Mostrando entradas con la etiqueta NASA's Ames Research Center. Mostrar todas las entradas
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domingo, 8 de mayo de 2016

NASA : Mission Manager Q&A: Recovering The Kepler Spacecraft To Hunt For Exoplanets Again .- Responsable de la Misión Q & A: Recuperación de la nave espacial Kepler a la caza de exoplanetas nuevo


Artist's concept of Kepler-452b

Engineers, and their scientist colleagues, who saved NASA’s Kepler spacecraft – twice – will answer questions about what it took to recover Kepler and get it back on the job of searching for exoplanets and a menagerie of astrophysical phenomenon on Wednesday, May 4 at 2 p.m. EDT during a Reddit.com "Ask Me Anything" or AMA.
 
k2_explained_25nov_story.jpg
Engineers developed an innovative way to stabilize and control the spacecraft. This technique of using the sun as the "third wheel" has Kepler searching for planets again, but also making discoveries on young stars to supernovae.
Credits: NASA Ames/W Stenzel
 
The engineers and scientists at NASA's Ames Research Center in California's Silicon Valley, Ball Aerospace and the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado, both located in Boulder, had saved Kepler once before in 2013, using the subtle pressure from our sun as balance after wheels keeping the spacecraft steady failed soon after it completed an additional year in an extended mission. This save gave the spacecraft a new job called the K2 mission. K2 continues the legacy of planet hunting but has presented new opportunities to study supernovae, star clusters and galaxies far, far away. On April 8, right before it was slated to embark on K2's Campaign 9, a monumental scientific expedition to search for far out worlds, engineers found the spacecraft in a fuel-intensive “coma.” On April 22, the spacecraft was recovered to science mode and began making observations for the K2 mission once again.

NASA's Kepler and K2’s mission manager Charlie Sobeck, who will also be participating in Wednesday's AMA, sat down to talk with us about what happens once a spacecraft goes into emergency mode.


MJ: So let's start at the beginning. What happened to the Kepler spacecraft on April 8?

CS: Well, the first thing to remember was that we weren’t expecting anything like this. We had talked with the spacecraft four days earlier and everything was ready.  It was scheduled to make the turn to its observing attitude (MJ: where the spacecraft points the telescope to make observations) in the blind – that is, on its own without supervision from the ground. We’d completed eight previous campaigns, and although this one was going to be the first that looked in the forward velocity vector (MJ: instead of looking towards where it’s been, the spacecraft will look in the direction of where it’s going), there wasn’t much point in tying up an antenna at NASA's Deep Space Network (DSN) just to receive confirmation it was turning. Instead, we’d scheduled our next DSN contact for when the spacecraft should have thermally stabilized and had been collecting data for a few hours. We expected to find it happily humming away. Instead, on April 8 at 1:05 a.m. PDT, we found it in Emergency Mode. Not Safe Mode, mind you, where it’s gone in the past due to anomalies, but Emergency Mode, just a step from being altogether lost. This was the first time the spacecraft had ever been so desperate. Even when the reaction wheels failed, we never went into Emergency Mode.

So immediately, people started to gather. The Ball Aerospace engineers who manage the spacecraft operations on a day-to-day basis were already on-station (MJ: the Ball team was in place and in contact with the DSN station) for the contact, and as we had prearranged, they didn’t wait for the rest of us to get in before they started the recovery process. The first thing we knew was that the spacecraft had been in Emergency Mode for about 30 hours before we began our contact. That told us that whatever had happened, it happened before the spacecraft ever began the turn to the forward velocity vector. That eliminated the possibility that we had planned the turn wrong, or that the reaction wheels were a part of the problem, since they don’t start to spin until we get to our observing attitude.

We also knew that the fault which sent us to Emergency Mode was a Sun Avoidance fault – a pointing response, rather than say, an under-voltage or over-voltage condition. Beyond that, we were pretty blind. Telemetry is limited in Emergency mode.

The first order of business was to bring the spacecraft back from the edge, so to speak, to a more amenable Safe Mode, where we could gather some more data and lower the rate of fuel burn.

Those first data indicated a multi-system problem – thrusters, communication hardware, wheels, etc.  Since it is unlikely that many things would fail at once, this suggested that it was more likely a problem of the systems properly reporting their status.  You can see how the pieces of the puzzle start coming into focus, one piece at a time.

Once we had established a stable Safe Mode, we still needed to bring it back one step farther before we could begin the investigation in earnest. In both Safe Mode and Emergency Mode, the spacecraft points the solar panels towards the sun and goes into a slow spin to ensure that the transmitting antenna will sweep past Earth and give us a link. But this meant we could only gather limited data for 20 minutes every couple of hours when the antenna was pointed toward Earth during each rotation. To really dig into the problem we had to stop the spin while the antenna was pointed towards the Earth. When we did this, the recovery was able to really pick up speed.


MJ: What state is Kepler in now? Is it back to normal operations?

CS: Yes, Kepler is back to normal operations and has begun the K2 mission's Campaign 9, two weeks late. We still don’t know exactly what started all the problems, but once we completed the recovery all systems tested normal and it made no sense to keep it from its job while we dug into all the data that we collected and talked to the experts about what might have occurred.  We’ll continue the investigation while Kepler goes about its observations, though we’ll check on the spacecraft a bit more often until we gain confidence that is truly healthy and not just feeling OK.

But unless something new pops up, all the signs are that it should have no ill effects from its spree.


MJ: What is emergency mode and what does it mean to declare a spacecraft emergency?

CS: Emergency Mode is the spacecraft's last-ditch effort to save itself if all other actions fail to work. As such, it assumes that none of the regular tools in the toolbox are working properly (or it wouldn't have gotten to this state), and it reverts to only the most basic set of tools.

The most important distinction between Emergency Mode and any other mode the spacecraft works in, is the computers used to control the spacecraft. Kepler has two main computers, a prime and a secondary. It also has two back-up computers, prime & secondary. Emergency mode assumes that neither of the main computers is working and shuts them down, defaulting to the back-up pair. The back-up computers are more robust, but less capable than the main computers, and they also aren't trying to do as much.

Emergency Mode also turns off all “non-essential” equipment. So the photometer and data recorder are turned off. So are the reaction wheel and star trackers, along with the main computers and some other subsystems. The critical systems for Emergency Mode to keep on are the backup computers, the solar panels, a minimum set of thrusters and the communications systems to allow contact with the ground.

Data is limited in Emergency Mode, and is not stored, but simply transmitted in real time.

The spacecraft is pointed with the solar panels toward the sun to maximize the available power, and with the non-essential systems powered off, the power needs are minimized. The spacecraft is put into a slow spin about the sun-line, at about one full turn every two hours, or 20 seconds to move one degree. With the wheels off, thrusters must be used to establish the orientation, begin the spin and keep the solar panels toward the sun. This means a significantly higher rate of fuel burn, hence the need to respond quickly.

Declaring a spacecraft emergency establishes priority access to the DSN antennas. Typically, the DSN works with missions to allocate antenna access weeks to months in advance. When something unusual occurs this coordination can be shortened considerably, with the DSN facilitating negotiations between the various missions that use the antennas. But when a spacecraft is at serious and substantial risk of being lost, and the project manager is authorized to declare a “Spacecraft Emergency,” and negotiations are bypassed entirely, with all the necessary resources made available to support the mission at risk. Because other missions are doing unique and important work, disrupting them with an unplanned emergency is not an action that is taken lightly. We do not declare a spacecraft emergency when the spacecraft merely goes into Safe Mode, or if we simply don’t know what is going on. We use the spacecraft emergency card only when we truly believe the loss of the spacecraft is imminent without it.

This was the first, and hopefully last, use of a spacecraft emergency by the Kepler/K2 team.


MJ: Take us back to the days immediately following the spacecraft emergency declaration. What steps did the team take to recover the spacecraft from emergency? Who was involved? How did the team respond to the high-stakes nature of the situation?

CS: I described many of the steps we took in the answer to the first question.  The very first steps taken were to wake up the team members who were not already on duty.  Normal operations are conducted with a staff that consists of a flight director and flight operators working at the University of Colorado’s Laboratory for Atmospheric and Space Physics (LASP) in Boulder Colorado, and a mission operations manager and flight engineers at Ball Aerospace, also in Boulder. The staff at the LASP is the folks that are directly talking with the spacecraft, receiving the data and issuing commands through the DSN. The folks at Ball Aerospace have the responsibility to oversee that work and in addition, calculate and write the commands and determine what commands should be sent, in what sequence and with what timing. In our parlance, LASP is the mission operations center, and Ball operates the flight planning center. These are both professional and experienced organizations.

When the spacecraft was found to be in Emergency Mode, a network of phone calls went out to bring in additional staff and expertise. In particular, the mission director, the project systems engineer and the project manager from Ames were called in, as well as the Ball program manager. These additions would provide real-time, authoritative decisions, such as the declaration of a spacecraft emergency, and the ability to bring on specific resource as required. Resources such as the people who designed and built the spacecraft in the first place.

As I recall, I received a call from the mission director at Ames, Marcie Smith, at 1:25 a.m. Friday morning. Knowing that there was a planned spacecraft contact, I expected that she would tell me that the spacecraft point was just a bit off, and we’d have to give it a nudge. Instead I heard, “We’re in Emergency Mode.”  Within two minutes we confirmed what steps should be taken, and what resources needed to be immediately brought in, and that the flight team in Boulder had already begun the recovery actions. I headed into the office.

When I got to the office, Marcie was already at her desk with an open phone line that included both the Boulder groups as well as Ames, and the project systems engineer at Ames, Stephen Walker, joined us soon thereafter.

We pretty much lived in that environment for the next three days as we recovered the spacecraft to a manageable state and were able to end the spacecraft emergency declaration.

Throughout the process the team was focused and professional.  I was impressed with the commitment, which everyone on the team demonstrated, and the cool, thoughtful approach that was taken. As part of my roll, I alerted Ames and NASA management of the problem and kept them informed with regular status updates. Again, I was impressed with everyone’s ability to help when they could, and to stay out of the way when they couldn’t.


MJ: [Operating in emergency mode is fuel-intensive.] Has the fuel-intensive emergency mode impacted remaining plans for the K2 mission? Will fuel conservation measures be needed or will plans be altered?

CS: It is too early to adjust any plans based on the fuel status. It’s clear that this emergency consumed fuel at an accelerated rate, but it’s not clear how much was consumed, or why. It appears to me as though we lost more fuel than I had hoped, but less than I had feared. With the fuel loss, there has been a noticeable drop in the fuel tank pressure, but the pressure drop in not linear, so it isn’t immediately obvious what this means. I suspect it will take a few months of normal usage to recalibrate our fuel estimates. Generally we do this annually, and it seems that each year our estimates of our fuel efficiency is better than the year before.

The K2 mission has always been fundamentally limited by fuel, so to perform the maximum amount of science observations conserving fuel is an ongoing job. As we gain experience in operating the spacecraft in its two-wheel mode, we learn ways to improve our efficiency. Several steps have already been taken, which have doubled our initial mission duration estimates, but we’ve probably already made most of the gains that can be expected, so I don’t expect a lot more.

Measure the quantity of a liquid in space is a difficult business, so how much fuel we have left is uncertain. It has been our plan to continue operating the K2 mission until the fuel runs out. Meaning that at some point we will begin a campaign and will never hear back from the spacecraft.


MJ: It was reported that the cause is likely a transient event. What is a transient event and when will you know the root cause of the spacecraft anomaly?

CS: By a “transient event,” I mean something that existed for a relatively short period of time, and then went away, either on it’s own or because of the emergency mode and its recovery. Transient events might result from highenergy cosmic rays that can randomly hit a sensitive piece in the electronics. Power surges or dropouts that can cause the electronics to perform atypically for a period of time, or by a race condition that results from a timing conflict between two contradictory signals can also cause transient events.

Whatever the cause, what distinguishes a transient event is the fact that it is reversible, and the systems can be restored. Often when the system is restored, the nature of the transient remains unknown, and this may be true in this case as well. This is as opposed to a “hard failure,” such as a fuse blowing out or a hard disk physically crashing. These things are not reversible.

We are all used to such unexplained transient events in our daily lives: our cell phones drop out, our computer hangs up and the lights dim. Sometimes these are explainable (the lights dim when the refrigerator compressor comes on), but often they are not. We learn to live with them as a normal part of life. We call back and we reboot the computer.

Spacecraft are designed and built to be more reliable than many of our everyday appliances, but it doesn’t mean they are totally immune from these failures. The spacecraft today, looks to be operating just as it did before the event.  So whatever happened, it appears to have not only been reversible, but has now reverted to its previous state.


MJ: Kepler has had mechanical problems in the past. Is this recent event connected to previous issues, and does this signal end-of-life for the spacecraft?

CS:  The Emergency Mode doesn’t appear to be related to any of previous problem, the main one that comes to mind is the reaction wheels. The wheels were not spinning and not being used when the Emergency Mode occurred.

We have seen other surprises during the course of the mission: counters that rolled over to zero, optical reflections of bright objects. But this event doesn’t seem to resemble these… at least, so far.  We don’t yet know what spawn the problem, and we may never know, but the first effects that we’ve found were a sudden series of alarms that caused the onboard fault protection to react.  Although the fault protection seems to have responded appropriately to each of the alarms, the alarms themselves seem to be erroneous: That is, they were false alarms that didn’t accurately reflect what was going on. As a result, the spacecraft’s response didn’t address the real situation, only the situation that was reported. In such conditions the resulting actions can, and this case were, detrimental rather than helpful.

We have seen erroneous alarms before, but not like this.

The good news is that everything seems to have returned to normal, and while this still may be a sign of the aging of the systems, it could have also been a random occurrence.


MJ: Had Kepler been unrecoverable, what were some of the planned scientific targets that we may have missed out on

CS: If the spacecraft were truly unrecoverable, then no further science will be gathered and the K2 mission would end. We would have completed eight of the expected 18 or so campaigns. The fields of view of the remaining planned campaigns can be found at the Kepler Science Center site. The K2 targets are entirely selected through competitive process, with proposals considered for two to three campaigns at a time. Information on the observed and planned targets can also be found at the Kepler Science Center.


Q9: How often is the status and health of Kepler checked in on, typically, and how closely is it being monitored now?

CS: Typically the spacecraft is contacted at least twice a week to verify that it remains in its expected state of health. During the initial recovery, it was monitored as continuously as possible, with occasional gaps of three to four hours in order to allow the ground antennas to check on other NASA spacecraft. These gaps occurred overnight, while the ground team got some sleep. Once the spacecraft was out of immediate danger and we released the declaration of a spacecraft emergency, it was monitored as much as possible, given the constraints of also operating other missions, but at least several hours each day.

Now that the spacecraft is back in normal operations we will generally contact it daily for a couple of weeks while we build confidence that there is no persistent problem. Eventually I expect that we will return to our normal practice of checking on it twice a week.


MJ: The Kepler mission, and the follow-on mission called K2, is one of NASA's most visible missions. How did it feel to manage the team through the crisis as many watched with great interest and anticipation? Did you have your doubts that the spacecraft would return to make new scientific observations?

CS: I think there are many people who face this kind of situation daily: first responders, emergency rooms, etc. There is a sense of satisfaction in doing a job well and doing it under pressure. This was our emergency, and our opportunity to respond.

I was fully aware that the situation was serious and needed focused attention.  But I also knew that we had a good team with a lot of experience. There was no panic. Rather there was a focused determination. The team worked professionally, dealing with the problem at hand, prioritizing actions and implementing solutions.

For the most part, we weren’t occupied with worrying about the future, but focusing on the present before us. When there were periods where there was time to reflect, most of the discussions were speculations on the potential causes, what those causes might mean in the near term, and what actions could be taken to mitigate them. I don’t believe anyone had more than a momentary thought that the mission had ended.


MJ: Charlie, thank you for your candor and walking us through an incredible experience—once again demonstrating when faced with adversity, a calm and collected response prevails. In that vain, what advice would you give to the next generation of engineers and scientists interested in pursuing the type of work you do at NASA?

CS: For my part, I feel that NASA does important work, and it’s work that I wanted to be a part of. I’ve enjoyed my job and am grateful to have had the opportunities I’ve had. My advice for someone interested in pursuing a job at NASA is much the same as I would give to anyone else: Do what you enjoy. Do what you’re good at. Do something you feel is important. And whatever it is you do, try to do it well. Be open to opportunities. Be helpful. 

There are many opportunities. Not all of us are astronauts, but we can all be helpful and productive as we continue to explore the space around us and far, far away.

Regards,
Charlie Sobeck
Kepler and K2 mission manager
NASA's Ames Research Center

Media contact:
Michele Johnson
Ames Research Center, Moffett Field, Calif.
650-604-6982
michele.johnson@nasa.gov
Last Updated: May 6, 2016
Editor: Michele Johnson
NASA
Guillermo Gonzalo Sánchez Achutegui
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lunes, 29 de junio de 2015

NASA : Measuring the Mass of a Mars-size Exoplanet .- La medición de la masa de un exoplaneta del tamaño de Marte

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, sobre la medición del tamaño de los exo planetas de la Serie Kepler-138. 
NASA, nos dice: Determinación del tamaño de un exoplaneta del tamaño de la Tierra por la cantidad de luz de las estrellas bloquea los cientos de años luz de distancia, una vez fue el reino de la ciencia ficción. La medición de la masa de un planeta tan pequeño en función de su gravedad era otro nivel completamente, pero los astrónomos han hecho precisamente eso para un exoplaneta del cincuenta por ciento del tamaño de la Tierra.
Los investigadores que utilizan datos de la misión Kepler de la NASA ha medido la masa de un exoplaneta del tamaño de Marte que es aproximadamente una décima parte de la masa de la Tierra. Llamado Kepler-138b, es el primer exoplaneta más pequeño que la Tierra para tener midieron tanto su masa y tamaño. Esto amplía significativamente el rango de planetas con densidades medidas.
More information............
http://www.nasa.gov/ames/kepler/measuring-the-mass-of-a-mars-size-exoplanet

Measuring the Mass of a Mars-size Exoplanet

Determining the size of an Earth-size exoplanet by the amount of starlight it blocks hundreds of light-years away once was the realm of science fiction. Measuring the mass of such a small planet based on its gravity was another level entirely, but astronomers have done just that for an exoplanet fifty percent the size of Earth.
Researchers using NASA's Kepler mission data have measured the mass of a Mars-size exoplanet that is about one tenth the mass of Earth. Called Kepler-138b, it is the first exoplanet smaller than Earth to have both its mass and size measured. This significantly extends the range of planets with measured densities.

Mars-size exoplanet gets a mass
The artistic concept shows the planetary system harboring Kepler-138b, the first exoplanet smaller than Earth with both a mass and size measurement. The sizes of the planets relative to the star have been exaggerated.
Credits: SETI Institute/Danielle Futselaar
 
To determine a planet's mass, astronomers typically measure the minuscule movement of the star caused by the gravitational tug of an orbiting planet. For planets the mass of Earth detecting such a tiny tug is extraordinarily challenging with current technology. Fortunately, when a star hosts multiple planets that orbit closely together, scientists have developed another way to get at the planets’ masses.
Daniel Jontof-Hutter, a research associate at the Pennsylvania State University’s Center for Exoplanets and Habitable Worlds, led a team of astronomers in a study to measure the mass of all three planets by precisely observing the times each planet passed in front of, or transited, the star Kepler-138.
"Each planet periodically slows down and accelerates ever so slightly from the gravity of its neighboring planets. The slight change in time between transits allows us to measure the masses of the planets," said Jontof-Hutter. 
Each time a planet transits a star it blocks a small fraction of the star's light, allowing astronomers to measure the size of the planet. This is how the Kepler spacecraft has detected thousands of planets around other stars.
By measuring both the mass and size of an exoplanet, scientists can calculate the density and infer the bulk composition to determine if a planet is predominantly made of rock, water or gas. Tiny Kepler-138b's density is consistent with a rocky composition like Earth or Mars, but further observations are needed before astronomers can definitively say that it is a rocky world.
Kepler-138b is the innermost of three planets that orbit Kepler-138, a star less than half the size of our sun and roughly 30 percent cooler. The Kepler-138 system is located about 200 light-years from Earth in the direction of the constellation Lyra. 
The outer two planets, Kepler-138c and Kepler-138d, are approximately the size of Earth. Kepler-138c is likely to be rocky, whereas Kepler-138d is less dense and cannot be made of the same mix of material as Earth. All three planets orbit too close to their star for liquid water to exist on the surface and support life, as we know it.

Mass and Radius of Kepler-138 Planets
This plot shows the masses and sizes of the smallest exoplanets for which both quantities have been measured. The solar system planets (shown in red) are for comparison.The three Kepler-138 planets (shown in orange) are among the four smallest exoplanets with both size and mass measurements. Kepler-138b is the first exoplanet smaller than Earth to have both its mass and size measured. This significantly extends the range of planets with measured densities.
Credits: NASA Ames/W Stenzel
"The substantial difference between the densities of the two larger planets tells us that not all planets similar to Earth in size are rocky," said Jack Lissauer, co-author and planetary scientist at NASA's Ames Research Center in Moffett Field, Calif. "Further study of small planets will help provide more understanding of the diversity that exists in nature, and will help determine if rocky planets like Earth are common or rare."
Much like astronomers in the early 20th century studied a wide variety of stars to characterize and classify different types, astronomers in the 21st century are doing the same to understand the diversity and demographics of planet populations in our Milky Way galaxy. 
Scientists are working to use these new measurements of small planets from Kepler and NASA's upcoming Transiting Exoplanet Survey Satellite to identify patterns in the relationship between mass and size. These insights will provide context for understanding the history of Earth and other planets in our own solar system, and inform the next generation planet hunters as they search for life beyond the solar system. 
A previous study had measured the masses of the two outer planets. This new study performed a more detailed analysis of the Kepler-138 system using additional Kepler data. This enabled the measurement of the mass of the Mars-size inner planet and improved the accuracy of the size and mass measurements for the outer planets. The results will appear in this Thursday's issue of the journal Nature.
Ames Research Center in Moffett Field, California, manages the Kepler and K2 missions for NASA’s Science Mission Directorate. NASA's Jet Propulsion Laboratory in Pasadena, California, managed Kepler mission development. Ball Aerospace & Technologies Corp. operates the flight system with support from the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder.
For more information on the Kepler mission, visit: www.nasa.gov/kepler.
A team of astronomers have measured the mass and size of the smallest exoplanet yet, a Mars-sized planet named Kepler-138b orbiting a red dwarf star about 200 light years from the Solar System. The animation shows the mass-radius diagram based on measurements of 127 exoplanets. The video begins by showing planets with masses similar to Jupiter and slowly zooms towards small masses and radii planets to display a comparison of the physical properties of the Kepler-138 planets relative to Earth, Venus, Mars and Mercury. The planet Kepler-138b is the first exoplanet smaller than the Earth to have both its mass and its size measured, and is one of three planets that orbit the star Kepler-138, and pass in front of it, or transit, every orbit. Each time a planet transits the star, it blocks a small fraction of the star's light, allowing astronomers to measure the size of the planet. All three planets were identified by NASA's Kepler mission that has discovered over a thousand planets around other stars.
Credits: Jason Rowe, NASA Ames/SETI Institute

Michele Johnson
Ames Research Center, Moffett Field, Calif.
650-604-6982
michele.johnson@nasa.gov
Last Updated: June 29, 2015
Editor: Michele Johnson
Tags:  Ames Research Center, Distant Planets, Kepler and K2, Mars, Universe
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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viernes, 23 de enero de 2015

NASA : Astronomers Discover First Multiple-Planet System From K2 .- Astrónomos Descubren el primer sistema de múltiple-Planet Desde K2

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido de la Agencia Espacial NASA, la información sobre el descubrimiento un sistema múltiple desde el NASA's planet-hunting Kepler spacecraft; los astrónomos que usan datos de misión K2 renacer de la nave espacial Kepler de la NASA pueden haber hecho su primer descubrimiento de una estrella con tres exoplanetas-planetas que orbitan otras estrellas que nuestro sol. Un artículo que informa de este descubrimiento ha sido enviado para su publicación en The Astrophysical Journal.
NASA, nos dice "....Su tamaño varía entre cincuenta por ciento más grande que un poco más del doble del tamaño de la Tierra, los posibles planetas orbitan una estrella alrededor de la mitad del tamaño y la masa de nuestro sol. , La distancia de una estrella donde podría existir agua líquida Las órbitas de planetas más exteriores en el borde cálido de la zona habitable de la superficie de un planeta en órbita...."
NASA, agrega : ""Estamos encantados de ver la respuesta entusiasta de K2. La misión ha ampliado la capacidad de búsqueda del telescopio a una nueva parte del cielo, marcando el primer descubrimiento de exoplanetas K2 hace menos de un mes, y ahora el posible descubrimiento de la primera múltiple K2 sistema -PLANET ", dijo Charles Sobeck, director del proyecto Kepler en el Centro de Investigación Ames de la NASA en Moffett Field, California "Esperamos con interés los resultados del proceso de revisión de este último resultado."
The artistic concept shows NASA's planet-hunting Kepler spacecraft operating in a new mission profile called K2
The artistic concept shows NASA's planet-hunting Kepler spacecraft operating in a new mission profile called K2. Using publicly available data, astronomers may have confirmed K2's first discovery of star with more than one planet.
Image Credit: 
NASA Ames/JPL-Caltech/T Pyle
 
Astronomers using data from the NASA Kepler spacecraft's reborn K2 mission may have made its first discovery of a star with three exoplanets—planets that orbit stars other than our sun. A paper reporting this discovery has been submitted for publication in The Astrophysical Journal.
 
Ranging in size from fifty percent larger to a little more than twice the size of Earth, the possible planets orbit a star about half the size and mass of our sun. The outermost planet orbits on the warm edge of the habitable zone, the distance from a star where liquid water might exist on the surface of an orbiting planet.
 
"We are delighted to see the enthusiastic response for K2. The mission has extended the telescope's search capability to a new part of the sky, marking the first K2 exoplanet discovery less than a month ago, and now the possible discovery of the first K2 multiple-planet system," said Charles Sobeck, Kepler project manager at NASA's Ames Research Center in Moffett Field, CA. "We look forward to the outcome of the peer-review process of this latest result."
The star, called EPIC 2011367065, home to these possible planets is about 150 light-years away in the constellation Leo.
For more information about the Kepler and K2 missions, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui
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domingo, 30 de noviembre de 2014

NASA : Supercomputer Simulation of Magnetic Field Loops on the Sun.- Supercomputadora Simulación de Campo Magnético Loops en el Sol

Hola amigos: A VUELO DE UN QUINDE EL BLOG., la Agencia Espacial NASA, nos informa sobre la simulación  del Gran Campo Magnético del Sol en una computadora; Los campos magnéticos que salen de debajo de la superficie del sol influye en el viento solar, una corriente de partículas que  sopla continuamente de la atmósfera del Sol a través del sistema solar. Los investigadores de la NASA y sus socios de la universidad con sus  instrumentos de alta fidelidad van haciendo y utilizando simulaciones por ordenador para aprender. Estos campos magnéticos emergen, calentar la atmósfera externa del sol y producir manchas y llamaradas.
Supercomputer Simulation of Magnetic Field Loops on the Sun
 
Magnetic fields emerging from below the surface of the sun influence the solar wind—a stream of particles that blows continuously from the sun’s atmosphere through the solar system. Researchers at NASA and its university partners are using high-fidelity computer simulations to learn how these magnetic fields emerge, heat the sun’s outer atmosphere and produce sunspots and flares.
This visualization shows magnetic field loops in a portion of the sun, with colors representing magnetic field strength from weak (blue) to strong (red). The simulation was run on the Pleiades supercomputer at the NASA Advanced Supercomputing facility at NASA's Ames Research Center in Moffett Field, California. 
The knowledge gained through simulation results like this one help researchers better understand the sun, its variations, and its interactions with Earth and the solar system.
Image Credit: Robert Stein, Michigan State University; Timothy Sandstrom, NASA/Ames
> Related: NASA showcased more than 35 of the agency’s exciting computational achievements at SC14, the international supercomputing conference, Nov. 16-21, 2014, in New Orleans.
NASA
Guillermo Gonzalo Sánchez Achutegui
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sábado, 23 de agosto de 2014

NASA : NASA Picks Top Earth Data Challenge Ideas, Opens Call for Climate Apps


OpenNEX Challenge Phase II
OpenNEX Challenge Phase II
Image Credit: 
NASA
 
NASA has selected four ideas from the public for innovative uses of climate projections and Earth-observing satellite data. The agency also has announced a follow-on challenge with awards of $50,000 to build climate applications based on OpenNEX data on the Amazon cloud computing platform.

Both challenges use the Open NASA Earth Exchange, or OpenNEX, a data, cloud computing, and knowledge platform where users can share modeling and analysis codes, scientific results, information and expertise to solve big data challenges in the Earth sciences. OpenNEX provides users a large collection of climate and Earth science satellite data sets, including global land surface images, vegetation conditions, climate observations and climate projections.
The four winners of the "ideation" stage of the OpenNEX challenge, which ran from July 1 through Aug. 1, will share a $10,000 award for their ideas on novel uses of the datasets. Abdal Elhassani of Indiana University, Bloomington, proposed an app to predict how plant hardiness zones will change in the future with a changing climate. Edward Aboufadel of Grand Valley State University, Allendale, Michigan, suggested using the data to compare a local community's future predicted climate with the historical record of another community.
A team led by Raymond Milowski of San Francisco proposed converting the storehouse of OpenNEX climate model data to formats compatible with the Open Web Platform to facilitate wider use by web developers. Reuben Cummings from Peoria, Illinois, suggested a web application to map potential and actual climate-related environmental hazards such as wildfires, flood, and drought across the United States.
"The ideas generated by this OpenNEX challenge demonstrate the value of these NASA data assets when put in the hands of citizen scientists," said Ramakrishna Nemani, principal scientist for the NEX project at NASA's Ames Research Center in Moffett Field, California. "Our second challenge seeks to rapidly turn these ideas into practical applications."
The second "builder" challenge that opens Friday offers awards for the development of an application or algorithm that communicates climate change impacts to the general public using the OpenNEX data. Submissions based on the winning proposals in the "ideation" challenge are encouraged, in addition to new ideas that focus on climate change impacts.
Applications should communicate through concise summaries of impacts over time that can be easily related to familiar climate-related events and processes. The summaries may rely on key climatic events or observable events dependent on climate, such as changes in the timing of snow melt and runoff, plant flowering and the start of the allergy season, and the annual migration of birds. Developers are not limited to these examples, and are encouraged to consider solutions that incorporate other scientifically-based climate summaries and analogs.
“NASA is committed to engaging and enabling individuals and groups to make use of these high-quality scientific data and innovative technologies to better communicate climate change impacts to the general public," said Tsengdar Lee, program manager in the Earth Science Division of the Science Mission Directorate at NASA Headquarters in Washington.
Entries are due by Oct. 21 and NASA plans to announce the winners on Dec. 15.
NASA's OpenNEX challenge ties in to a number of White House initiatives, including Open Data, Big Data and Climate Data. These initiatives advance national goals to address climate change impacts on economic growth, health and livelihood, and include the use of competitions and challenges to foster regional innovation.
The challenges are managed by NASA's Center of Excellence for Collaborative Innovation. The center was established in coordination with the White House Office of Science and Technology Policy to advance NASA’s open innovation efforts and extend that expertise to other federal agencies. The challenges are released on the NASA Innovation Pavilion, one of the center's platforms available to NASA team members, through its contract with InnoCentive, Inc.
To educate citizen scientists about how the data on OpenNEX can be used, NASA has created a series of online video lectures and hands-on lab modules. To view this material, and for information on registering for the challenges, visit:
OpenNEX is hosted on the Amazon Web Services (AWS) cloud and available to the public through a Space Act Agreement. Challenge developers are eligible for credits on the AWS platform to build their applications.
NASA monitors Earth's vital signs from land, air and space with a fleet of satellites and ambitious airborne and ground-based observation campaigns. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records and computer analysis tools to better see how our planet is changing. The agency shares this unique knowledge with the global community and works with institutions in the United States and around the world that contribute to understanding and protecting our home planet.
For more information about NASA's Earth science activities in 2014, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui
Inscríbete en el Foro del blog y participa : A Vuelo De Un Quinde - El Foro!

domingo, 13 de julio de 2014

NASA :NASA TV Coverage Reset for Sunday Orbital-2 Mission to Space Station


Orbital Sciences Corporation Antares rocket
Orbital Sciences Corporation's Cygnus spacecraft will launch atop an Antares rocket carrying more than 3,000 pounds of supplies to the International Space Station, including science experiments, experiment hardware, spare parts, and crew provisions.
Image Credit: NASA/Aubrey Gemignani
 
NASA Television will provide live coverage of the upcoming Orbital Sciences' mission to resupply the International Space Station. Orbital's Cygnus cargo spacecraft is schedule to launch from the Mid-Atlantic Regional Spaceport's Launch Pad 0A at NASA's Wallops Flight Facility in Virginia on Sunday, July 13 at 12:52 p.m. EDT.
Severe weather in the Wallops area throughout the week repeatedly interrupted Orbital’s operations schedule leading up to the launch, resulting in the company deciding to postpone launch to Sunday.
NASA TV will air a comprehensive video feed of launch preparations and other footage related to the mission beginning at 11:30 a.m. Launch coverage on NASA TV will begin at noon. A post-launch news conference will be held about an hour-and-a-half after launch.
On Saturday, July 12, a prelaunch status from Wallops will be broadcast on NASA TV at 1 p.m. A media briefing previewing the science and technology cargo headed to the space station will still occur at 4 p.m. today, as previously planned.
Media also may join the briefings by phone. To obtain dial-in information, media must contact Rachel Kraft at rachel.h.kraft@nasa.gov with their name and media affiliation no later than 30 minutes before the beginning of each briefing. The public also may ask questions on social media using the hashtag #AskNASA.
The Cygnus will be filled with approximately 3,300 pounds of supplies for the station, including science experiments to expand the research capability of the space station's Expedition 40 crew members aboard the station, crew provisions, spare parts and experiment hardware.
Among the research investigations headed to the orbital laboratory are a flock of nanosatellites designed to take images of Earth, developed by Planet Labs of San Francisco, and a satellite-based investigation called TechEdSat-4 built by NASA's Ames Research Center in Moffett Field, California, which aims to develop technology that eventually will enable small samples to be returned to Earth from the space station. In addition, a host of student experiments are on board as part of the Student Spaceflight Experiment Program, an initiative of the National Center for Earth and Space Science Education and NanoRacks.
This and future commercial cargo resupply flights will ensure a robust national capability to deliver critical science research to orbit, significantly increasing NASA's ability to conduct new science investigations to the only laboratory in microgravity.
If Cygnus launches as scheduled, the spacecraft will arrive at the space station on Wednesday, July 16. Station commander Steven Swanson of NASA and Flight Engineer Alexander Gerst of the European Space Agency will be standing by in the station’s cupola to capture the resupply craft with the station's robotic arm and install it on the Earth-facing port of the station's Harmony module.
NASA TV coverage of capture will begin at 5:15 a.m. on July 16. Grapple is scheduled at approximately 6:37 a.m. Installation coverage of Cygnus onto Harmony will begin at 8:30 a.m.
For a full update of media activities and more information on the Orbital-2 mission, visit: 
                                          
For NASA TV streaming video, downlink and scheduling information, visit:
For video b-roll and media resources on the International Space Station, visit:
For more information about International Space Station, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui

jueves, 3 de julio de 2014

NASA : NASA Television Coverage Set for Orbital-2 Mission to Space Station


Orbital Sciences Corp.’s Antares rocket for the Orb-2 cargo resupply mission to the International Space Station is lifted onto the Transporter/Erector/Launcher (TEL). The stage one core for the next mission, Orb-3, is on the left. Orbital is scheduled to launch its Cygnus cargo spacecraft to the space station on July 11 from the Mid-Atlantic Spaceport’s Pad 0A at NASA’s Wallops Flight Facility in Virginia.
Orbital Sciences Corp.’s Antares rocket for the Orb-2 cargo resupply mission to the International Space Station is lifted onto the Transporter/Erector/Launcher (TEL). The stage one core for the next mission, Orb-3, is on the left. Orbital is scheduled to launch its Cygnus cargo spacecraft to the space station on July 11 from the Mid-Atlantic Spaceport’s Pad 0A at NASA’s Wallops Flight Facility in Virginia.
Image Credit: Orbital Sciences
 

NASA Television will provide live coverage of the upcoming Orbital Sciences Corp.'s mission to resupply the International Space Station.

Orbital's Cygnus cargo spacecraft is scheduled to launch from the Mid-Atlantic Regional Spaceport's Launch Pad 0A at NASA's Wallops Flight Facility in Virginia on Friday, July 11 at 1:40 p.m. EDT.
NASA TV will air a comprehensive video feed of launch preparations and other footage related to the mission beginning at 12:30 p.m. Launch coverage on NASA TV will begin at 1 p.m.
On Thursday, July 10, media briefings previewing the mission's science cargo and a prelaunch status from Wallops will be broadcast on NASA TV at 4 p.m. and 5 p.m., respectively.
The Cygnus will be filled with more than 3,000 pounds of supplies for the station, including science experiments to expand the research capability of the Expedition 40 crew members aboard the orbiting laboratory, crew provisions, spare parts and experiment hardware.
Among the research investigations headed to the space station aboard Orbital-2 are a flock of nanosatellites that are designed to take images of Earth, developed by Planet Labs of San Francisco; and a satellite-related investigation called TechEdSat-4 built by NASA's Ames Research Center in California, which aims to develop technology that will eventually enable small samples to be returned to Earth from the space station. In addition, a host of student experiments are being flown in association with the Student Spaceflight Experiment Program, an initiative of the National Center for Earth and Space Science Education and NanoRacks.
This and future commercial cargo resupply flights will ensure a robust national capability to deliver critical science research to orbit, significantly increasing NASA's ability to conduct new science investigations to the only laboratory in microgravity.
If Cygnus launches as scheduled, the spacecraft will arrive at the space station on Tuesday, July 15. Station commander Steven Swanson of NASA and Flight Engineer Alexander Gerst of the European Space Agency will be standing by in the station’s cupola to capture the resupply craft with the station's robotic arm and install it on the Earth-facing port of the station's Harmony module.
NASA TV coverage of capture and installation will begin at 6:15 a.m.  on July 15. Grapple is scheduled at approximately 7:24 a.m. Coverage of the installation of Cygnus onto Harmony will begin at 9:30 a.m.
For a full update of media activities and more information on the Orbital-2 mission, visit:                                          
For NASA TV streaming video, downlink and scheduling information, visit:
For video b-roll and media resources on the International Space Station, visit:
For more information about International Space Station, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui

sábado, 21 de junio de 2014

NASA : College Students Study Earth From NASA's DC-8 Flying Lab


Professor Donald Blake of the University of California—Irvine outlines procedures for installation of air canister racks on NASA's DC-8 flying laboratory to students participating in NASA's 2014 Student Airborne Research Program.
Professor Donald Blake of the University of California—Irvine outlines procedures for installation of air canister racks on NASA's DC-8 flying laboratory to students participating in NASA's 2014 Student Airborne Research Program.
 
Thirty-two undergraduate students from a like number of colleges and universities are participating in an eight-week NASA Airborne Science Program field experience designed to immerse them in the agency's Earth Science research.
Jonathan Hemingway, an applied meteorology and computational mathematics major at Embry-Riddle Aeronautical University in Florida, assists in installation of the Whole Air Sampler instrument on NASA's DC-8 flying laboratory.
Jonathan Hemingway, an applied meteorology and computational mathematics major at Embry-Riddle Aeronautical University in Florida, assists in installation of the Whole Air Sampler instrument on NASA's DC-8 flying laboratory.
 
Josette Marrero, a Ph.D. candidate in the Rowland-Blake Lab at UC Irvine, explains the installation of the Whole Air Sampler on board NASA's DC-8 to Student Airborne Research Program participants.
Josette Marrero, a Ph.D. candidate in the Rowland-Blake Lab at UC Irvine, explains the installation of the Whole Air Sampler on board NASA's DC-8 to Student Airborne Research Program participants.
 
Caleb Sykora-Bodie, an environmental geoscience and geography major at Slippery Rock University, connects lines during installation of the Whole Air Sampler instrument for the SARP flights.
Caleb Sykora-Bodie, an environmental geoscience and geography major at Slippery Rock University, connects lines during installation of the Whole Air Sampler instrument for the SARP flights.
Krystal Vasquez, a chemistry major at the University of California, Riverside, assists in the installation of the Whole Air Sampler instrument on NASA's DC-8 flying laboratory.
Krystal Vasquez, a chemistry major at the University of California, Riverside, assists in the installation of the Whole Air Sampler instrument on NASA's DC-8 flying laboratory.
 
Flying aboard NASA’s DC-8 airborne laboratory, students will measure pollution, aerosols (small particles suspended in the atmosphere) and air quality in the Los Angeles basin and California’s central valley. They will also use remote sensing instruments to study forest ecology in the Sierra Nevada and ocean biology along the California coast.
Now in its sixth year, NASA's Student Airborne Research Program (SARP) provides a unique opportunity for undergraduate students majoring in the sciences, mathematics and engineering to participate in all aspects of a NASA Airborne Science research campaign.
SARP participants are given a rare behind-the-scenes look at the instrument installation, flight planning and scientific data collection that is the basis of every successful NASA Earth Science airborne campaign. These campaigns play a pivotal role in the acquisition of process-oriented knowledge about the Earth system, as well as calibration of NASA's space-borne Earth observation instruments, validation of remote sensing measurements and high-resolution imagery for Earth system science.
SARP began June 16 at NASA Armstrong Flight Research Center's facility in Palmdale, California, with lectures by university faculty members, NASA scientists and NASA program managers. The students will then be aboard the DC-8 on five flights during the week of June 23. They will acquire multi-spectral images of kelp beds in the Santa Barbara Channel and of forests in the Sierra Nevada.
In addition, the students will fly over dairies and oil fields in the San Joaquin Valley, parts of the Los Angeles basin and the Salton Sea at altitudes as low as 1,000 feet in order to collect air samples, measure aerosols and air quality. During the final flight, half of the students will be in the field taking ground validation or complementary measurements while the DC-8 flies overhead.
The final six weeks of the program will take place at the University of California, Irvine where students will analyze and interpret the data they collected from science instruments on the aircraft.  At the conclusion of the program, the students will each deliver final presentations about their results and conclusions in front of an audience of NASA scientists and administrators, university faculty members and their fellow SARP students. In past summers, many students have gone on to present their SARP research projects at national conferences.
Students participating in the 2014 SARP represent 32 different colleges and universities from across the United States. They were competitively selected based on their outstanding academic performance, future career plans and interest in the Earth System Science.
The Student Airborne Research Program is one of NASA's tools to expose future scientists to the Earth Science missions that support environmental studies and the testing and development of new instruments and future satellite mission concepts. The program's goal is to stimulate interest in NASA's Earth Science research and aid in the recruitment and training of the next generation of scientists and engineers, many of whom will be getting their first hands-on research experience during this program.
NASA monitors Earth's vital signs from land, air and space with a fleet of satellites and ambitious airborne and ground-based observation campaigns. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records and computer analysis tools to better see how our planet is changing. The agency shares this unique knowledge with the global community and works with institutions in the United States and around the world that contribute to understanding and protecting our home planet.
SARP is managed by NASA's Ames Research Center at Moffett Field, California, through the National Suborbital Education and Research Center (NSERC) at the University of North Dakota.  As part of the Ames Cooperative for Research in Earth Science and Technology, NSERC receives funding and support from NASA’s Earth Science Division.
For additional information about SARP, visit:
View video about the 2013 SARP experience:
For more about NASA's Earth science activities in 2014, visit:
For more on NASA's Airborne Science Program, visit:
For additional information about NASA's DC-8, visit:
NASA / NSERC photos by Jane Peterson
NASA
Guillermo Gonzalo Sánchez Achutegui

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