Mostrando entradas con la etiqueta Distant Planets. Mostrar todas las entradas
Mostrando entradas con la etiqueta Distant Planets. Mostrar todas las entradas

viernes, 13 de mayo de 2016

NASA : NASA's Kepler Mission Announces Largest Collection of Planets Ever Discovered .- Misión Kepler de la NASA anuncia la mayor colección de planetas descubierto que nunca

Hola mis amigos: A VUELO DE UN QUINDE EL BLOG., la Agencia Espacial NASA, anuncia su satisfacción por la gran colección de planetas descubiertos hasta ahora cono su misión del Telescopio Espacial Kepler; NASA, nos dice: "La misión Kepler de la NASA ha verificado 1.284 nuevos planetas - el mayor hallazgo de planetas hasta la fecha.
"Este anuncio es más del doble el número de planetas confirmados de Kepler", dijo Ellen Stofan, jefe científico de la NASA en Washington. "Esto nos da esperanzas de que en algún lugar, alrededor de una estrella muy parecida a la nuestra, eventualmente podemos descubrir otra tierra."
El análisis se realizó de julio el año 2015 Catálogo candidato a planeta del telescopio espacial Kepler, que identificó 4.302 potenciales planetas. Para 1.284 de los candidatos, la probabilidad de ser un planeta es mayor que el 99 por ciento - el mínimo requerido para ganar el estado de un 1.327 candidatos adicionales son más propensos que los no ser planetas reales, pero que no cumplen con el "planeta". 99 por ciento de umbral y requerirán un estudio adicional. Los restantes 707 son más propensos a ser algún otro fenómenos astrofísicos. Este análisis también validó 984 candidatos verificados previamente por otras técnicas....."
More information....

This artist's concept depicts select planetary discoveries made to date by NASA's Kepler space telescope.
This artist's concept depicts select planetary discoveries made to date by NASA's Kepler space telescope.
Credits: NASA/W. Stenzel
 
NASA's Kepler mission has verified 1,284 new planets – the single largest finding of planets to date.

“This announcement more than doubles the number of confirmed planets from Kepler,” said Ellen Stofan, chief scientist at NASA Headquarters in Washington. “This gives us hope that somewhere out there, around a star much like ours, we can eventually discover another Earth.” 

Analysis was performed on the Kepler space telescope’s July 2015 planet candidate catalog, which identified 4,302 potential planets. For 1,284 of the candidates, the probability of being a planet is greater than 99 percent – the minimum required to earn the status of “planet.” An additional 1,327 candidates are more likely than not to be actual planets, but they do not meet the 99 percent threshold and will require additional study. The remaining 707 are more likely to be some other astrophysical phenomena. This analysis also validated 984 candidates previously verified by other techniques.

"Before the Kepler space telescope launched, we did not know whether exoplanets were rare or common in the galaxy. Thanks to Kepler and the research community, we now know there could be more planets than stars,” said Paul Hertz, Astrophysics Division director at NASA Headquarters. "This knowledge informs the future missions that are needed to take us ever-closer to finding out whether we are alone in the universe."

Kepler captures the discrete signals of distant planets – decreases in brightness that occur when planets pass in front of, or transit, their stars – much like the May 9 Mercury transit of our sun. Since the discovery of the first planets outside our solar system more than two decades ago, researchers have resorted to a laborious, one-by-one process of verifying suspected planets.

This latest announcement, however, is based on a statistical analysis method that can be applied to many planet candidates simultaneously. Timothy Morton, associate research scholar at Princeton University in New Jersey and lead author of the scientific paper published in The Astrophysical Journal, employed a technique to assign each Kepler candidate a planet-hood probability percentage – the first such automated computation on this scale, as previous statistical techniques focused only on sub-groups within the greater list of planet candidates identified by Kepler.

"Planet candidates can be thought of like bread crumbs,” said Morton. “If you drop a few large crumbs on the floor, you can pick them up one by one. But, if you spill a whole bag of tiny crumbs, you're going to need a broom. This statistical analysis is our broom."

In the newly-validated batch of planets, nearly 550 could be rocky planets like Earth, based on their size. Nine of these orbit in their sun's habitable zone, which is the distance from a star where orbiting planets can have surface temperatures that allow liquid water to pool. With the addition of these nine, 21 exoplanets now are known to be members of this exclusive group.

"They say not to count our chickens before they're hatched, but that's exactly what these results allow us to do based on probabilities that each egg (candidate) will hatch into a chick (bona fide planet)," said Natalie Batalha, co-author of the paper and the Kepler mission scientist at NASA's Ames Research Center in Moffett Field, California. “This work will help Kepler reach its full potential by yielding a deeper understanding of the number of stars that harbor potentially habitable, Earth-size planets -- a number that's needed to design future missions to search for habitable environments and living worlds.”

Of the nearly 5,000 total planet candidates found to date, more than 3,200 now have been verified, and 2,325 of these were discovered by Kepler. Launched in March 2009, Kepler is the first NASA mission to find potentially habitable Earth-size planets. For four years, Kepler monitored 150,000 stars in a single patch of sky, measuring the tiny, telltale dip in the brightness of a star that can be produced by a transiting planet. In 2018, NASA’s Transiting Exoplanet Survey Satellite will use the same method to monitor 200,000 bright nearby stars and search for planets, focusing on Earth and Super-Earth-sized.
 
Ames manages the Kepler missions for NASA’s Science Mission Directorate in Washington. The agency’s Jet Propulsion Laboratory in Pasadena, California, managed Kepler mission development. Ball Aerospace & Technologies Corporation operates the flight system, with support from the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder.

For more information about the Kepler mission, visit:

 
-end-
Felicia Chou
Headquarters, Washington
202-358-0257
felicia.chou@nasa.gov
Michele Johnson
Ames Research Center, Moffett Field, Calif.
650-604-6982
michele.johnson@nasa.gov
Last Updated: May 11, 2016
Editor: Karen Northon
NASA
Guillermo Gonzalo Sánchez Achutegui
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domingo, 8 de mayo de 2016

NASA : NASA to Announce Latest Kepler Discoveries During Media Teleconference .- La NASA Anuncia Los últimos descubrimientos de Kepler Durante la teleconferencia de medios

http://www.nasa.gov/press-release/nasa-to-announce-latest-kepler-discoveries-during-media-teleconference
NASA's planet-hunting mission, the Kepler Space Telescope
NASA's planet-hunter, the Kepler Space Telescope
Credits: NASA

NASA will host a news teleconference at 1 p.m. EDT Tuesday, May 10 to announce the latest discoveries made by its planet-hunting mission, the Kepler Space Telescope.

The briefing participants are:
  • Paul Hertz, Astrophysics Division director at NASA Headquarters in Washington
  • Timothy Morton, associate research scholar at Princeton University in New Jersey
  • Natalie Batalha, Kepler mission scientist at NASA's Ames Research Center in Moffett Field, California
  • Charlie Sobeck, Kepler/K2 mission manager at Ames

For dial-in information, media must e-mail their name, affiliation and telephone number to Felicia Chou at felicia.chou@nasa.gov no later than 11 a.m. Tuesday. Questions can be submitted on Twitter during the teleconference using the hashtag #askNASA.

The teleconference audio and visuals will be streamed live at:


When Kepler was launched in March 2009, scientists did not know how common planets were outside our solar system. Thanks to Kepler’s treasure trove of discoveries, astronomers now believe there may be at least one planet orbiting every star in the sky.

Kepler completed its prime mission in 2012, and collected data for an additional year in an extended mission. In 2014, the spacecraft began a new extended mission called K2. K2 continues the search for exoplanets while introducing new research opportunities to study young stars, supernovae and other cosmic phenomena.

For more information about NASA’s Kepler mission, visit:


-end-
Felicia Chou
Headquarters, Washington
202-358-0257
felicia.chou@nasa.gov

Michele Johnson
Ames Research Center, Moffett Field, Calif.
650-604-6982
michele.johnson@nasa.gov
Last Updated: May 4, 2016
Editor: Karen Northon
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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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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domingo, 1 de mayo de 2016

NASA : Light Echoes Used to Study Protoplanetary Disks .- Los ecos de luz utilizado para estudiar los discos protoplanetarios

Hola amigos: A VUELO DE UN QUINDE EL BLOG., la Agencia Espacial NASA, nos informa sobre : "Un nuevo estudio publicado en la revista Astrophysical Journal utiliza los datos del telescopio espacial Spitzer de la NASA y cuatro telescopios terrestres para determinar la distancia de una estrella hasta el borde interno de su disco protoplanetario que rodea. Los investigadores utilizaron un método llamado "foto-reverberación," también conocido como "ecos de luz." Cuando la estrella central ilumina, algo de la luz golpea el disco circundante, causando un retraso "eco". Los científicos midieron el tiempo necesario para que la luz que viene directamente de la estrella para llegar a la Tierra, y luego esperó a que su eco en llegar............"
More information...........

This illustration shows a star surrounded by a protoplanetary disk
A new study published in the Astrophysical Journal uses data from NASA's Spitzer Space Telescope and four ground-based telescopes to determine the distance from a star to the inner rim of its surrounding protoplanetary disk. Researchers used a method called "photo-reverberation," also known as "light echoes." When the central star brightens, some of the light hits the surrounding disk, causing a delayed “echo.” Scientists measured the time it took for light coming directly from the star to reach Earth, then waited for its echo to arrive.
 
The Spitzer study marks the first time the light echo method was used in the context of protoplanetary disks.
 
This illustration shows a star surrounded by a protoplanetary disk. Material from the thick disk flows along the star’s magnetic field lines and is deposited onto the star’s surface. When material hits the star, it lights up brightly.
Image Credit: NASA/JPL-Caltech
Last Updated: April 26, 2016
Editor: Sarah Loff
NASA
Guillermo Gonzalo Sánchez Achutegui
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domingo, 17 de abril de 2016

NASA : Mission Manager Update: Kepler Remains Stable as Health Check Continues .- Continúa Gestor de actualizaciones Misión: Kepler mantiene estable como chequeo

Hola amigos: A VUELO DE UN QUINDE EL BLOG., La nave espacial Kepler se mantiene estable ya que el proceso de devolverlo a la ciencia continúa. La causa de la anomalía, informó por primera vez el 8 de abril, sigue bajo investigación.
Desde el domingo por la mañana la nave espacial se ha mantenido de manera segura "aparcado" en una configuración en punta estable llamado Punto Resto Estado. En este estado, el consumo de combustible sigue siendo bajo y el enlace de comunicación con la Tierra es buena. A partir del martes, los ingenieros de operaciones de la misión habían enlace descendente todos los datos necesarios de Kepler de triaje la situación y planificar los pasos hacia la recuperación.
More information....

Kepler detecting the brightening of a star

Mission Manager Update: Kepler Remains Stable as Health Check Continues

The Kepler spacecraft remains stable as the process of returning it to science continues. The cause of the anomaly, first reported on April 8, remains under investigation.

Since Sunday morning the spacecraft has remained safely "parked" in a stable pointed configuration called Point Rest State. In this state, fuel usage remains low and the communication link to Earth is good. As of Tuesday, mission operations engineers had downlinked all the necessary data from Kepler to triage the situation and plan the steps toward recovery.

The recovery to science began with a thorough assessment of the data, which took a couple days, after which the team had learned all they could about the state of the spacecraft from the data. It was then time to turn back on and test the components deemed low-risk to spacecraft health. Testing begins on the Kepler spacecraft simulator at the flight planning center at Ball Aerospace in Boulder, Colorado. With the ground-based simulation a success, we were ready to conduct the tests on Kepler, 75 million miles away. The engineers sent the instructions, along with commands for the spacecraft to protect itself and enter a safe operating mode if there was a problem, and waited for the spacecraft to report back.

The spacecraft returned a response that is the equivalent of 'so far, so good.' It did not experience any faults from switching on the components, and all the data suggest the components are working normally. The spacecraft is another step closer to returning to scientific observations for the K2 mission.

The photometer – Kepler’s camera – and the solid state recorder are powered on. The subsystem interface box, which is the interface between the spacecraft sensors and the main computer, was only briefly powered on for an initial assessment, but should be back online early next week. The team will continue recovering the components, as they are deemed safe and low-risk to the spacecraft.

Over the weekend, NASA's Deep Space Network (DSN) will remain in contact with the spacecraft while the team gets some much-needed rest. To watch the worldwide array of antennae communicate with the spacecraft, tune-in to DSN Now.

The recovery started slowly and carefully, as we initially merely tried to understand the situation and recover the systems least likely to have been the cause. Over the last day and a half, we’ve begun to turn the corner, by powering on more suspect components. With just one more to go, I expect that we will soon be on the home stretch and picking up speed towards returning to normal science operations.
Updates will be provided as information warrants.
Regards,

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






4/11, Update 1: Kepler Recovered from Emergency and Stable
Mission operations engineers have successfully recovered the Kepler spacecraft from Emergency Mode (EM). On Sunday morning, the spacecraft reached a stable state with the communication antenna pointed toward Earth, enabling telemetry and historical event data to be downloaded to the ground. The spacecraft is operating in its lowest fuel-burn mode.

The mission has cancelled the spacecraft emergency, returning the Deep Space Network ground communications to normal scheduling.

Once data is on the ground, the team will thoroughly assess all on board systems to ensure the spacecraft is healthy enough to return to science mode and begin the K2 mission's microlensing observing campaign, called Campaign 9. This checkout is anticipated to continue through the week.

Earth-based observatories participating in Campaign 9 will continue to make observations as Kepler's health check continues. The K2 observing opportunity for Campaign 9 will end on July 1, when the galactic center is no longer in view from the vantage point of the spacecraft.

K2's previous science campaign concluded on March 23. After data was downlinked to the ground, the spacecraft was placed in what is termed Point Rest State (PRS). While in PRS, the spacecraft antenna is pointed toward Earth and it operates in a fuel-efficient mode, with the reaction wheels at rest.

The Emergency Mode began approximately 14 hours before the planned maneuver to orient the spacecraft toward the center of the Milky Way for Campaign 9. The team has therefore ruled out the maneuver and the reaction wheels as possible causes of the EM event. An investigation into what caused the event will be pursued in parallel, with a priority on returning the spacecraft to science operations.

The anomalous EM event is the first that the Kepler spacecraft has encountered during its seven years in space. Mission operations at NASA's Ames Research Center in California's Silicon Valley, Ball Aerospace and the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder remain vigilant.

It was the quick response and determination of the engineers throughout the weekend that led to the recovery. We are deeply appreciative of their efforts, and for the outpouring of support from the mission's fans and followers from around the world.  We also recognize the tremendous support from NASA’s Deep Space Network, managed by the Jet Propulsion Laboratory in Pasadena, California, and to NASA’s other missions that surrendered their scheduled telemetry links in order to provide us with the resources needed to protect the Kepler spacecraft.

Updates will be provided as information warrants.
Regards,

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






April 8, Original Report: Kepler in Emergency Mode
During a scheduled contact on Thursday, April 7, mission operations engineers discovered that the Kepler spacecraft was in Emergency Mode (EM). EM is the lowest operational mode and is fuel intensive. Recovering from EM is the team's priority at this time.

The mission has declared a spacecraft emergency, which provides priority access to ground-based communications at the agency's Deep Space Network.

Initial indications are that Kepler entered EM approximately 36 hours ago, before mission operations began the maneuver to orient the spacecraft to point toward the center of the Milky Way for the K2 mission's microlensing observing campaign.

The spacecraft is nearly 75 million miles from Earth, making the communication slow. Even at the speed of light, it takes 13 minutes for a signal to travel to the spacecraft and back.

The last regular contact with the spacecraft was on April. 4.  The spacecraft was in good health and operating as expected.

Kepler completed its prime mission in 2012, detecting nearly 5,000 exoplanets, of which, more than 1,000 have been confirmed. In 2014 the Kepler spacecraft began a new mission called K2. In this extended mission, K2 continues the search for exoplanets while introducing new research opportunities to study young stars, supernovae, and many other astronomical objects.

Updates will be provided as additional information is available.
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: April 15, 2016
Editor: Michele Johnson
 
Free-floating exoplanet

Searching for Far Out and Wandering Worlds


Astronomers have made great strides in discovering planets outside of our solar system, termed “exoplanets.” In fact, over the past 20 years more than 5,000 exoplanets have been detected beyond the eight planets that call our solar system home.
 
K2 and gravitational microlensing
As an exoplanet passes in front of a more distant star, its gravity causes the trajectory of the starlight to bend, and in some cases results in a brief brightening of the background star as seen by a telescope. The artistic concept illustrates this effect. This phenomenon of gravitational microlensing enables scientists to search for exoplanets that are too distant and dark to detect any other way.
Credits: NASA Ames/JPL-Caltech/T. Pyle
The majority of these exoplanets have been found snuggled up to their host star completing an orbit (or year) in hours, days or weeks, while some have been found orbiting as far as Earth is to the sun, taking one-Earth-year to circle. But, what about those worlds that orbit much farther out, such as Jupiter and Saturn, or, in some cases, free-floating exoplanets that are on their own and have no star to call home? In fact, some studies suggest that there may be more free-floating exoplanets than stars in our galaxy.

This week, NASA's K2 mission, the repurposed mission of the Kepler space telescope, and other ground-based observatories have teamed up to kick-off a global experiment in exoplanet observation. Their mission: survey millions of stars toward the center of our Milky Way galaxy in search of distant stars' planetary outposts and exoplanets wandering between the stars.

While today's planet-hunting techniques have favored finding exoplanets near their sun, the outer regions of a planetary system have gone largely unexplored. In the exoplanet detection toolkit, scientists have a technique well suited to search these farthest outreaches and the space in between the stars. This technique is called gravitational microlensing.


Gravitational Microlensing

For this experiment, astronomers rely on the effect of a familiar fundamental force of nature to help detect the presence of these far out worlds— gravity. The gravity of massive objects such as stars and planets produces a noticeable effect on other nearby objects.

But gravity also influences light, deflecting or warping, the direction of light that passes close to massive objects. This bending effect can make gravity act as a lens, concentrating light from a distant object, just as a magnifying glass can focus the light from the sun. Scientists can take advantage of the warping effect by measuring the light of distant stars, looking for a brightening that might be caused by a massive object, such as a planet, that passes between a telescope and a distant background star. Such a detection could reveal an otherwise hidden exoplanet.
"The chance for the K2 mission to use gravity to help us explore exoplanets is one of the most fantastic astronomical experiments of the decade," said Steve Howell, project scientist for NASA's Kepler and K2 missions at NASA’s Ames Research Center in California's Silicon Valley. "I am happy to be a part of this K2 campaign and look forward to the many discoveries that will be made."
 
K2's Microlensing Search Area - zoom
In a global experiment in exoplanet observation, the K2 mission and Earth-based observatories on six continents will survey millions of stars toward the center of our Milky Way galaxy. Using a technique called gravitational microlensing, scientists will hunt for exoplanets that orbit far from their host star, such as Jupiter is to our sun, and for free-floating exoplanets that wander between the stars. The method allow exoplanets to be found that are up to 10 times more distant than those found by the original Kepler mission, which used the transit technique. The artistic concept illustrates the relative locations of the search areas for NASA's K2 and Kepler missions.
Credits: NASA Ames/W. Stenzel and JPL-Caltech/R. Hurt
 
This phenomenon of gravitational microlensing – “micro” because the angle by which the light is deflected is small – is the effect for which scientists will be looking during the next three months. As an exoplanet passes in front of a more distant star, its gravity causes the trajectory of the starlight to bend, and in some cases results in a brief brightening of the background star as seen by the observatory.
The lensing events caused by a free-floating exoplanet last on the order of a day or two, making the continuous gaze of the Kepler spacecraft an invaluable asset for this technique.
"We are seizing the opportunity to use Kepler's uniquely sensitive camera to sniff for planets in a different way," said Geert Barentsen, research scientist at Ames.

The ground-based observatories will record simultaneous measurements of these brief events. From their different vantage points, space and Earth, the measurements can determine the location of the lensing foreground object through a technique called parallax.
“This is a unique opportunity for the K2 mission and ground-based observatories to conduct a dedicated wide-field microlensing survey near the center of our galaxy," said Paul Hertz, director of the astrophysics division in NASA’s Science Mission Directorate at the agency’s headquarters in Washington. "This first-of-its-kind survey serves as a proof of concept for NASA’s Wide-Field Infrared Survey Telescope (WFIRST), which will launch in the 2020s to conduct a larger and deeper microlensing survey. In addition, because the Kepler spacecraft is about 100 million miles from Earth, simultaneous space- and ground-based measurements will use the parallax technique to better characterize the systems producing these light amplifications."
To understand parallax, extend your arm and hold up your thumb. Close one eye and focus on your thumb and then do the same with the other eye. Your thumb appears to move depending on the vantage point. For humans to determine distance and gain depth perception, the vantage points, our eyes, use parallax.

Flipping the Spacecraft

The Kepler spacecraft trails Earth as it orbits the sun and is normally pointed away from Earth during the K2 mission. But this orientation means that the part of the sky being observed by the spacecraft cannot generally be observed from Earth at the same time, since it is mostly in the daytime sky.

To allow simultaneous ground-based observations, flight operations engineers at Ball Aerospace and the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder will perform a maneuver turning the spacecraft around to point the telescope in the forward velocity vector. So, instead of looking towards where it’s been, the spacecraft will look in the direction of where it’s going.

This alignment will yield a viewing opportunity of Earth and the moon as they cross the spacecraft's field of view. On April 14 at 11:50 a.m. PDT (18:50 UT), Kepler will record a full frame image. The result of that image will be released to the public archive in June once the data has been downloaded and processed. Kepler measures the change in brightness of objects and does not resolve color or physical characteristics of an observed object.

Observing from Earth

To achieve the objectives of this important path-finding research and community exercise in anticipation of WFIRST, approximately two-dozen ground-based observatories on six continents will observe in concert with K2. Each will contribute to various aspects of the experiment and will help explore the distribution of exoplanets across a range of stellar systems and distances.

These results will aid in our understanding of both planetary system architectures as well as the frequency of exoplanets throughout our galaxy.

For a complete list of participating observatories, reference the paper that defines the experiment: Campaign 9 of the K2 mission.

During the roughly 80-day observing period or campaign, astronomers hope to discover over 100 lensing events, ten or more of which may have signatures of exoplanets occupying relatively unexplored regimes of parameter space.

Ames 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 Corporation operates the flight system with support from the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder.

 
For more information about the Kepler and K2 missions, visit:

The animation depicts the phenomenon of gravitational microlensing. As an exoplanet passes in front of a more distant star, its gravity causes the trajectory of the starlight to bend, and in some cases results in a brief brightening of the background star as seen by a telescope. Teaming up on a global experiment in exoplanet observation, NASA's K2 mission and Earth-based observatories on six continents will use gravitational microlensing to search for exoplanets that are too distant and dark to detect any other way.
Credits: NASA Ames/JPL-Caltech/T. Pyle



Media contact:

Michele Johnson
Ames Research Center, Moffett Field, Calif.
650-604-6982
michele.johnson@nasa.gov
Last Updated: April 8, 2016
Editor: Michele Johnson
NASA
Guillermo Gonzalo Sánchez Achutegui
Inscríbete en el Foro del blog y participa : A Vuelo De Un Quinde - El Foro!

viernes, 15 de abril de 2016

NASA : Mission Manager Update: Kepler Recovered from Emergency and Stable .- Misión gestor de actualizaciones: Kepler recuperado de Emergencia y Estable



Mission operations engineers have successfully recovered the Kepler spacecraft from Emergency Mode (EM). On Sunday morning, the spacecraft reached a stable state with the communication antenna pointed toward Earth, enabling telemetry and historical event data to be downloaded to the ground. The spacecraft is operating in its lowest fuel-burn mode.

The mission has cancelled the spacecraft emergency, returning the Deep Space Network ground communications to normal scheduling.

Once data is on the ground, the team will thoroughly assess all on board systems to ensure the spacecraft is healthy enough to return to science mode and begin the K2 mission's microlensing observing campaign, called Campaign 9. This checkout is anticipated to continue through the week.

Earth-based observatories participating in Campaign 9 will continue to make observations as Kepler's health check continues. The K2 observing opportunity for Campaign 9 will end on July 1, when the galactic center is no longer in view from the vantage point of the spacecraft.

K2's previous science campaign concluded on March 23. After data was downlinked to the ground, the spacecraft was placed in what is termed Point Rest State (PRS). While in PRS, the spacecraft antenna is pointed toward Earth and it operates in a fuel-efficient mode, with the reaction wheels at rest.

The Emergency Mode began approximately 14 hours before the planned maneuver to orient the spacecraft toward the center of the Milky Way for Campaign 9. The team has therefore ruled out the maneuver and the reaction wheels as possible causes of the EM event. An investigation into what caused the event will be pursued in parallel, with a priority on returning the spacecraft to science operations.

The anomalous EM event is the first that the Kepler spacecraft has encountered during its seven years in space. Mission operations at NASA's Ames Research Center in California's Silicon Valley, Ball Aerospace and the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder remain vigilant.

It was the quick response and determination of the engineers throughout the weekend that led to the recovery. We are deeply appreciative of their efforts, and for the outpouring of support from the mission's fans and followers from around the world.  We also recognize the tremendous support from NASA’s Deep Space Network, managed by the Jet Propulsion Laboratory in Pasadena, California, and to NASA’s other missions that surrendered their scheduled telemetry links in order to provide us with the resources needed to protect the Kepler spacecraft.

Updates will be provided as information warrants.
Regards,

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



Original April 8 Update: Kepler in Emergency Mode
During a scheduled contact on Thursday, April 7, mission operations engineers discovered that the Kepler spacecraft was in Emergency Mode (EM). EM is the lowest operational mode and is fuel intensive. Recovering from EM is the team's priority at this time.

The mission has declared a spacecraft emergency, which provides priority access to ground-based communications at the agency's Deep Space Network.

Initial indications are that Kepler entered EM approximately 36 hours ago, before mission operations began the maneuver to orient the spacecraft to point toward the center of the Milky Way for the K2 mission's microlensing observing campaign.

The spacecraft is nearly 75 million miles from Earth, making the communication slow. Even at the speed of light, it takes 13 minutes for a signal to travel to the spacecraft and back.

The last regular contact with the spacecraft was on April. 4.  The spacecraft was in good health and operating as expected.

Kepler completed its prime mission in 2012, detecting nearly 5,000 exoplanets, of which, more than 1,000 have been confirmed. In 2014 the Kepler spacecraft began a new mission called K2. In this extended mission, K2 continues the search for exoplanets while introducing new research opportunities to study young stars, supernovae, and many other astronomical objects.

Updates will be provided as additional information is available.
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: April 11, 2016
Editor: Michele Johnson
NASA
Guillermo Gonzalo Sánchez Achutegui
Inscríbete en el Foro del blog y participa : A Vuelo De Un Quinde - El Foro!

domingo, 10 de abril de 2016

NASA : Using Starlight to Find Wandering Worlds.- Searching for Far Out and Wandering Worlds .- La búsqueda muy lejos de errante mundos


The animation depicts the phenomenon of gravitational microlensing. As an exoplanet passes in front of a more distant star, its gravity causes the trajectory of the starlight to bend, and in some cases results in a brief brightening of the background star as seen by a telescope. Teaming up on a global experiment in exoplanet observation, NASA's K2 mission and Earth-based observatories on six continents will use gravitational microlensing to search for exoplanets that are too distant and dark to detect any other way.
Credits: NASA Ames/JPL-Caltech/T. Pyle

Media contact:

Michele Johnson
Ames Research Center, Moffett Field, Calif.
650-604-6982
michele.johnson@nasa.gov
Last Updated: April 8, 2016
Editor: Michele Johnson

Searching for Far Out and Wandering Worlds


Astronomers have made great strides in discovering planets outside of our solar system, termed “exoplanets.” In fact, over the past 20 years more than 5,000 exoplanets have been detected beyond the eight planets that call our solar system home.
K2 and gravitational microlensing
As an exoplanet passes in front of a more distant star, its gravity causes the trajectory of the starlight to bend, and in some cases results in a brief brightening of the background star as seen by a telescope. The artistic concept illustrates this effect. This phenomenon of gravitational microlensing enables scientists to search for exoplanets that are too distant and dark to detect any other way.
Credits: NASA Ames/JPL-Caltech/T. Pyle
 
The majority of these exoplanets have been found snuggled up to their host star completing an orbit (or year) in hours, days or weeks, while some have been found orbiting as far as Earth is to the sun, taking one-Earth-year to circle. But, what about those worlds that orbit much farther out, such as Jupiter and Saturn, or, in some cases, free-floating exoplanets that are on their own and have no star to call home? In fact, some studies suggest that there may be more free-floating exoplanets than stars in our galaxy.

This week, NASA's K2 mission, the repurposed mission of the Kepler space telescope, and other ground-based observatories have teamed up to kick-off a global experiment in exoplanet observation. Their mission: survey millions of stars toward the center of our Milky Way galaxy in search of distant stars' planetary outposts and exoplanets wandering between the stars.

While today's planet-hunting techniques have favored finding exoplanets near their sun, the outer regions of a planetary system have gone largely unexplored. In the exoplanet detection toolkit, scientists have a technique well suited to search these farthest outreaches and the space in between the stars. This technique is called gravitational microlensing.


Gravitational Microlensing

For this experiment, astronomers rely on the effect of a familiar fundamental force of nature to help detect the presence of these far out worlds— gravity. The gravity of massive objects such as stars and planets produces a noticeable effect on other nearby objects.

But gravity also influences light, deflecting or warping, the direction of light that passes close to massive objects. This bending effect can make gravity act as a lens, concentrating light from a distant object, just as a magnifying glass can focus the light from the sun. Scientists can take advantage of the warping effect by measuring the light of distant stars, looking for a brightening that might be caused by a massive object, such as a planet, that passes between a telescope and a distant background star. Such a detection could reveal an otherwise hidden exoplanet.
"The chance for the K2 mission to use gravity to help us explore exoplanets is one of the most fantastic astronomical experiments of the decade," said Steve Howell, project scientist for NASA's Kepler and K2 missions at NASA’s Ames Research Center in California's Silicon Valley. "I am happy to be a part of this K2 campaign and look forward to the many discoveries that will be made."
 
K2's Microlensing Search Area - zoom
In a global experiment in exoplanet observation, the K2 mission and Earth-based observatories on six continents will survey millions of stars toward the center of our Milky Way galaxy. Using a technique called gravitational microlensing, scientists will hunt for exoplanets that orbit far from their host star, such as Jupiter is to our sun, and for free-floating exoplanets that wander between the stars. The method allow exoplanets to be found that are up to 10 times more distant than those found by the original Kepler mission, which used the transit technique. The artistic concept illustrates the relative locations of the search areas for NASA's K2 and Kepler missions.
Credits: NASA Ames/W. Stenzel and JPL-Caltech/R. Hurt
 
This phenomenon of gravitational microlensing – “micro” because the angle by which the light is deflected is small – is the effect for which scientists will be looking during the next three months. As an exoplanet passes in front of a more distant star, its gravity causes the trajectory of the starlight to bend, and in some cases results in a brief brightening of the background star as seen by the observatory.
The lensing events caused by a free-floating exoplanet last on the order of a day or two, making the continuous gaze of the Kepler spacecraft an invaluable asset for this technique.
"We are seizing the opportunity to use Kepler's uniquely sensitive camera to sniff for planets in a different way," said Geert Barentsen, research scientist at Ames.

The ground-based observatories will record simultaneous measurements of these brief events. From their different vantage points, space and Earth, the measurements can determine the location of the lensing foreground object through a technique called parallax.
“This is a unique opportunity for the K2 mission and ground-based observatories to conduct a dedicated wide-field microlensing survey near the center of our galaxy," said Paul Hertz, director of the astrophysics division in NASA’s Science Mission Directorate at the agency’s headquarters in Washington. "This first-of-its-kind survey serves as a proof of concept for NASA’s Wide-Field Infrared Survey Telescope (WFIRST), which will launch in the 2020s to conduct a larger and deeper microlensing survey. In addition, because the Kepler spacecraft is about 100 million miles from Earth, simultaneous space- and ground-based measurements will use the parallax technique to better characterize the systems producing these light amplifications."
To understand parallax, extend your arm and hold up your thumb. Close one eye and focus on your thumb and then do the same with the other eye. Your thumb appears to move depending on the vantage point. For humans to determine distance and gain depth perception, the vantage points, our eyes, use parallax.

Flipping the Spacecraft

The Kepler spacecraft trails Earth as it orbits the sun and is normally pointed away from Earth during the K2 mission. But this orientation means that the part of the sky being observed by the spacecraft cannot generally be observed from Earth at the same time, since it is mostly in the daytime sky.

To allow simultaneous ground-based observations, flight operations engineers at Ball Aerospace and the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder will perform a maneuver turning the spacecraft around to point the telescope in the forward velocity vector. So, instead of looking towards where it’s been, the spacecraft will look in the direction of where it’s going.

This alignment will yield a viewing opportunity of Earth and the moon as they cross the spacecraft's field of view. On April 14 at 11:50 a.m. PDT (18:50 UT), Kepler will record a full frame image. The result of that image will be released to the public archive in June once the data has been downloaded and processed. Kepler measures the change in brightness of objects and does not resolve color or physical characteristics of an observed object.

Observing from Earth

To achieve the objectives of this important path-finding research and community exercise in anticipation of WFIRST, approximately two-dozen ground-based observatories on six continents will observe in concert with K2. Each will contribute to various aspects of the experiment and will help explore the distribution of exoplanets across a range of stellar systems and distances.

These results will aid in our understanding of both planetary system architectures as well as the frequency of exoplanets throughout our galaxy.

For a complete list of participating observatories, reference the paper that defines the experiment: Campaign 9 of the K2 misión.

During the roughly 80-day observing period or campaign, astronomers hope to discover over 100 lensing events, ten or more of which may have signatures of exoplanets occupying relatively unexplored regimes of parameter space.

Ames 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 Corporation operates the flight system with support from the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder.

For more information about the Kepler and K2 missions, visit:

NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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