en las brillantes aguas verdes del lago sucias por las algas, dice Hans Paerl, científico ambiental en la Universidad de Carolina del Norte en Chapel Hill.
En los lagos de agua dulce de todo el mundo, estas floraciones de algas suelen ser consecuencia de un exceso de lo que se conoce como las cianobacterias, o algas verde-azules......
Forma cianobacterias flores generalizadas, muy visibles que se parecen a pintura azul-verde o escoria que flota en el agua. Ellos pueden ser tóxicos para los seres humanos y otros animales.
Estas bacterias filamentosas se agrupan en las esteras que cubren la superficie de un lago de una orilla a la otra, con un máximo de oxígeno en el agua y, finalmente, convertir las profundidades lagos en una zona muerta....................."

More information....

Not when it's the bright green waters of algae-fouled lakes and rivers
Collage of images showing algae in alakes and researcher
View a photo gallery of algae blooms in lakes.
Credit and Larger Version
April 15, 2015
The following is part 15 in a series on the National Science Foundation's (NSF) Environmental Research and Education (ERE) programs. Parts one, two, three, four, five, six, seven, eight, nine, 10, 11, 12, 13 and 14 in this series are available on the NSF website.
Going green. On Earth Day and every day, being "greener" is linked with good things like lowering your carbon footprint and eating locally-grown foods.
But not when it comes to drinking or swimming in the bright green waters of lakes fouled by algae, says Hans Paerl, an environmental scientist at the University of North Carolina at Chapel Hill.
In freshwater lakes around the world, such algae blooms often result from an overabundance of what's known as cyanobacteria, or blue-green algae.
Cyanobacteria form widespread, very visible blooms that look like blue-green paint or scum floating on the water. They may be toxic to humans and other animals.
These filamentous bacteria clump into mats that cover a lake's surface from one shore to the other, using up oxygen in the water and eventually turning the lake's depths into a dead zone.
From Lake Taihu, China, to Lake Erie in the U.S.
It was June 2007, and water spouting from kitchen faucets in Wuxi, China, was pea-soup green. The water came from Taihu, China's third largest lake.
Cyanobacteria obscured the surface of the 900-square-mile lake and quickly overwhelmed the intake plant for the city of Wuxi's drinking water.
Chinese officials scooped 6,000 tons of algae from Taihu and diverted water from the Yangtze River to flush the lake. However, says Paerl, the bloom persisted. "It was fall when it finally abated."
Two weeks into the bloom, Paerl was in China, leaning over the side of a small boat to take samples of Taihu's scum.
He discovered that the algae is similar to that found in blooms in North Carolina's ponds, rivers and estuaries, and in many larger bodies of water such as Lake Erie, Lake Victoria and the Baltic Sea.
"Nowhere are the blooms worse than on Taihu, however," says Paerl, whose work is funded by an NSF Dimensions of Biodiversity grant. "Habitat for fish, crabs and other aquatic species is becoming endangered."
Ten million people also depend on Taihu for drinking water, fisheries and tourism.
Lake Erie on the border of the United States and Canada faces the same challenges.
In 2011, a record-breaking bloom of similar cyanobacteria to the species that plagued Taihu smothered Lake Erie, turning it a bright-green that showed up on satellite images.
At the bloom's peak in October, it expanded to more than 1,930 square miles, three times larger than any Lake Erie bloom on record.
New "recipe" for controlling algae blooms
The "recipe" for controlling the problem, says Paerl, "has been to reduce phosphorus finding its way into lakes from sources on land like fertilizers. That's based on the long-standing paradigm that phosphorus is the key nutrient limiting freshwater algae blooms."
But another element, nitrogen, flowing into lakes and rivers is increasing more rapidly than phosphorus. "It's led researchers to question whether both nitrogen and phosphorus should be controlled to stem the tide of proliferating algae blooms," says Paerl.
Lake Taihu, he says, is a "looking glass" for addressing such nutrient overenrichment and toxic algae blooms.
"Our NSF Dimensions of Biodiversity project is determining what roles specific nutrients like nitrogen and phosphorus play in the frequency and extent of algae blooms in lakes, and how they affect these ecosystems."
Data from experiments on the relationship between nutrients and algae blooms are being used to formulate a nutrient reduction management strategy. Scientists hope it will lead to the control of blooms in Taihu and other lakes.
The goal, Paerl says, is to find new ways of ensuring sustainable uses of lakes prone to blooms.
Other scientists involved in the research are Wayne Gardner of the University of Texas, Ferdi Hellweger of Northeastern University and Steven Wilhelm of the University of Tennessee.
"Harmful cyanobacteria blooms caused by excessive phosphorus and nitrogen are threatening freshwater lakes worldwide," says Simon Malcomber, lead NSF program director for Dimensions of Biodiversity, which is supported by NSF's Directorates for Biological Sciences and Geosciences.
"This research shows the importance of taking a holistic approach to understanding harmful cyanobacteria blooms," says Malcomber. "Only with an ecosystems approach can long-term successful sustainability strategies be formulated."
Chain of events links land and lake
The complex chain that leads to algae blooms in freshwater begins not in lakes but on land.
Farmers often overfertilize their fields. The excess fertilizer, laden with nutrients like phosphorus and nitrogen, washes into creeks and rivers, where it's eventually carried to lakes.
"Nitrogen is necessary for increasing crop yields," says Paerl, "but plants are inefficient at taking it up. More fertilizer is often added than plants need."
Only a fraction of the nitrogen applied to soils ends up in crops; in some regions, it's less than 20 percent. The rest is on the loose.
When the excess eventually reaches freshwater, it fertilizes aquatic algae such as cyanobacteria--just as it encourages plants on land to grow. The algae proliferate, becoming massive blooms.
As the algae die, they fall to the lake's bottom and are digested by microorganisms. The process removes oxygen from the water, creating low-oxygen "dead zones," fish kills and tainted waters.
Extreme algae blooms: The new normal?
Are algae blooms in lakes around the world a new normal?
Scientists are working to find answers.
"This important work is linking the diversity and identity of algae with nitrogen cycling and harmful algal blooms in heavily affected freshwater lakes," says Mike Sieracki, Dimensions of Biodiversity program director in NSF's Division of Ocean Sciences.
This week at an NSF-funded workshop--Global Solutions to Regional Problems: Collecting Global Expertise to Address the Problem of Harmful Algal Blooms--researchers discussed the current science on algae blooms, and identified knowledge gaps in bloom prevention and mitigation.
"We hope that this workshop will lead to strategies to mitigate future blooms in waterbodies in the U.S. and around the world," says Bill Cooper, program director in NSF's Division of Chemical, Bioengineering, Environmental and Transport Systems.
Meeting topics included the biology of bloom-forming species, environmental factors underlying bloom formation, sensor development in bloom detection, prediction of blooms, and best practices for control.
"New nutrient reduction strategies," wrote Paerl and colleagues in the journal Science in October 2014, "should incorporate point and non-point sources, including nitrogen removal in wastewaters, optimization of fertilizer application, and erosion controls.
"An investment in joint phosphorus and nitrogen controls will counter the very high costs of harmful algal bloom events and the losses of freshwater resources worldwide."
It's the only way, Paerl says, to keep blooms of cyanobacteria and other algae in check. When it comes to lakes and rivers, streams and ponds, "going green" means anything but.
-- Cheryl Dybas, NSF (703) 292-7734 cdybas@nsf.gov
Related Programs Dimensions of Biodiversity
Related WebsitesWhither the diversity of life on Earth? NSF, partners award $23 million for studies of planet's biodiversity: 
http://www.nsf.gov/news/news_summ.jsp?cntn_id=132506
Earth Week: A Stream Is a Stream Is a Stream: Or Is It?:
 http://www.nsf.gov/discoveries/disc_summ.jsp?cntn_id=123855&org=NSF
Staple of recipe favorites--the tomato--reveals processes that maintain biodiversity:
 http://nsf.gov/discoveries/disc_summ.jsp?cntn_id=129676
NSF Grant: Anthropogenic nutrient input drives genetic, functional and taxonomic biodiversity in hypereutrophic Lake Taihu, China:

A toxic algae bloom, one of many around the world, covers North Carolina's Cape Fear River.
Credit and Larger Version
China's Lake Taihu, showing an extensive algae bloom that reaches the lake's shores.
China's Lake Taihu shows an extensive algae bloom that reaches the lake's shores.
Credit and Larger Version
boat going through Lake Taihu's thick algae scum.
Researchers travel by boat through Lake Taihu's thick algae scum.
Credit and Larger Version
Scientist Hans Paerl holding a bottle with algae in water from in Lake Taihu.
Scientist Hans Paerl collects samples of the algae bloom in Lake Taihu.
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Satellite view of a widespread algae bloom in September 2013, in Lake Erie.
Satellite view of a widespread algae bloom in September 2013, in Lake Erie.
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the National Science Foundation(NSF)
Guillermo Gonzalo Sánchez Achutegui
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NASA : Solar Arrays on the International Space Station .- Paneles solares en la Estación Espacial Internacional

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido de la Agencia Espacial NASA, la información sobre los paneles solares que están instalados en la Estación Espacial Internacional, que generan la energía eléctrica. Paneles solares de la Estación Espacial contienen un total de 262.400 células solares y cubren un área de cerca de 27.000 pies cuadrados (2.500 metros cuadrados) - más de la mitad de la superficie de un campo de fútbol. Envergadura de un panel solar de 240 pies (73 metros) es más largo que la envergadura de un Boeing 777, que es de 212 pies (65 metros). En total, los cuatro conjuntos de matrices pueden generar 84-120 kilovatios de electricidad - suficiente para proporcionar electricidad a más de 40 viviendas. Los paneles solares producen más energía que la estación necesita de una sola vez para sistemas de estación y experimentos. Cuando la estación se encuentra en la luz del sol, alrededor del 60 por ciento de la electricidad que los paneles solares generan se utiliza para cargar las baterías de la estación. A veces, algunos o todos de los paneles solares están en la sombra de la Tierra o la sombra de la parte de la estación. Esto significa que esos arreglos no están recogiendo la luz del sol. Las baterías de energía de la estación suplen la energía cuando no está en el sol.


Giant solar arrays with Earth below at left of frame
Expedition 43 Flight Engineer Samantha Cristoforetti of the European Space Agency (ESA) photographed the giant solar arrays on the International Space Station on Feb. 12, 2015.
 
The space station's solar arrays contain a total of 262,400 solar cells and cover an area of about 27,000 square feet (2,500 square meters) -- more than half the area of a football field. A solar array's wingspan of 240 feet (73 meters) is longer than a Boeing 777's wingspan, which is 212 feet (65 meters). Altogether, the four sets of arrays can generate 84 to 120 kilowatts of electricity -- enough to provide power to more than 40 homes. The solar arrays produce more power than the station needs at one time for station systems and experiments. When the station is in sunlight, about 60 percent of the electricity that the solar arrays generate is used to charge the station's batteries. At times, some or all of the solar arrays are in the shadow of Earth or the shadow of part of the station. This means that those arrays are not collecting sunlight. The batteries power the station when it is not in the sun.
Image Credit: ESA/NASA
Last Updated: April 19, 2015
Editor: Sarah Loff
NASA
Guillermo Gonzalo Sánchez Achutegui
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NASA : Layers and Dark Dunes on the Surface of Mars .- Capas y dunas oscuras en la superficie de Marte

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, sobre sus investigaciones en Marte, sobre capas y dunas oscuras sobre la superficie de Marte, justamente  el : NASA's Mars Reconnaissance Orbiter (MRO) por medio del : the High Resolution Imaging Science Experiment (HiRISE), tuvieron como  el objetivo de esta observación es una depresión circular en una unidad de tono oscuro asociada a un campo de conos al noreste. En la escala de una imagen tomada por la cámara OPF Contexto, que ofrece amplias vistas de la zona para proporcionar un contexto para el análisis de alta resolución, la depresión aparece para exponer capas especialmente en los lados o paredes, que están cubierta por arena oscura presumiblemente asociados a la oscuridad unidad -toned. La resolución de la cámara HiRISE, que es mucho mayor que la de la Cámara de contexto y su mayor huella, puede ayudar a identificar posibles capas.

Circular depression in flat Mars surface with smaller crater indentations on right
This image of a circular depression on the surface of Mars was acquired on Jan. 5, 2015 by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter (MRO). The spacecraft has been orbiting Mars since March 2006 and completed its 40,000th orbit around Mars on Feb. 7, 2015.
 
The target of this observation is a circular depression in a dark-toned unit associated with a field of cones to the northeast. At the scale of an image taken by MRO's Context Camera, which provides wide area views to provide context for high-resolution analysis, the depression appears to expose layers especially on the sides or walls, which are overlain by dark sands presumably associated with the dark-toned unit. The HiRISE camera's resolution, which is far higher than that of the Context Camera and its larger footprint, can help identify possible layers.
HiRISE is one of six instruments on the 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 Project for NASA's Science Mission Directorate, Washington.
Image Credit: NASA/JPL-Caltech/University of Arizona
Caption: HiRISE Science Team
Last Updated: April 19, 2015
Editor: Sarah Loff
NASA
Guillermo Gonzalo Sánchez Achutegui
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NASA : The Mercury Astronauts .- Astronautas del Proyecto Mercury

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido una información de la Agencia Espacial NASA, sobre el Proyecto Mercurio, que consistió en Project Mercury  el 9 de abril del 1,959, se hizo el primer compromiso importante de la NASA. Los objetivos del programa eran para colocar una nave espacial para personas, en órbita alrededor de la Tierra, observar el desempeño de los astronautas en tales condiciones y segura recuperar el astronauta y la nave espacial. Los vuelos Mercury probó que los seres humanos podrían vivir y trabajar en el espacio, y allanó el camino para los programas Gemini y Apollo, así como para todos los vuelos espaciales tripulados más,

Original Mercury astronauts stand in group for photo in front of spacecraft
On April 9, 1959, NASA's first administrator, Dr. Keith Glennan, announced the names of the agency's first group of astronauts at a news conference in Washington, D.C. Now known as the "Original Seven," they included three Naval aviators, M. Scott Carpenter, Walter M. Schirra Jr., and Alan B. Shepard Jr.; three Air Force pilots, L. Gordon Cooper Jr., Virgil I. (Gus) Grissom, and Donald K. (Deke) Slayton; along with Marine Corps aviator John H. Glenn Jr. This group photo of the original Mercury astronauts was taken in June 1963 at the Manned Spacecraft Center (MSC), now Johnson Space Center, in Houston, Texas. The astronauts are, left-to-right: Cooper, Schirra, Shepard, Grissom, Glenn, Slayton and Carpenter.
 
Project Mercury became NASA's first major undertaking. The objectives of the program were to place a human-rated spacecraft into orbit around Earth, observe the astronaut's performance in such conditions and safely recover the astronaut and the spacecraft. The Mercury flights proved that humans could live and work in space, and paved the way for the Gemini and Apollo programs as well as for all further human spaceflight.
Image Credit: NASA
Last Updated: April 19, 2015
Editor: Sarah Lof
Tags:  Mercury, NASA History,
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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NASA : The Solar System and Beyond is Awash in Water .- El Sistema Solar y más allá está inundado de agua

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido la información de la Agencia Espacial NASA, quien nos dice que el Sistema Solar y allende el espacio está inundado de agua. NASA, nos dice: Como misiones de la NASA a explorar nuestro sistema solar y la búsqueda de nuevos mundos, que están encontrando agua en lugares sorprendentes. El agua no es más que una pieza de nuestra búsqueda de planetas habitables y la vida fuera de la Tierra, sin embargo, que vincula muchas palabras aparentemente no relacionadas de manera sorprendente.
"Las actividades de ciencia de la NASA han proporcionado una ola de descubrimientos asombrosos relacionados con el agua en los últimos años que nos inspiran a seguir investigando los orígenes y las fascinantes posibilidades de otros mundos, y la vida en el universo", dijo Ellen Stofan, jefe científico de la agencia . "En nuestra vida, podemos muy bien finalmente responder si estamos solos en el sistema solar y más allá."

Artist's concept of our universe
NASA is exploring our solar system and beyond to understand the workings of the universe, searching for water and life among the stars
Credits: NASA
As NASA missions explore our solar system and search for new worlds, they are finding water in surprising places. Water is but one piece of our search for habitable planets and life beyond Earth, yet it links many seemingly unrelated worlds in surprising ways.
"NASA science activities have provided a wave of amazing findings related to water in recent years that inspire us to continue investigating our origins and the fascinating possibilities for other worlds, and life, in the universe," said Ellen Stofan, chief scientist for the agency. "In our lifetime, we may very well finally answer whether we are alone in the solar system and beyond."
 
La Tierra no es el único mundo océano en nuestro sistema solar. Los océanos podrían existir en diversas formas en las lunas y planetas enanos, ofrecer pistas a la búsqueda para descubrir la vida más allá de nuestro planeta. Esta ilustración representa a los candidatos más conocidos en nuestra búsqueda de vida en el sistema solar.
 
This illustration depicts the best-known candidates in our search for life in the solar system
Earth isn't the only ocean world in our solar system. Oceans could exist in diverse forms on moons and dwarf planets, offering clues in the quest to discover life beyond our home planet. This illustration depicts the best known candidates in our search for life in the solar system.
 
 
 
 
Credits: NASA/JPL-Caltech
 
 
 
The chemical elements in water, hydrogen and oxygen, are some of the most abundant elements in the universe. Astronomers see the signature of water in giant molecular clouds between the stars, in disks of material that represent newborn planetary systems, and in the atmospheres of giant planets orbiting other stars.
There are several worlds thought to possess liquid water beneath their surfaces, and many more that have water in the form of ice or vapor. Water is found in primitive bodies like comets and asteroids, and dwarf planets like Ceres. The atmospheres and interiors of the four giant planets -- Jupiter, Saturn, Uranus and Neptune -- are thought to contain enormous quantities of the wet stuff, and their moons and rings have substantial water ice.
Perhaps the most surprising water worlds are the five icy moons of Jupiter and Saturn that show strong evidence of oceans beneath their surfaces: Ganymede, Europa and Callisto at Jupiter, and Enceladus and Titan at Saturn.
Scientists using NASA's Hubble Space Telescope recently provided powerful evidence that Ganymede has a saltwater, sub-surface ocean, likely sandwiched between two layers of ice.
Europa and Enceladus are thought to have an ocean of liquid water beneath their surface in contact with mineral-rich rock, and may have the three ingredients needed for life as we know it: liquid water, essential chemical elements for biological processes, and sources of energy that could be used by living things. NASA's Cassini mission has revealed Enceladus as an active world of icy geysers. Recent research suggests it may have hydrothermal activity on its ocean floor, an environment potentially suitable for living organisms.
NASA spacecraft have also found signs of water in permanently shadowed craters on Mercury and our moon, which hold a record of icy impacts across the ages like cryogenic keepsakes.
While our solar system may seem drenched in some places, others seem to have lost large amounts of water.
On Mars, NASA spacecraft have found clear evidence that the Red Planet had water on its surface for long periods in the distant past. NASA's Curiosity Mars Rover discovered an ancient streambed that existed amidst conditions favorable for life as we know it.
More recently, NASA scientists using ground-based telescopes were able to estimate the amount of water Mars has lost over the eons. They concluded the planet once had enough liquid water to form an ocean occupying almost half of Mars' northern hemisphere, in some regions reaching depths greater than a mile (1.6 kilometers). But where did the water go?
It's clear some of it is in the Martian polar ice caps and below the surface. We also think much of Mars' early atmosphere was stripped away by the wind of charged particles that streams from the sun, causing the planet to dry out. NASA's MAVEN mission is hard at work following this lead from its orbit around Mars.
The story of how Mars dried out is intimately connected to how the Red Planet's atmosphere interacts with the solar wind. Data from the agency's solar missions -- including STEREO, Solar Dynamics Observatory and the planned Solar Probe Plus -- are vital to helping us better understand what happened.
Understanding the distribution of water in our solar system tells us a great deal about how the planets, moons, comets and other bodies formed 4.5 billion years ago from the disk of gas and dust that surrounded our sun. The space closer to the sun was hotter and drier than the space farther from the sun, which was cold enough for water to condense. The dividing line, called the "frost line," sat around Jupiter's present-day orbit. Even today, this is the approximate distance from the sun at which the ice on most comets begins to melt and become "active." Their brilliant spray releases water ice, vapor, dust and other chemicals, which are thought to form the bedrock of most worlds of the frigid outer solar system.
Scientists think it was too hot in the solar system's early days for water to condense into liquid or ice on the inner planets, so it had to be delivered -- possibly by comets and water-bearing asteroids. NASA's Dawn mission is currently studying Ceres, which is the largest body in the asteroid belt between Mars and Jupiter. Researchers think Ceres might have a water-rich composition similar to some of the bodies that brought water to the three rocky, inner planets, including Earth.
The amount of water in the giant planet Jupiter holds a critical missing piece to the puzzle of our solar system's formation. Jupiter was likely the first planet to form, and it contains most of the material that wasn't incorporated into the sun. The leading theories about its formation rest on the amount of water the planet soaked up. To help solve this mystery, NASA's Juno mission will measure this important quantity beginning in mid-2016.
Looking further afield, observing other planetary systems as they form is like getting a glimpse of our own solar system's baby pictures, and water is a big part of that story. For example, NASA's Spitzer Space Telescope has observed signs of a hail of water-rich comets raining down on a young solar system, much like the bombardment planets in our solar system endured in their youth.
With the study of exoplanets -- planets that orbit other stars -- we are closer than ever to finding out if other water-rich worlds like ours exist. In fact, our basic concept of what makes planets suitable for life is closely tied to water: Every star has a habitable zone, or a range of distances around it in which temperatures are neither too hot nor too cold for liquid water to exist. NASA's planet-hunting Kepler mission was designed with this in mind. Kepler looks for planets in the habitable zone around many types of stars.
Recently verifying its thousandth exoplanet, Kepler data confirm that the most common planet sizes are worlds just slightly larger than Earth. Astronomers think many of those worlds could be entirely covered by deep oceans. Kepler's successor, K2, continues to watch for dips in starlight to uncover new worlds.
The agency's upcoming TESS mission will search nearby, bright stars in the solar neighborhood for Earth- and super-Earth-sized exoplanets. Some of the planets TESS discovers may have water, and NASA's next great space observatory, the James Webb Space Telescope, will examine the atmospheres of those special worlds in great detail.
It's easy to forget that the story of Earth's water, from gentle rains to raging rivers, is intimately connected to the larger story of our solar system and beyond. But our water came from somewhere -- every world in our solar system got its water from the same shared source. So it's worth considering that the next glass of water you drink could easily have been part of a comet, or an ocean moon, or a long-vanished sea on the surface of Mars. And note that the night sky may be full of exoplanets formed by similar processes to our home world, where gentle waves wash against the shores of alien seas.
For more information about NASA's exploration of the solar system and beyond, visit:
Preston Dyches
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-7013
preston.dyches@jpl.nasa.gov
 
Felicia Chou
NASA Headquarters, Washington
202-358-0257
Felicia.chou@nasa.gov
2015-119
NASA
Guillermo Gonzalo Sánchez Achutegui
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miércoles, 15 de abril de 2015

NASA : NASA Joins Forces to Put Satellite Eyes on Threat to U.S. Freshwater .- NASA une fuerzas para poner Satélite, comolos ojos qe vigilen ante amenaza para los Estados Unidos de su agua dulce

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, sobre el temor que siente Los Estados Unidos de América de un envenenamiento de su agua dulce por algas.
La NASA ha unido fuerzas con la Agencia de Protección Ambiental, Administración Nacional Oceánica y Atmosférica, y el Servicio Geológico de Estados Unidos para transformar los datos de satélite diseñado para investigar la biología del océano en información que ayudará a proteger al público estadounidense de las floraciones de algas nocivas agua dulce.

Lake Erie algal blooms
Toxic algal blooms like this one in Lake Erie in 2011 can cause human and animal health risks, fish kills, and degrade drinking water supplies.
Image Credit: 
USGS/NASA Earth Observatory
NASA has joined forces with the U.S. Environmental Protection Agency, National Oceanic and Atmospheric Administration, and U.S. Geological Survey to transform satellite data designed to probe ocean biology into information that will help protect the American public from harmful freshwater algal blooms.
Algal blooms are a worldwide environmental problem causing human and animal health risks, fish kills, and taste and odor in drinking water. In the United States, the cost of freshwater degraded by harmful algal blooms is estimated at $64 million annually. In August 2014, officials in Toledo, Ohio, banned the use of drinking water supplied to more than 400,000 residents after it was contaminated by an algal bloom in Lake Erie.
The new $3.6 million, multi-agency effort will use ocean color satellite data to develop an early warning indicator for toxic and nuisance algal blooms in freshwater systems and an information distribution system to aid expedient public health advisories.
“The vantage point of space not only contributes to a better understanding of our home planet, it helps improve lives around the world,” said NASA Administrator Charles Bolden. “We’re excited to be putting NASA’s expertise in space and scientific exploration to work protecting public health and safety.”
Ocean color satellite data from NASA’s Aqua, the USGS-NASA Landsat, and the European Space Agency’s Sentinel-2 and -3 are currently available to scientists, but are not routinely processed and produced in formats that help state and local environmental and water quality managers. Through this project, satellite data on harmful algal blooms developed by the partner agencies will be converted to a format that stakeholders can use through mobile devices and web portals.
“Observations from space-based instruments are an ideal way to tackle this type of public health hazard because of their global coverage and ability to provide detailed information on material in the water, including algal blooms,” said Paula Bontempi of the Earth Science Division at NASA Headquarters in Washington.
NOAA and NASA pioneered the use of satellite data to monitor and forecast harmful algal blooms. Satellites allow for more frequent observations over broader areas than water sampling. The satellite data support NOAA’s existing forecasting systems in the Gulf of Mexico and Great Lakes.
“Observing harmful algae is critical to understanding, managing, and forecasting these blooms,” said Holly Bamford, acting NOAA assistant secretary for conservation and management and deputy administrator in Washington. “This collaboration will assure that NOAA’s efforts will assist the coastal and inland public health officials and managers across the country to distribute this information to the community in an easily understandable fashion, making them more resilient to environmental events.”
The new network builds on previous NASA ocean satellite sensor technologies created to study the global ocean’s microscopic algal communities, which play a major role in ocean ecology, the movement of carbon dioxide between the atmosphere and ocean, and climate change. These sensors detect the color of the sunlit upper layer of the ocean and are used to create indicators that can help identify harmful algal blooms.
Under certain environmental conditions, algae naturally present in marine and fresh waters rapidly multiply to create a bloom. Some species of algae called cyanobacteria produce toxins that can kill wildlife and domestic animals and cause illness in humans through exposure to contaminated freshwater and the consumption of contaminated drinking water, fish or shellfish. Cyanobacteria blooms are a particular concern because of their dense biomass, toxins, taste and odor.
“EPA researchers are developing important scientific tools to help local communities respond quickly and efficiently to real-time water quality issues and protect drinking water for their residents,” said EPA Administrator Gina McCarthy. “Working with other federal agencies, we are leveraging our scientific expertise, technology and data to create a mobile app to help water quality managers make important decisions to reduce negative impacts related to harmful algal blooms, which have been increasingly affecting our water bodies due to climate change.”
The project also includes a research component to improve understanding of the environmental causes and health impacts of cyanobacteria and phytoplankton blooms across the United States. Blooms in lakes and estuaries are produced when aquatic plants receive excess nutrients under suitable environmental conditions. Various land uses, such as urbanization and agricultural practices, change the amount of nutrients and sediment delivered in watersheds, which can influence cyanobacterial growth.
Researchers will compare the new freshwater algal blooms data with satellite records of land cover changes over time to identify specific land-use activities that may have caused environmental changes linked to the frequency and intensity of blooms. The results will help to develop better forecasts of bloom events.
NASA uses the vantage point of space to increase our understanding of our home planet, improve lives, and safeguard our future. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term satellite data records. The agency freely shares this unique knowledge and works with institutions around the world to gain new insights into how our planet is changing.
For more information on NASA’s Earth science activities, visit:
 
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Guillermo Gonzalo Sánchez Achutegui
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NASA : NASA Extends Campaign for Public to Name Features on Pluto .- NASA extiende la Campaña para público a nombre satélite que orbita en Plutón

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, que el satélite : NASA’s New Horizons spacecraft, ha descubierto un satélite que orbita alrededor de Plutón y la Agencia desea la participación del Público para poner un nombre a este nuevo descubrimiento.
Como sabemos que La Unión Astronómica Internacional (UAI) con sede en París, es la única en poner nombres a los diferentes cuerpos celestes que se encuentran en El Universo, pero esta vez se pide la participación del público en general y llegar a un consenso en nombrar al nuevo satélite que orbita alrededor de Plutón.
New Horizons spacecraft as it approaches Pluto and it's largest moon, Charon
Artist’s concept of NASA’s New Horizons spacecraft as it passes Pluto and Pluto’s largest moon, Charon, in July 2015.
Image Credit: 
NASA/JHU APL/SwRI/Steve Gribben
The public has until Friday, April 24 to help name new features on Pluto and its orbiting satellites as they are discovered by NASA’s New Horizons mission.
Announced in March, the agency wants to give the worldwide public more time to participate in the agency’s mission to Pluto that will make the first-ever close flyby of the dwarf planet on July 14.
The campaign extension, in partnership with the International Astronomical Union (IAU) in Paris, was due to the overwhelming response from the public.
“Due to increasing interest and the number of submissions we’re getting, it was clear we needed to extend this public outreach activity,” said Jim Green, director of NASA’s Planetary Science Division at the agency’s headquarters in Washington. “This campaign not only reveals the public’s excitement about the mission, but helps the team, which will not have time to come up with names during the flyby, to have a ready-made library of names in advance to officially submit to the IAU.”
The IAU is the formal authority for naming celestial bodies. Submissions must follow a set of accepted themes and guidelines set out by the IAU’s Working Group for Planetary System Nomenclature. After the campaign concludes, NASA’s New Horizons team will sort through the names and submit its recommendations to the IAU. The IAU will decide whether and how the names will be used.
The campaign allows the public of all ages to submit names for the many new features scientists expect to discover on Pluto following the encounter.
"I’m impressed with the more than 40,000 thoughtful submissions,” said Mark Showalter, scientist New Horizons science team co-investigator, and SETI Institute in Mountain View, California, which is hosting the naming website. “Every day brings new lessons in the world's history, literature and mythology. Participation has come from nearly every country on Earth, so this really is a worldwide campaign.”
New Horizons already has covered more than 3 billion miles since it launched on Jan. 19, 2006. Its journey has taken it past each planet’s orbit, from Mars to Neptune, in record time, and now it’s in the first stage of an historic encounter with Pluto that includes long-distance imaging, as well as dust, energetic particle and solar wind measurements to characterize the space environment near Pluto.
The spacecraft will pass Pluto at a speed of 31,000 mph taking thousands of images and making a wide range of science observations. At a distance of nearly 4 billion miles from Earth at flyby, it will take approximately 4.5 hours for data to reach Earth.
The Johns Hopkins Applied Physics Laboratory (APL) manages the New Horizons mission for NASA’s Science Mission Directorate in Washington. Alan Stern, of the Southwest Research Institute (SwRI), is the principal investigator. SwRI leads the science team, payload operations and encounter science planning. New Horizons is part of the New Frontiers Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. APL designed, built and operates the spacecraft for NASA.
To find out more information about how to participate in the Pluto naming contest, visit:
Detailed IAU guidelines for acceptable names submissions are available online at:
For images and updates on the July 14 Pluto flyby, visit:
and
Dwayne Brown
Headquarters, Washington
202-358-1726
dwayne.c.brown@nasa.gov
Lars Lindberg Christensen
IAU Press Officer
Garching bei München, Germany
+49 89 320 06 761, cell: +49 173 38 72 621
lars@eso.org
NASA
Guillermo Gonzalo Sánchez Achutegui
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