domingo, 15 de marzo de 2015

NASA : New NASA Mission to Study Ocean Color, Airborne Particles and Clouds .- Nueva Misión NASA’s PACE spacecraft para estudiar Océano color, partículas y las nubes

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido de la Agencia Espacial NASA, la información que su nave  NASA’s PACE spacecraft estudiará el color de los Océanos, las partículas aerotransportadas y las nubes de la Tierra.
Global ocean color observations from data gathered by NASA’s PACE spacecraft
New measurements by NASA’s PACE spacecraft will advance our understanding of how living marine resources respond to a changing climate. NASA pioneered the field of global ocean color observations with the SeaWIFS satellite sensor from 1997 to 2010.
Image Credit: 
NASA
NASA is beginning work on a new satellite mission that will extend critical climate measurements of Earth’s oceans and atmosphere and advance studies of the impact of environmental changes on ocean health, fisheries and the carbon cycle.
 
Tentatively scheduled to launch in 2022, the Pre-Aerosol Clouds and ocean Ecosystem (PACE) mission will study Earth’s aquatic ecology and chemistry, and address the uncertainty in our understanding of how clouds and small airborne particles called aerosols affect Earth’s climate. PACE will be managed by NASA's Goddard Space Flight Center in Greenbelt, Maryland.
“Knowing more about global phytoplankton community composition will help us understand how living marine resources respond to a changing climate,” said Jeremy Werdell, PACE project scientist at Goddard. “With PACE, we will learn more about the role of marine phytoplankton in the global carbon cycle.”
NASA has long used satellites to observe the global ocean’s microscopic algal communities, which play a significant role in the ocean’s ecology and the global carbon cycle. PACE will provide a global view of the planet's microscopic ocean algae called phytoplankton. Phytoplankton live in the sunlit upper layer of the ocean, producing at least half of the oxygen on Earth and form the base of the marine food chain.
Goddard will build PACE’s ocean color instrument. This PACE sensor will allow scientists to see the colors of the ocean, from the ultraviolet to near infrared, and obtain more accurate measurements of biological and chemical ocean properties, such as phytoplankton biomass and the composition of phytoplankton communities. These changes in the ocean’s color help identify harmful algal blooms.
Quantifying phytoplankton is essential for understanding the carbon cycle and tracking climate variability and change. The ocean absorbs atmospheric carbon dioxide into solution at the sea surface. Like land plants, phytoplankton use carbon dioxide to create their organic biomass via photosynthesis. Phytoplankton vary greatly in their size, function, and response to environmental and ecosystem changes or stresses such as ocean acidification.
Dissolved carbon dioxide also reacts with seawater and alters its acidity. About one fourth of human-made carbon dioxide ends up in the ocean.
"NASA Goddard pioneered ocean color remote sensing 35 years ago with the very first satellite observations, and the Center has been committed to supporting the science ever since," said Piers Sellers, deputy director of NASA Goddard Earth Science. "Goddard scientists play a critical role in generating and improving core satellite data sets for the international ocean biology community. We look forward to extending this important record into the future with PACE."
In addition to gathering data on ocean color, PACE will measure clouds and tiny airborne particles like dust, smoke and aerosols in the atmosphere to supplement measurements from existing NASA satellite missions. These measurements are critical for understanding the flow of natural and human made aerosols in the environment. Aerosols affect how energy moves in and out of Earth’s atmosphere directly by scattering sunlight, and indirectly by changing the composition of clouds. Aerosols also can affect the formation of precipitation in clouds and change rainfall patterns.
The blend of atmospheric and oceanic observations from PACE is critical as ocean biology is affected by aerosols deposited onto the ocean, which in turn, produce aerosol precursors that influence atmospheric composition and climate. NASA is currently planning a second PACE instrument, a polarimeter, to better measure aerosol and cloud properties. These measurements will improve understanding of the roles of aerosols in the climate system.
Goddard's proof-of-concept sensor for measuring ocean color — the Coastal Zone Color Scanner that flew on the Nimbus-7 satellite from 1978 to 1986 — was the first sensor to demonstrate phytoplankton biomass could be quantified from space. The Sea-Viewing Wide Field-of-View Sensor or SeaWiFS mission collected data from 1997 to 2010 and was the first mission dedicated to routinely observe ocean biology, chemistry, and ecology for long-term climate research. Currently, researchers employ the Moderate Resolution Imaging Spectroradiometer that flies aboard both NASA’s Terra and Aqua spacecraft, and the Visible Infrared Imager Radiometer Suite aboard the NASA-NOAA Suomi National Polar-orbiting Partnership satellite, to measure biological and chemical properties of the ocean, as well as aerosol and cloud properties.
NASA capped the costs for PACE at $805 million, to cover the spacecraft, mission design and engineering, science, instruments, launch vehicle, data processing, and operations.
For more information about PACE, visit:
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 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:
NASA
Guillermo Gonzalo Sánchez Achutegui
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La Casa de la Loma tiene un Fantasma: Capítulo CCXCIX.- Horacio aplicando la experiencia acumulada logra dominar al último torete, que trató de embestirlo y fue salvado por el caballo negro...

Hola amigos: A VUELO DE UN QUINDE EL BLOG., continuando con la historia de La Casa de la Loma tiene un Fantasma, y como informamos en el capítulo anterior; Horacio Manchay estaba empeñado en un entrenamiento de doblegar toretes ariscos, era un desafío que se practicaba en Ambasal, que justamente con motivo de la Celebración de la Festividad Religiosa, ofrecida honor a San José de Ambasal, y como desarrollo de la fiesta había competencias de lacear y doblegar toretes ariscos desde la montura de un caballo; reto para este tipo de competencia, para Horacio era la oportunidad para competir junto o contra Natalia "ojos verdes" quien era una joven hacendada ecuatoriana, soltera y tomó una fuerte curiosidad en conocer al Primo  de Jurupe, que le había mencionado su amiga Adelaida. Horacio, estaba luchando contra el último torete, y éste animal al sentirse sujetado por la veta(cuerda) dio la vuelta y trató de embestir; por escasos milímetros escaparon Horacio y Adelaida, aún así el torete logró enlazar su asta con la blusa de la espalda de Adelaida.

Aquí en la imagen observamos una típica casa en la Comunidad Campesina de Socchabamba, Ayabaca, Piura, Perú; es una construcción de adobe con techo de tejas rojas y a dos aguas, sobre el techo distinguimos un fantasma que viene a ser el "El Rey de las Tinieblas" : Satanás, seguido de vampiros y una siniestra sombra negra que rodea al misterioso personaje satánico, para comprender la narrativa de la obra literaria: "LA CASA DE LA LOMA TIENE UN FANTASMA" , esta imagen será nuestro símbolo de identificación y el logotipo en creación, impresión y distribución literaria. Con reconocimiento de derechos de autor, con Partida Registral Nº 00393-2010, Asiento 01, con fecha 27 de marzo de 2010 por INDICOPI.
Este es el símbolo de Marca Perú, que distingue para todos los productos elaborados por peruanos.

Estamos llegando a las 17:00 horas del día, en Pacainio se encontraban Horacio y Adelaida, escapando a la embestida  del último torete; el animal fue laceado por Horacio, y tratando de sujetarlo por que pretendía escapar hacia la Quebrada Grande; huida que no le iban a permitir ni Horacio, menos Adelaida.
Horacio desde la montura de su caballo negro logró lacearlo, pero la fuerza descomunal del torete, tuvo que apearse y con la ayuda de Adelaida, detuvieron al torete, y éste animal no quería que nadie le obstaculice su huida;  retrocedió y trató de embestirlos en forma sorpresiva, quienes apenas tuvieron tiempo de escapar, aún así una asta cogió cogió la blusa por la espalda de Adelaida.
El torete trató de levantar por los aires el cuerpo de Adelaida, pero felizmente la blusa se rasgó y el asta quedó libre y como ellos huían cuesta arriba, el torete perdió terreno, quedándose rezagado por escasos centímetros de los cuerpos huidizos.
Pero, el torete no se daba por vencido, luego de un ligero resbalón, emprendió la subida por la pendiente del terreno, siguiendo sus planes de ataque, pero los jóvenes le sacaron ventaja y desde arriba Horacio, espantaba al torete dándole fuerte gritos que paralice la subida del animal, pero no entendía estaba demasiado agresivo.
Entonces, el caballo "negro" como le llamaba Horacio; intuyó y vio los graves peligros y aprietos que estaba padeciendo su amo; y con el hocico mordió la punta del otro extremo de la veta y haló hacia abajo con tanta fuerza que detuvo al torete y lo hizo tambalear y finalmente cayó cuesta abajo con la parte trasera si control y rodó un trecho, pero el torete reaccionó y se reincorporó y la emprendió contra el caballo que lo había doblegado.
El noble equino, sabía que estaba expuesto a merced del ataque del torete, si continuaba corriendo cuesta abajo; entonces soltó la veta y dio un viraje hacia arriba y haciendo tremendo esfuerzo  galopó hacia donde estaba su amo.
En cambio el torete que no pensaba, solo actuaba por instinto, aplicando la fuerza bruta no pude detener su brusca bajada y se fue con todo su cuerpo hacia la pequeña pampa( explanada); estando allí comenzó a raspar la tierra con las patas delanteras(manos), levantando polvo de tierra y mugía en forma agresiva; los cuatro restante toretes se reincorporaron y se unieron al quisquilloso;  hermano haciendo causa común vacuna.
Horacio, miró a Adelaida y telepáticamente se comunicaron en bajar hasta la misma pampa(explanada) y halar la veta que sostenía al díscolo torete, montó su caballo negro y cabalgó tan rápido como pudo, al llegar se apeó cogiendo el extremo de la punta de la veta y montó de nuevo para acercarse y de alguna manera meterse entre ellos saltar  a la nunca  del torete.
Entonces, los cinco toretes se juntaron tratando de huir del jinete que se venía contra ellos y haciendo una jugada casi suicida, se acercó al torete laceado y logró aflojar el botón que sostenía la penca de la veta aflojándose y se soltó la veta el cuello del torete quedando libre.
El animal que no razonaba, pero si actuaba por instinto, viéndose libre, paró en seco su huida hacia adelante , y retrocedió el cuerpo hacia atrás jugada que adivinó Horacio y dirigió su caballo hacia arriba, justo lo que esperaba el torete, quien como cazador, emprendió cuesta arriba para atacar al jinete montado que constituía su "presa".
Horacio, con la experiencia acumulada por los otros cuatro toretes, detuvo la subida y dio vuelta a su caballo y lo hizo tan rápido  que casi pierde el equilibrio el noble equino. Y sin saber a donde lo llevaba su amo, obedeció al movimiento de las riendas del jinete que también actuaba por instinto y cerebro; le tendió una trampa al torete, dirigió su caballo alejándose del torete, luego comenzó a bajar en forma diagonal hacia la derecha; el torete no pudo entender la jugada de su víctima y levantando la cola en señal de  ataque, siguió al jinete y cuando se acercaba, Horacio quitó el cuerpo hacia arriba, el pesado cuerpo del torete no pudo controlar su impulso y siguió torpemente hacia adelante en falso.
Entonces, Horacio quien  hábilmente dirigió su caballo, se le presentó la única oportunidad de doblegar al agresivo torete; guió de nuevo hacia abajo a  su caballo y aplicó espuelas hasta aproximarse al descontrolado cuerpo del torete y cuando lo tuvo a su alcance, soltó saltando de la montura y logró caer a la altura de la nuca del torete  y se aferró en las astas y el torete soportando mucho peso sobre su cabeza la bajó y sus patas delanteras se enredaron entre ellas  y perdió el equilibrio cayendo de bruces, soportando todo el peso de su cuerpo más el de Horacio y al caer la cabeza chocó contra el suelo y el cuello soportó el esfuerzo y peso;  que por poco se tuerce y no se produjo justamente por que indirectamente el cuerpo de Horacio le sirvió como cuña; impidiendo una muerte segura por rompimiento del cuello( en Socchabamba se llama desnucado por el rompimiento de la nuca, también le llaman rodado, por que una de las astas se introduce en el suelo y por el peso del cuerpo al caer de costado se rompe todos los huesos de la nuca).
El torete completamente agotado y con un asta introducida parcialmente en el terreno, fue doblegado fácilmente por Horacio, que se dio el lujo de  colocar el lazo de su veta a las astas del torete, sin que éste reaccione; el jinete rápidamente se levantó y elevó las dos brazos en señal de triunfo; que no se hizo esperar la felicitación de Adelaida, quien abrazó amorosamente al primo, diciéndole:
--- Primo Horacio, tu serás el próximo hacendado de la Hacienda  "Loma Fértil"  de Macará, estás dotado de : Coraje, arrojo, habilidad para domar y actitud para triunfar, creo que con esas "amorosas armas" conquistarás el corazón de Natalia "ojos verdes".
Ambos primos, festejaron las ocurrentes expresiones, cuyas palabras promisorias, retumbaron en la hoyada de Quebrada Grande.
Luego retiraron la veta del último torete, los arriaron hacia la Quebrada Grande para que retornen al potrero de donde se salieron, ahorrándole el trabajo a Hilario y sus peones que desconociendo por completo la ubicación de los toretes, los cinco regresaban y se toparían con sus seguidores.
Siendo aproximadamente las 18:00 horas del día (6:00 de la tarde) era la "Hora de la Oración", muy pesada en algunos lugares, por que los espíritus malignos afloraban desde el interior de la tierra a acosar a los humanos......
Continuaremos...................
Guillermo Gonzalo Sánchez Achutegui
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La Historia del Amor Cruel : Capítulo CXC.- Sobeida logra que Feder vaya a la cárcel, pero se encuentra con Pamela y ésta decide apoyar a Feder...

Hola amigos: A VUELO DE UN QUINDE EL BLOG., continuando con La Historia del Amor Cruel entre Iarma y Olzagon y como informamos en el capítulo anterior, Federico (Feder) fue apresado por la policía francesa a pedido del Fiscal, por los cargos de jurar en falso; que según la legislación es Perjurio,  que bajo la Comunidad Francesa es intolerable; además, le sumarán cargos por falta de respeto e insulto a las Autoridades, asimismo habrá más cargos por haber insultado de prostituta a Sobeida, la Comunidad le brindará un Abogado de Oficio y el Fiscal le aplicó 45 días de prisión preventiva en una Cárcel de Alta Seguridad, hasta que se le prepare la Carpeta Judicial, e invitaron a Sobeida a la Fiscalía para los tramites  para sustentar los cargos en contra Feder....


Aquí en la imagen observamos una típica representación de la terrible situación que muchos hogares atraviesan en el transcurso de existencia por que siempre hay la existencia de un tercer elemento (amante tanto para él como para ella) que como una tentación tenebrosa carcomen la consistencia del matrimonio, y más si los esposos viven solamente la apariencia y no la triste realidad de que no son felices. Fuente: Archivos del blog. Obra Literaria reconocida con Derecho de Autor, según Partida Registral No. 00855-2012, Asiento: 01; con fecha: 10 de Agosto de 2012, por : INDECOPI.
Este es el símbolo de Marca Perú, que distingue para todos los productos elaborados por peruanos.
Pamela, seguía caminando y haciendo turismo por el Boulevard; pero no borraba de su mente el Hostal "El descanso Eterno" quiso entrar y en la puerta desistió; pero esta vez no pudo con su curiosidad y desde aproximadamente 15 cuadras del lugar, decidió regresar al hostal e ingresar para conocerlo.
Pamela, aceleró la marcha de regreso caminando aceleradamente y pronto llegó y observó a la altura de la puerta, automóviles oficiales: Patrullero Policial, automóvil  de la Fiscalía; automóvil de la Municipalidad, y en el preciso instante que ella subía el primer peldaño de la escalera por la puerta de ingreso al Hostal.
Esta puerta se abría saliendo un policía y un detenido, y que sorpresa era "Feder" quien con las manos esposadas hacia atrás; ella al verlo sintió escalofríos en todo su cuerpo, por el estupor que le produjo al verlo demacrado y preso. Feder, intentó ocultar su rostro, pero adónde, si ni siquiera sus manos estaban libres; él estaba solo, bajó la atormentada cabeza humillado y como pasaba a escasos centímetros de su persona. Pamela, le preguntó:
--- Feder: ¿Qué haz hecho?
Feder, muy humillado, le contestó:
--- Sobeida me acusó de secuestro a un grupo de su familia y la Policía aceptó la falsa denuncia, y por eso me llevan preso a la cárcel.
Pamela, muy sorprendida de lo que veían sus ojos, borró por un momento el odio que sentía por él,  y le dio lástima verlo preso, junto a un fornido policía, quien le empujaba a subir al automóvil policial y alcanzó hacerle la última pregunta:
--- No entiendo nada, si ya deberías estar volando al País de Cunante, seguramente haz cometido un grave delito,  para que la Policía te haya apresado.
Feder ya no pudo contestar el policía cerró la puerta y partió a su destino.
Entonces, Pamela aumentó su curiosidad y esta vez entró al Hostal y otra sorpresa, en ese momento salían don Javier, Elías y Sobeida, con quienes tenía una lejana amistad por pertenecer al mismo círculo social que ella frecuentaba, se acercó a saludarlos y dijo:
--- Pero, que sorpresa, estoy viendo a la familia completa ¿Cómo están?
Sobeida tomó la iniciativa de contestar el saludo de la familia y le contestó:
--- Hola Pamela, que sorpresa encontrarte en este Hostal, no sabía que te habían alojado aquí;  nosotros ya nos vamos al país de Cunante y dime: ¿Cómo te ha tratado París?
Pamela, seguía sorprendida y la respuesta la contestó con otra pregunta:
--- Acabo de ver preso a Federico, y por lo poco que conversé, me dijo que tu lo haz denunciado por secuestro; como él es aún mi novio, te hago la pregunta: ¿ a Quién de ustedes o de tu familia había secuestrado Feder?
Sobeida, que en ese momento se encontraba muy ofuscada, por que no contaba con la presencia de Pamela, a quien no estimaba, pero si la soportaba por ser de su vínculo social, le contestó:
--- Federico, me humilló y también a toda mi familia, al compromiso de "Pedida de mano", al no asistir ni siquiera dio alguna explicación de su lamentable ausencia y en aquel día, toda mi familia estaba reunida en mi casa para celebrar mi próximo matrimonio con Federico: te aclaro que  yo nunca supe que él, también era tu novio.
Pamela, al escuchar la explicación, le desaparició  la compasión que en principio sintió por Feder y le enervó la sangre y mostrando su coraje ante la traición, le dijo:
--- Sobeida, ahora somos dos mujeres, que hemos caído en las garras de éste individuo, si bien conmigo no ha habido un compromiso formal, si tenemos como 10 años que salimos y como tu bien me conoces no me gusta ser sojuzgada por ningún hombre, por esa razón nunca lo presenté en Sociedad como mi enamorado; pero desde hace unos 4 años adelante, existe más frecuencia en nuestras salidas, y dime : ¿Cómo fue el chasco de tu deshonra con Feder?
Sobeida, una vez más entendió que estaba conversando con la persona equivocada y mordiéndose los labios para no explotar de cólera que sentía, le contestó:
--- Por favor Pamela, mide bien tus palabras, yo nunca fui deshonrada, por que jamás entregué mi cuerpo, fuimos novios manteniendo el respeto hasta el matrimonio; pero faltó a su compromiso cuando iba a pedirme; nunca se presentó.
Pamela, se rió a carcajada suelta, por que le causó tanta gracia estar conversando con una mojigata puritana, quien según ella, todavía no sabía nada del sexo salvaje que tanto le gustaba a Feder y ella lo complacía en todo lo que él deseaba... pensó para sus adentros: "con razón nunca se presentó a pedir su mano a una mojigata anticuada"
Entonces, muy enojada Sobeida, agregó:
--- No se que te causó tanta gracia, creo que hablé bien claro mi posición.
Pamela, sosteniendo un poco sus carcajadas, le contestó así :
--- Mi querida Sobeida, tal como eres quizá ningún hombre irá a tu casa a pedirte que case contigo, por que tu vives tiempos de la Edad Media, donde se practicaba la Virginidad que hasta la practicaban y conservaban con candados, Federico es un hombre fogoso y practicante del amor libre y creo que en sus planes no existe la Palabra Matrimonio para él; en mi particular caso, él si me pidió que me casara con él, y yo lo desprecié, por que  yo nunca creo que el matrimonio sirva para hacer feliz a un hombre en la cama.....
Sobeida, una mujer practicante religiosa y apegada a las buenas costumbres familiares no podía seguir escuchando; tanta blasfemia para sus oídos de una lasciva mujer y le contestó:
--- Pamela, eres un satán caminando y " Nunca Haz sido santo de mi devoción", no tengo nada más que conversar contigo y si tanto te gusta Federico, visítalo en la cárcel, que es el lugar que le corresponde por patán, y me retiro, adiós amiga Pamela....
En efecto Sobeida y su familia salieron del Hostal, dejando en el interior a Pamela, quien fue testigo de los graves apuros que estaba pasando Federico y de nuevo tuvo compasión por él,  y más por amor propio por que la insultó Sobeida, decidió visitar a Feder y ver como lo puede ayudar para sacarlo de la prisión.
De primera intención, hizo un esfuerzo mas mental de olvidar lo malcriado que se portó contra ella por haberla abandonado en el hotel y al mismo tiempo pasó por su mente: No darle el gusto a Sobeida que nunca la apreció como una amiga y ella era la causante del apresamiento de Feder y dijo en sus pensamientos: "Bruja virginal vas a pagar muy caro haber ofendido a Federico al convertirlo en un vulgar delincuente en París"..................
Continuaremos.................
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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NASA : NASA's MMS Spacecraft Launches on an Atlas V Rocket .- Atlas V Rocket lanza MMS Las naves espaciales de la NASA

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, sobre el lanzamiento de sus naves NASA’s MMS misión - MMS, impulsadas por el cohete : The United Launch Alliance Atlas V rocket.
NASA, nos dice : " El cohete United Launch Alliance Atlas V con la nave espacial de la NASA Magnetosférica Multiescala (MMS) lanza a bordo de la Estación de Lanzamiento Espacial de la Fuerza Aérea de Cabo Cañaveral Complejo 41, Jueves, 12 de marzo 2015, Florida. Misión MMS de la NASA estudia el misterio de cómo los campos magnéticos alrededor de la Tierra a conectar y desconectar, liberando energía en forma explosiva a través de un proceso conocido como reconexión magnética. MMS consta de cuatro naves espaciales idénticas que trabajan juntos para proporcionar la primera vista tridimensional de este proceso fundamental, que se produce en todo el universo....."

More information...

NASA's MMS Spacecraft Launches on an Atlas V Rocket
The United Launch Alliance Atlas V rocket with NASA’s Magnetospheric Multiscale (MMS) spacecraft onboard launches from the Cape Canaveral Air Force Station Space Launch Complex 41, Thursday, March 12, 2015, Florida. NASA’s MMS mission studies the mystery of how magnetic fields around Earth connect and disconnect, explosively releasing energy via a process known as magnetic reconnection. MMS consists of four identical spacecraft that work together to provide the first three-dimensional view of this fundamental process, which occurs throughout the universe.
Image Credit: NASA/Aubrey Gemignani
NASA

NASA Spacecraft in Earth’s Orbit, Preparing to Study Magnetic Reconnection

NASA's MMS lifts off atop Atlas V
The United Launch Alliance Atlas V rocket with NASA’s Magnetospheric Multiscale (MMS) spacecraft onboard launches from the Cape Canaveral Air Force Station Space Launch Complex 41, Thursday, March 12, 2015, Florida.
Image Credit: 
NASA
Following a successful launch at 10:44 p.m. EDT Thursday, NASA’s four Magnetospheric Multiscale (MMS) spacecraft are positioned in Earth’s orbit to begin the first space mission dedicated to the study of a phenomenon called magnetic reconnection. This process is thought to be the catalyst for some of the most powerful explosions in our solar system.
The spacecraft, positioned one on top of the other on a United Launch Alliance Atlas V 421 rocket, launched from Cape Canaveral Air Force Station, Florida. After reaching orbit, each spacecraft deployed from the rocket’s upper stage sequentially, in five-minute increments, beginning at 12:16 a.m. Friday, with the last separation occurring at 12:31 a.m. NASA scientists and engineers were able to confirm the health of all separated spacecraft at 12:40 a.m.
"I am speaking for the entire MMS team when I say we’re thrilled to see all four of our spacecraft have deployed and data indicates we have a healthy fleet,” said Craig Tooley, project manager at NASA's Goddard Space Flight Center in Greenbelt, Maryland.
Atlas V with MMS Spacecraft Takes Flight
As an Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station in the background, the launch can also be seen on the countdown clock at the Kennedy Space Center's Press Site. The rocket is carrying NASA's Magnetospheric Multiscale, or MMS, spacecraft.
Image Credit: 
NASA/Frankie Martin
Over the next several weeks, NASA scientists and engineers will deploy booms and antennas on the spacecraft, and test all instruments. The observatories will later be placed into a pyramid formation in preparation for science observations, which are expected to begin in early September.
“After a decade of planning and engineering, the science team is ready to go to work,” said Jim Burch, principal investigator for the MMS instrument suite science team at the Southwest Research Institute in San Antonio (SwRI). “We’ve never had this type of opportunity to study this fundamental process in such detail.”
The mission will provide the first three-dimensional views of reconnection occurring in Earth's protective magnetic space environment, the magnetosphere. Magnetic reconnection occurs when magnetic fields connect, disconnect, and reconfigure explosively, releasing bursts of energy that can reach the order of billions of megatons of trinitrotoluene (commonly known as TNT). These explosions can send particles surging through space near the speed of light.
Scientists expect the mission will not only help them better understand magnetic reconnection, but also will provide insight into these powerful events, which can disrupt modern technological systems such as communications networks, GPS navigation, and electrical power grids.
By studying reconnection in this local, natural laboratory, scientists can understand the process elsewhere, such as in the atmosphere of the sun and other stars, in the vicinity of black holes and neutron stars, and at the boundary between our solar system's heliosphere and interstellar space.
artist's concept of the MMS observatory fleet with rainbow magnetic lines
Artist's concept of the MMS observatory fleet with rainbow magnetic lines.
Image Credit: 
NASA
The spacecraft will fly in a tight formation through regions of reconnection activity. Using sensors designed to measure the space environment at rates100 times faster than any previous mission.
“MMS is a crucial next step in advancing the science of magnetic reconnection – and no mission has ever observed this fundamental process with such detail,” said Jeff Newmark, interim director for NASA’s Heliophysics Division at the agency’s Headquarters in Washington. “The depth and detail of our knowledge is going to grow by leaps and bounds, in ways that no one can yet predict.”
MMS is the fourth mission in the NASA Solar Terrestrial Probes Program. Goddard built, integrated and tested the four MMS spacecraft and is responsible for overall mission management and operations. The principal investigator for the MMS instrument suite science team is based at the SwRI. Science operations planning and instrument commanding are performed at the MMS Science Operations Center at the University of Colorado Boulder’s Laboratory for Atmospheric and Space Physics. 


 
More information about the MMS mission is available at:
 
 
Launch of Magnetospheric Multiscale Spacecraft Aboard Atlas V Rocket
The United Launch Alliance Atlas V rocket with NASA’s Magnetospheric Multiscale (MMS) spacecraft onboard launches from the Cape Canaveral Air Force Station Space Launch Complex 41, Thursday, March 12, 2015, Florida. NASA’s MMS mission studies the mystery of how magnetic fields around Earth connect and disconnect, explosively releasing energy via a process known as magnetic reconnection. MMS consists of four identical spacecraft that work together to provide the first three-dimensional view of this fundamental process, which occurs throughout the universe.
Photo Credit: NASA/Aubrey Gemignani
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NASA : NASA’s Hubble Observations Suggest Underground Ocean on Jupiter's Largest Moon .- Las observaciones del Telescopio Espacial Hubble de la NASA Sugiera la existencia de océano subterraneo en Gaminedes, el más grande satélite de Júpiter

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido de la Agencia Espacial NASA, la información que el Telescopio Espacial Hubble, ha captado información sobre la existencia de un Océano Subterráneo en Ganímedes que bien a ser el satélite más grande del Planeta Júpiter.
NASA, nos dice : " Telescopio Espacial Hubble de la NASA tiene la mejor evidencia hasta ahora de un océano de agua salada subterránea en Ganímedes, la luna más grande de Júpiter. El océano subterráneo se cree que tiene más agua que toda el agua en la superficie de la Tierra...."

More information....

Artist concept of Ganymede and Jupiter
In this artist’s concept, the moon Ganymede orbits the giant planet Jupiter. NASA’s Hubble Space Telescope observed aurorae on the moon generated by Ganymede’s magnetic fields. A saline ocean under the moon’s icy crust best explains shifting in the auroral belts measured by Hubble.
Image Credit: 
NASA/ESA
NASA’s Hubble Space Telescope has the best evidence yet for an underground saltwater ocean on Ganymede, Jupiter’s largest moon. The subterranean ocean is thought to have more water than all the water on Earth's surface.
Identifying liquid water is crucial in the search for habitable worlds beyond Earth and for the search of life as we know it.
“This discovery marks a significant milestone, highlighting what only Hubble can accomplish,” said John Grunsfeld, associate administrator of NASA’s Science Mission Directorate at NASA Headquarters, Washington. “In its 25 years in orbit, Hubble has made many scientific discoveries in our own solar system. A deep ocean under the icy crust of Ganymede opens up further exciting possibilities for life beyond Earth.”
Ganymede is the largest moon in our solar system and the only moon with its own magnetic field. The magnetic field causes aurorae, which are ribbons of glowing, hot electrified gas, in regions circling the north and south poles of the moon. Because Ganymede is close to Jupiter, it is also embedded in Jupiter’s magnetic field. When Jupiter’s magnetic field changes, the aurorae on Ganymede also change, “rocking” back and forth.
By watching the rocking motion of the two aurorae, scientists were able to determine that a large amount of saltwater exists beneath Ganymede’s crust affecting its magnetic field.
Hubble telescope image of Ganymede auroral belts
NASA Hubble Space Telescope images of Ganymede's auroral belts (colored blue in this illustration) are overlaid on a Galileo orbiter image of the moon. The amount of rocking of the moon's magnetic field suggests that the moon has a subsurface saltwater ocean.
Image Credit: 
NASA/ESA
A team of scientists led by Joachim Saur of the University of Cologne in Germany came up with the idea of using Hubble to learn more about the inside of the moon.
"I was always brainstorming how we could use a telescope in other ways," said Saur. "Is there a way you could use a telescope to look inside a planetary body? Then I thought, the aurorae! Because aurorae are controlled by the magnetic field, if you observe the aurorae in an appropriate way, you learn something about the magnetic field. If you know the magnetic field, then you know something about the moon’s interior."
If a saltwater ocean were present, Jupiter’s magnetic field would create a secondary magnetic field in the ocean that would counter Jupiter’s field. This “magnetic friction” would suppress the rocking of the aurorae. This ocean fights Jupiter's magnetic field so strongly that it reduces the rocking of the aurorae to 2 degrees, instead of the 6 degrees, if the ocean was not present.
Scientists estimate the ocean is 60 miles (100 kilometers) thick – 10 times deeper than Earth's oceans – and is buried under a 95-mile (150-kilometer) crust of mostly ice.
Scientists first suspected an ocean in Ganymede in the 1970s, based on models of the large moon. NASA's Galileo mission measured Ganymede's magnetic field in 2002, providing the first evidence supporting those suspicions. The Galileo spacecraft took brief "snapshot" measurements of the magnetic field in 20-minute intervals, but its observations were too brief to distinctly catch the cyclical rocking of the ocean’s secondary magnetic field.
The new observations were done in ultraviolet light and could only be accomplished with a space telescope high above the Earth's atmosphere, which blocks most ultraviolet light.
NASA’s Hubble Space Telescope is celebrating 25 years of groundbreaking science on April 24. It has transformed our understanding of our solar system and beyond, and helped us find our place among the stars. To join the conversation about 25 years of Hubble discoveries, use the hashtag #Hubble25.
Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, Inc., in Washington.
For images and more information about Hubble, visit:
and
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Guillermo Gonzalo Sánchez Achutegui
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NASA : NASA's Space Launch System Booster Passes Major Ground Test.- Lanzamiento Espacial de la NASA System Booster Pasa la prueba de tierra Major

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido de la Agencia Espacial NASA, la información que su:  NASA System Booster, pasó la prueba en efectuada en "Tierra Mayor".
NASA, nos dice: "El más grande, más poderoso cohete jamás construido encendió miércoles para una prueba de tierra; constituyendo un  importante hito en la preparación para futuras misiones para ayudar a impulsar el cohete de la NASA Espacial Launch System (SLS) y la nave espacial Orion a destinos del espacio profundo, incluyendo un asteroide y Marte fue todo un  éxito.

For more information read below attached ....

Space Launch System rocket booster test
At the Orbital ATK test facility, the booster for NASA’s Space Launch System rocket was fired for a two minute test on March 11. The test is one of two that will qualify the booster for flight before SLS begins carrying NASA’s Orion spacecraft and other potential payloads to deep space destinations.
Image Credit: 
NASA
The largest, most powerful rocket booster ever built successfully fired up Wednesday for a major-milestone ground test in preparation for future missions to help propel NASA’s Space Launch System (SLS) rocket and Orion spacecraft to deep space destinations, including an asteroid and Mars.
The booster fired for two minutes, the same amount of time it will fire when it lifts the SLS off the launch pad, and produced about 3.6 million pounds of thrust. The test was conducted at the Promontory, Utah test facility of commercial partner Orbital ATK, and is one of two tests planned to qualify the booster for flight. Once qualified, the flight booster hardware will be ready for shipment to NASA’s Kennedy Space Center in Florida for the first SLS flight.
"The work being done around the country today to build SLS is laying a solid foundation for future exploration missions, and these missions will enable us to pioneer far into the solar system," said William Gerstenmaier, NASA’s associate administrator for human exploration and operations. "The teams are doing tremendous work to develop what will be a national asset for human exploration and potential science missions."
It took months to heat the 1.6 million pound booster to 90 degrees Fahrenheit to verify its performance at the highest end of the booster’s accepted propellant temperature range. A cold-temperature test, at a target of 40 degrees Fahrenheit, the low end of the propellant temperature range, is planned for early 2016. These two tests will provide a full range of data for analytical models that inform how the booster performs. During the test, temperatures inside the booster reached more than 5,600 degrees.
"This test is a significant milestone for SLS and follows years of development," said Todd May, SLS program manager. "Our partnership with Orbital ATK and more than 500 suppliers across the country is keeping us on the path to building the most powerful rocket in the world."
During the test, more than 531 instrumentation channels on the booster were measured to help assess some 102 design objectives. The test also demonstrated the booster meets applicable ballistic performance requirements, such as thrust and pressure. Other objectives included data gathering on vital motor upgrades, such as the new internal motor insulation and liner and an improved nozzle design.
When completed, two five-segment boosters and four RS-25 main engines will power the SLS on deep space missions. The 177-feet-long solid rocket boosters operate in parallel with the main engines for the first two minutes of flight. They provide more than 75 percent of the thrust needed for the rocket to escape the gravitational pull of the Earth.
The first flight test of SLS will be configured for a 70-metric-ton (77-ton) lift capacity and carry an uncrewed Orion spacecraft beyond low-Earth orbit to test the performance of the integrated system. The SLS will later be configured to provide an unprecedented lift capability of 130 metric tons (143 tons) to enable missions farther into our solar system.
For more information on SLS, visit:
 

  • Test Firing of Booster for NASA's New Rocket
    The largest, most powerful rocket booster ever built successfully fired up Wednesday for a major-milestone ground test in preparation for future missions to help propel NASA’s Space Launch System (SLS) rocket and Orion spacecraft to deep space destinations, including an asteroid and Mars.
    The booster fired for two minutes, the same amount of time it will fire when it lifts the SLS off the launch pad, and produced about 3.6 million pounds of thrust. The test was conducted at the Promontory, Utah test facility of commercial partner Orbital ATK, and is one of two tests planned to qualify the booster for flight. Once qualified, the flight booster hardware will be ready for shipment to NASA’s Kennedy Space Center in Florida for the first SLS flight.
    Image Credit: Orbital ATK
     
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    Guillermo Gonzalo Sánchez Achutegui
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    NASA : Future Space Station Crew to Participate in NASA TV Briefing, Media Interviews .- Futura Expedición que participará en NASA TV Briefing, para entrevistas con los medios de comunicación....

    Hola amigos: A VUELO DE QUINDE EL BLOG., hemos recibido de la Agencia Espacial NASA, la información sobre la futura expedición de astronautas y cosmonautas que harán uso de NASA TV Briefing, para conceder entrevistas a los medios, desde la Estación Espacial Internacional  y ellos son: NASA astronaut Kjell Lindgren, Oleg Kononenko of the Russian Federal Space Agency and Kimiya Yui of the Japan Aerospace Exploration Agency.
    ISS Expedition 44 crew
    NASA astronaut Kjell Lindgren, Oleg Kononenko of the Russian Federal Space Agency and Kimiya Yui of the Japan Aerospace Exploration Agency launch May 26 to the International Space Station to join Expedition 44.
    Image Credit: 
    NASA/Stephanie Stoll
    NASA Astronaut Kjell Lindgren, part of the crew that’s scheduled to launch to the International Space Station in May, will take part in a NASA Television news conference and media interviews Wednesday, March 18, at the agency's Johnson Space Center in Houston.
    Lindgren, cosmonaut Oleg Kononenko of the Russian Federal Space Agency (Roscosmos) and Kimiya Yui of the Japan Aerospace Exploration Agency will launch to the space station aboard a Soyuz TMA-17M spacecraft May 26 from the Baikonur Cosmodrome in Kazakhstan to round out the Expedition 44 crew. The trio will return to Earth in November as part of the Expedition 45 crew.
    The news conference with the crew members will air live on NASA TV at 2 p.m. EDT. B-roll video of the crew will air beginning at 1:30 p.m. Reporters who wish to participate by telephone should call Johnson's newsroom at 281-483-5111 no later than 1:50 p.m. Those following the briefing on social media can ask questions using the hashtag #askNASA.
    After the news conference, interview opportunities are available in person or by phone. To request credentials to attend in person or to reserve an interview opportunity, media must contact Johnson's newsroom by 6 p.m. Monday, March 16.
    Board certified in emergency and aerospace medicine, Lindgren is a graduate of the U.S. Air Force Academy and Colorado State University. He was a member of the academy’s “Wings of Blue” parachute team. Lindgren received his medical degree from the University of Colorado. Lindgren began at Johnson Space Center as a flight surgeon before being selected as an astronaut in 2009.
    The Expedition 44 crew members will share their flight experiences on Instagram at:
     
    To follow Lindgren on Twitter, visit:
     
    For Lindgren’s full biography, visit:
     
    For NASA TV streaming video, schedule and downlink information, visit:
    For more information about the International Space Station and its crews, visit:
    NASA
    Guillermo Gonzalo SánchezAchutegui
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    viernes, 13 de marzo de 2015

    NASA : Expedition 42 Soyuz Landing

    Hola amigos: A VUELO DE UN QUINDE EL BLOG., la Agencia Espacial NASA, nos informa del retorno a La Tierra desde la Estación Espacial Internacional de los astronautas:Astronaut Barry Wilmore,Flight Engineer Alexander Samokutyaev,Flight Engineer Elena Serova, que conformaron la Expedición 42, y lo hicieron a bordo de la Nave : The Soyuz TMA-14M spacecraft; ellos permanecieron 167 días en el espacio.


    Expedition 42 Returns to Earth
     
    The Soyuz TMA-14M spacecraft is seen as it lands with International Space Station Expedition 42 commander Barry Wilmore of NASA, Alexander Samokutyaev of the Russian Federal Space Agency (Roscosmos) and Elena Serova of Roscosmos near the town of Zhezkazgan, Kazakhstan. The landing took place on the evening of Wednesday, March 11 in the U.S, and early in the morning on Thursday, March 12, in Kazakhstan.
    The three crew members returned to Earth after a 167-day mission on the orbital outpost that included hundreds of scientific experiments and several spacewalks to prepare the orbiting laboratory for future arrivals by U.S. commercial crew spacecraft.
    Credit: NASA/Bill Ingall
    Expedition 42 Soyuz Landing
    The Soyuz TMA-14M spacecraft is seen as it lands with Expedition 42 commander Barry Wilmore of NASA, Alexander Samokutyaev of the Russian Federal Space Agency (Roscosmos) and Elena Serova of Roscosmos near the town of Dzhezkazgan, Kazakhstan on Wednesday, March 11, 2015 (Thursday, March 12, Kazakh time). NASA astronaut Wilmore, Russian cosmonauts Samokutyaev and Serova returned to Earth after almost six months onboard the International Space Station where they served as members of the Expedition 41 and 42 crews. The spacecraft touched down safely at approximately 10:07 p.m. EDT.
    Image Credit: NASA/Bill Ingalls
     
     
    Space Station Crew Returns to Earth, Lands Safely in Kazakhstan
    From Russian command and control
    ЕСТЬ ПОСАДКА! They have landed! This message was posted to the center screen of the Russian Federal Space Agency's Mission Control Center in Korolev, Russia, the moment confirmation was received that the Soyuz carrying three crew members of the International Space Station's Expedition 42 had landed on time and target in Kazakhstan.
    Image Credit: 
    NASA
    Three crew members returned to Earth Wednesday after a 167-day mission on the International Space Station (ISS) that included hundreds of scientific experiments and several spacewalks to prepare the orbiting laboratory for future arrivals by U.S. commercial crew spacecraft.
     
    Expedition 42 commander Barry Wilmore of NASA and flight engineers Alexander Samokutyaev and Elena Serova of the Russian Federal Space Agency (Roscosmos) touched down at approximately 10:07 p.m. EDT (8:07 a.m. March 12, Kazakh time) southeast of the remote town of Dzhezkazgan in Kazakhstan.
    Expedition 42 commander Barry Wilmore of NASA
    Expedition 42 commander Barry Wilmore of NASA makes his way out of the Soyuz spacecraft following the crew's 167-day mission aboard the space station.
    Image Credit: 
    NASA
    During their time on station, the crew members participated in a variety of research focusing on the effects of microgravity on cells, Earth observation, physical science and biological and molecular science. One of several key research focus areas during Expedition 42 was human health management for long-duration space travel, as NASA and Roscosmos prepare for two crew members to spend one year aboard the space station.
    Expedition 42 flight engineer Elena Serova
    Her first mission to the space station, Expedition 42 flight engineer Elena Serova of the Russian Federal Space Agency is assisted in her exit from the Soyuz that returned her and her team members from the ISS.
    Image Credit: 
    NASA
    The space station also serves as a test bed to demonstrate new technology. The Cloud-Aerosol Transport System (CATS) arrived and was installed during Expedition 42, and already is providing data to improve scientists’ understanding of the structure and evolution of Earth's atmosphere. This may lead to enhancements to spacecraft launches, landings and communications systems; help guide future atmospheric investigations of Mars, Jupiter or other worlds; and help researchers model and predict climate changes on Earth.
    flight engineer Alexander Samokutyaev of the Russian Federal Space Agency
    With the end of this mission, flight engineer Alexander Samokutyaev of the Russian Federal Space Agency now has accrued 331 days in space.
    Image Credit: 
    NASA
    The newly installed Electromagnetic Levitator will allow scientists to observe fundamental physical processes as liquid metals cool, potentially leading to lighter, higher-performing alloy, mixtures of two or more metals or a metal and another material, for use on Earth and in space.
     
    The station crew also welcomed three cargo spacecraft with several tons of scientific investigations, food, fuel and other supplies. In January, the trio helped grapple and connect a SpaceX Dragon spacecraft on the company's fifth contracted commercial resupply mission to the station. The Dragon returned to Earth in February with critical science samples. Two Russian ISS Progress cargo craft docked to the station in October and February. The fifth and final European Automated Transfer Vehicle, bearing the name of Belgian physicist Georges Lemaître, considered the father of the big-bang theory, departed the station in February.
     
    During his time on the orbital complex, Wilmore ventured outside the space station with NASA astronaut Terry Virts on three spacewalks to prepare for new international docking adapters and future U.S. commercial crew spacecraft. Wilmore also completed a spacewalk in October with fellow NASA astronaut Reid Wiseman to replace a failed voltage regulator. Samokutyaev conducted one spacewalk during his time in space.
     
    Having completed his second space station mission, Samokutyaev now has spent 331 days in space. Wilmore, having previously flown as a shuttle pilot on STS-129, has spent 178 days in space. Serova spent 167 days in space on her first flight.
     
    Expedition 43 currently is operating the station, with Virts in command. Flight engineers Anton Shkaplerov of Roscosmos and Samantha Cristoforetti of ESA (European Space Agency), are continuing station research and operations until three new crewmates arrive in two weeks. NASA’s Scott Kelly and Roscosmos’ Mikhail Kornienko and Gennady Padalka are scheduled to launch from Kazakhstan March 27, Eastern time. Kelly and Kornienko will embark on the first joint U.S.-Russian one-year mission, an important stepping stone on NASA’s journey to Mars.
     
    For more information about the International Space Station and its crews, visit:
     
     
    For b-roll and other media resources, visit:
     
     
    Follow the station on Twitter at @Space_Station
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    Guillermo Gonzalo Sánchez Achutegui
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    NASA : Spacecraft Data Suggest Saturn Moon's Ocean May Harbor Hydrothermal Activity

    Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido de la Agencia Espacial NASA, la información de un satélite Encelado  de Saturno muestra actividad hidrotermal tal como sucede en La Tierra : Nave espacial Cassini de la NASA ha proporcionado a los científicos la primera evidencia clara de que la luna de Saturno Encelado muestra signos de actividad hidrotermal actual que pueden parecerse a la observada en los océanos profundos de la Tierra. Las implicaciones de tal actividad en un mundo distinto del nuestro planeta abren posibilidades científicos sin precedentes.
    NASA nos dice: "Estos resultados se suman a la posibilidad de que Encelado, que contiene un océano bajo la superficie y muestra actividad geológica notable, podría contener los entornos adecuados para los organismos vivos", dijo John Grunsfeld astronauta y administrador asociado del Directorio de Misiones Científicas de la NASA en Washington. "Los lugares de nuestro sistema solar, donde se producen los ambientes extremos en que la vida pudiera existir puede acercarnos más a responder a la pregunta: ¿Estamos solos en el Universo."
    NASA, agrega : "
    "Estos resultados se suman a la posibilidad de que Encelado, que contiene un océano bajo la superficie y muestra actividad geológica notable, podría contener los entornos adecuados para los organismos vivos", dijo John Grunsfeld astronauta y administrador asociado del Directorio de Misiones Científicas de la NASA en Washington. "Los lugares de nuestro sistema solar, donde se producen los ambientes extremos en que la vida pudiera existir puede acercarnos más a responder a la pregunta: ¿Estamos solos en el Universo.".

    More information..............
    Cutaway view of Saturn's moon Enceladus
    This cutaway view of Saturn's moon Enceladus is an artist's rendering that depicts possible hydrothermal activity that may be taking place on and under the seafloor of the moon's subsurface ocean, based on recently published results from NASA's Cassini mission.
    Image Credit: 
    NASA/JPL
     
    NASA's Cassini spacecraft has provided scientists the first clear evidence that Saturn’s moon Enceladus exhibits signs of present-day hydrothermal activity which may resemble that seen in the deep oceans on Earth. The implications of such activity on a world other than our planet open up unprecedented scientific possibilities.
    “These findings add to the possibility that Enceladus, which contains a subsurface ocean and displays remarkable geologic activity, could contain environments suitable for living organisms,” said John Grunsfeld astronaut and associate administrator of NASA's Science Mission Directorate in Washington. “The locations in our solar system where extreme environments occur in which life might exist may bring us closer to answering the question: are we alone in the Universe.”
    Hydrothermal activity occurs when seawater infiltrates and reacts with a rocky crust and emerges as a heated, mineral-laden solution, a natural occurrence in Earth’s oceans. According to two science papers, the results are the first clear indications an icy moon may have similar ongoing active processes.
    Potential origins of methane on Enceladus
    This illustration depicts potential origins of methane found in the plume of gas and ice particles that sprays from Enceladus, based on research by scientists working with the Cassini Ion and Neutral Mass Spectrometer.
    Image Credit: 
    Southwest Research Institute
    The first paper, published this week in the journal Nature, relates to microscopic grains of rock detected by Cassini in the Saturn system. An extensive, four-year analysis of data from the spacecraft, computer simulations and laboratory experiments led researchers to the conclusion the tiny grains most likely form when hot water containing dissolved minerals from the moon's rocky interior travels upward, coming into contact with cooler water. Temperatures required for the interactions that produce the tiny rock grains would be at least 194 degrees Fahrenheit (90 degrees Celsius).
     
    "It's very exciting that we can use these tiny grains of rock, spewed into space by geysers, to tell us about conditions on -- and beneath -- the ocean floor of an icy moon," said the paper’s lead author Sean Hsu, a postdoctoral researcher at the University of Colorado at Boulder.
     
    Cassini's cosmic dust analyzer (CDA) instrument repeatedly detected miniscule rock particles rich in silicon, even before Cassini entered Saturn’s orbit in 2004. By process of elimination, the CDA team concluded these particles must be grains of silica, which is found in sand and the mineral quartz on Earth. The consistent size of the grains observed by Cassini, the largest of which were 6 to 9 nanometers, was the clue that told the researchers a specific process likely was responsible.
     
    On Earth, the most common way to form silica grains of this size is hydrothermal activity under a specific range of conditions; namely, when slightly alkaline and salty water that is super-saturated with silica undergoes a big drop in temperature.
     
    "We methodically searched for alternate explanations for the nanosilica grains, but every new result pointed to a single, most likely origin," said co-author Frank Postberg, a Cassini CDA team scientist at Heidelberg University in Germany.
     
    Hsu and Postberg worked closely with colleagues at the University of Tokyo who performed the detailed laboratory experiments that validated the hydrothermal activity hypothesis. The Japanese team, led by Yasuhito Sekine, verified the conditions under which silica grains form at the same size Cassini detected. The researchers think these conditions may exist on the seafloor of Enceladus, where hot water from the interior meets the relatively cold water at the ocean bottom.
     
    The extremely small size of the silica particles also suggests they travel upward relatively quickly from their hydrothermal origin to the near-surface sources of the moon's geysers. From seafloor to outer space, a distance of about 30 miles (50 kilometers), the grains spend a few months to a few years in transit, otherwise they would grow much larger.
    The authors point out that Cassini's gravity measurements suggest Enceladus' rocky core is quite porous, which would allow water from the ocean to percolate into the interior. This would provide a huge surface area where rock and water could interact.
     
    The second paper, recently published in Geophysical Research Letters, suggests hydrothermal activity as one of two likely sources of methane in the plume of gas and ice particles that erupts from the south polar region of Enceladus. The finding is the result of extensive modeling by French and American scientists to address why methane, as previously sampled by Cassini, is curiously abundant in the plume.
    The team found that, at the high pressures expected in the moon's ocean, icy materials called clathrates could form that imprison methane molecules within a crystal structure of water ice. Their models indicate that this process is so efficient at depleting the ocean of methane that the researchers still needed an explanation for its abundance in the plume.
    In one scenario, hydrothermal processes super-saturate the ocean with methane. This could occur if methane is produced faster than it is converted into clathrates. A second possibility is that methane clathrates from the ocean are dragged along into the erupting plumes and release their methane as they rise, like bubbles forming in a popped bottle of champagne.
    The authors agree both scenarios are likely occurring to some degree, but they note that the presence of nanosilica grains, as documented by the other paper, favors the hydrothermal scenario.
     
    "We didn't expect that our study of clathrates in the Enceladus ocean would lead us to the idea that methane is actively being produced by hydrothermal processes," said lead author Alexis Bouquet, a graduate student at the University of Texas at San Antonio. Bouquet worked with co-author Hunter Waite, who leads the Cassini Ion and Neutral Mass Spectrometer (INMS) team at Southwest Research Institute in San Antonio.
    Cassini first revealed active geological processes on Enceladus in 2005 with evidence of an icy spray issuing from the moon's south polar region and higher-than-expected temperatures in the icy surface there. With its powerful suite of complementary science instruments, the mission soon revealed a towering plume of water ice and vapor, salts and organic materials that issues from relatively warm fractures on the wrinkled surface. Gravity science results published in 2014 strongly suggested the presence of a 6-mile- (10-kilometer-) deep ocean beneath an ice shell about 19 to 25 miles (30 to 40 kilometers) thick.
     
    The Cassini-Huygens mission is a cooperative project of NASA, ESA (European Space Agency) and the Italian Space Agency. NASA's Jet Propulsion Laboratory in Pasadena, California, manages the mission for the agency’s Science Mission Directorate in Washington. The Cassini CDA instrument was provided by the German Aerospace Center. The instrument team, led by Ralf Srama, is based at the University of Stuttgart in Germany.
     
    More information about Cassini, visit:
     
     
    and
     

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    Guillermo Gonzalo Sánchez Achutegui
     
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