Mostrando entradas con la etiqueta Universe. Mostrar todas las entradas
Mostrando entradas con la etiqueta Universe. Mostrar todas las entradas

jueves, 3 de noviembre de 2016

NASA : James Webb Space Telescope Mirrors Will Piece Together Cosmic Puzzles.- Los espejos del Telescopio Espacial James Webb, Juntos Puzzles Cósmicos

https://www.nasa.gov/image-feature/prototype-capture-system-mock-asteroid-help-simulate-mission-sequence

Webb Telescope honeycomb-shaped primary mirror upright in clean room
The primary mirror of NASA's James Webb Space Telescope consisting of 18 hexagonal mirrors looks like a giant puzzle piece standing in the massive clean room of NASA's Goddard Space Flight Center in Greenbelt, Maryland. Appropriately, combined with the rest of the observatory, the mirrors will help piece together puzzles scientists have been trying to solve throughout the cosmos.
Webb's primary mirror will collect light for the observatory in the scientific quest to better understand our solar system and beyond. Using these mirrors and Webb's infrared vision scientists will peer back over 13.5 billion years to see the first stars and galaxies forming out of the darkness of the early universe. Unprecedented infrared sensitivity will help astronomers to compare the faintest, earliest galaxies to today's grand spirals and ellipticals, helping us to understand how galaxies assemble over billions of years. Webb will see behind cosmic dust clouds to see where stars and planetary systems are being born. It will also help reveal information about atmospheres of planets outside our solar system, and perhaps even find signs of the building blocks of life elsewhere in the universe.
The Webb telescope was mounted upright after a "center of curvature" test conducted at Goddard. This initial center of curvature test ensures the integrity and accuracy, and test will be repeated later to verify those same properties after the structure undergoes launch environment testing. In the photo, two technicians stand before the giant primary mirror.
The Webb telescope is an international collaboration between NASA, the European Space Agency (ESA), and the Canadian Space Agency (CSA).
For information on the Webb's Center of Curvature test, visit:
Image Credit: NASA/Chris Gunn
Caption: Rob Gutro

Last Updated: Nov. 2, 2016
Editor: Sarah Loff
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
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domingo, 17 de julio de 2016

NASA : Hubble Spots a Secluded Starburst Galaxy .- Telescopio Espacial Hubble, descubre una aislada Galaxia Starburst

http://www.nasa.gov/image-feature/goddard/2016/hubble-spots-a-secluded-starburst-galaxy

A starburst galaxy on the left and a star in our own galaxy on the right
This image was taken by the NASA/ESA Hubble Space Telescope’s Advanced Camera for Surveys (ACS) and shows a starburst galaxy named MCG+07-33-027. This galaxy lies some 300 million light-years away from us, and is currently experiencing an extraordinarily high rate of star formation — a starburst. 

Normal galaxies produce only a couple of new stars per year, but starburst galaxies can produce a hundred times more than that. As MCG+07-33-027 is seen face-on, the galaxy’s spiral arms and the bright star-forming regions within them are clearly visible and easy for astronomers to study.

In order to form newborn stars, the parent galaxy has to hold a large reservoir of gas, which is slowly depleted to spawn stars over time. For galaxies in a state of starburst, this intense period of star formation has to be triggered somehow — often this happens due to a collision with another galaxy. MCG+07-33-027, however, is special; while many galaxies are located within a large cluster of galaxies, MCG+07-33-027 is a field galaxy, which means it is rather isolated. Thus, the triggering of the starburst was most likely not due to a collision with a neighboring or passing galaxy and astronomers are still speculating about the cause. The bright object to the right of the galaxy is a foreground star in our own galaxy.

Image credit: ESA/Hubble & NASA and N. Grogin (STScI)
Text credit: European Space Agency
Last Updated: July 15, 2016
Editor: Ashley Morrow
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
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domingo, 19 de junio de 2016

NASA : Hubble Uncovers a Mysterious Hermit .- Telescopio Espacial Hubble descubre un misterioso ermitaño

Hola amigos: A VUELO DE UN QUINDE EL BLOG., la Agencia Espacial NASA, nos informa sobre el descubrimiento del Telescopio Espacial Hubble de un grupo de galaxias.
NASA, nos dice: "La llovizna de estrellas dispersadas a través de esta imagen forma una galaxia conocida como UGC UGC 4879. 4879 es una galaxia enana irregular - como su nombre indica, las galaxias de este tipo son un poco más pequeño y más desordenado que sus primos cósmicos, que carecen de la majestuosa de un remolino espiral o la coherencia de una elíptica.Esta galaxia es también muy aislado. Hay alrededor de 2,3 millones de años luz entre UGC 4879 y su vecino más cercano, Leo A, que es aproximadamente la misma distancia que la que existe entre la galaxia de Andrómeda y la Vía Láctea.El aislamiento de esta galaxia significa que no ha interactuado con cualquier galaxias circundantes, por lo que es un laboratorio ideal para estudiar la formación de estrellas no complicada por las interacciones con otras galaxias. Los estudios de UGC 4879 han revelado una cantidad significativa de la formación de estrellas en los primeros 4 mil millones de años después del Big Bang, seguido de un período de calma 9 mil millones de años extraño en la formación de estrellas que terminó hace 1 mil millones de años por una más reciente re-ignición. La razón de este comportamiento, sin embargo, sigue siendo un misterio, y la galaxia solitaria sigue ofreciendo un amplio material de estudio para los astrónomos que buscan comprender los complejos misterios del nacimiento de las estrellas en el universo........"
More information...........
 

Galaxy UGC 4879
The drizzle of stars scattered across this image forms a galaxy known as UGC 4879. UGC 4879 is an irregular dwarf galaxy — as the name suggests, galaxies of this type are a little smaller and messier than their cosmic cousins, lacking the majestic swirl of a spiral or the coherence of an elliptical.

This galaxy is also very isolated. There are about 2.3 million light years between UGC 4879 and its closest neighbor, Leo A, which is about the same distance as that between the Andromeda Galaxy and the Milky Way.

This galaxy’s isolation means that it has not interacted with any surrounding galaxies, making it an ideal laboratory for studying star formation uncomplicated by interactions with other galaxies. Studies of UGC 4879 have revealed a significant amount of star formation in the first 4 billion years after the Big Bang, followed by a strange 9-billion-year lull in star formation that ended 1 billion years ago by a more recent re-ignition. The reason for this behavior, however, remains mysterious, and the solitary galaxy continues to provide ample study material for astronomers looking to understand the complex mysteries of star birth throughout the universe.
Image credit: NASA/ESA
Text credit: European Space Agency
Last Updated: June 10, 2016
Editor: Ashley Morrow
NASA
Guillermo Gonzalo Sánchez Achutegui

domingo, 15 de mayo de 2016

NASA : Hubble Spies a Spiral Snowflake .- Telescopio Espacial Hubbe, espía lo que parece un copo de nieve; que es la Galaxia Espiral NGC 6814

Hola amigos: A VUELO DE UN QUINDE EL BLOG., la Agencia Espacial NASA, nos informa que el Telescopio Espacial Hubble, ha captado el núcleo de una gigantesca Galaxia Espiral, conocida como : "NGC 6814 tiene un núcleo extremadamente brillante, un signo revelador de que la galaxia es una galaxia Seyfert. Estas galaxias tienen centros muy activos que pueden emitir fuertes explosiones de radiación. El luminoso corazón de NGC 6814 es una fuente altamente variable de la radiación de rayos X, provocando que los científicos sospechan que alberga un agujero negro supermasivo con una masa de unos 18 millones de veces la del sol...."
More information....

Spiral galaxy NGC 6814 with luminous arms and dark dust
Together with irregular galaxies, spiral galaxies make up approximately 60 percent of the galaxies in the local universe. However, despite their prevalence, each spiral galaxy is unique — like snowflakes, no two are alike. This is demonstrated by the striking face-on spiral galaxy NGC 6814, whose luminous nucleus and spectacular sweeping arms, rippled with an intricate pattern of dark dust, are captured in this NASA/ESA Hubble Space Telescope image.
 
NGC 6814 has an extremely bright nucleus, a telltale sign that the galaxy is a Seyfert galaxy. These galaxies have very active centers that can emit strong bursts of radiation. The luminous heart of NGC 6814 is a highly variable source of X-ray radiation, causing scientists to suspect that it hosts a supermassive black hole with a mass about 18 million times that of the sun.
 
As NGC 6814 is a very active galaxy, many regions of ionized gas are studded along its spiral arms. In these large clouds of gas, a burst of star formation has recently taken place, forging the brilliant blue stars that are visible scattered throughout the galaxy.
 
Image credit: ESA/Hubble & NASA; Acknowledgement: Judy Schmidt
Text credit: European Space Agency
Last Updated: May 13, 2016
Editor: Ashley Morrow
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
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NASA : Chandra Movie Captures Expanding Debris from a Stellar Explosion .- Telescopio Espacial Chandra, capta en una película los restos de una gran explosión estelar

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, sobre la captación de una película de los restos de una gigantesca explosión estelar, esto fue en Supernova Tycho, que lo hizo el Telescopio Espacial Chandra.
More information.......

Animations of Chandra observations from 2000 through 2015 of the Tycho supernova remnant’s X-ray evolution over time.
When the star that created this supernova remnant exploded in 1572, it was so bright that it was visible during the day. And though he wasn’t the first or only person to observe this stellar spectacle, the Danish astronomer Tycho Brahe wrote a book about his extensive observations of the event, gaining the honor of it being named after him.

In modern times, astronomers have observed the debris field from this explosion − what is now known as Tycho’s supernova remnant − using data from NASA’s Chandra X-ray Observatory, the NSF’s Karl G. Jansky Very Large Array (VLA) and many other telescopes. Today, they know that the Tycho remnant was created by the explosion of a white dwarf star, making it part of the so-called Type Ia class of supernovas used to track the expansion of the Universe.

Since much of the material being flung out from the shattered star has been heated by shock waves − similar to sonic booms from supersonic planes − passing through it, the remnant glows strongly in X-ray light. Astronomers have now used Chandra observations from 2000 through 2015 to create the longest movie of the Tycho remnant’s X-ray evolution over time, using five different images. This shows the expansion from the explosion is still continuing about 450 years later, as seen from Earth’s vantage point roughly 10,000 light years away.

By combining the X-ray data with some 30 years of observations in radio waves with the VLA, astronomers have also produced a movie, using three different images. Astronomers have used these X-ray and radio data to learn new things about this supernova and its remnant.

The researchers measured the speed of the blast wave at many different locations around the remnant. The large size of the remnant enables this motion to be measured with relatively high precision. Although the remnant is approximately circular, there are clear differences in the speed of the blast wave in different regions. The speed in the right and lower right directions is about twice as large as that in the left and the upper left directions. This difference was also seen in earlier observations.

This range in speed of the blast wave’s outward motion is caused by differences in the density of gas surrounding the supernova remnant. This causes an offset in position of the explosion site from the geometric center, determined by locating the center of the circular remnant. The astronomers found that the size of the offset is about 10% of the remnant’s current radius, towards the upper left of the geometric center. The team also found that the maximum speed of the blast wave is about 12 million miles per hour.

Offsets such as this between the explosion center and the geometric center could exist in other supernova remnants. Understanding the location of the explosion center for Type Ia supernovas is important because it narrows the search region for a surviving companion star. Any surviving companion star would help identify the trigger mechanism for the supernova, showing that the white dwarf pulled material from the companion star until it reached a critical mass and exploded. The lack of a companion star would favor the other main trigger mechanism, where two white dwarfs merge causing the critical mass to be exceeded, leaving no star behind.

The significant offset from the center of the explosion to the remnant’s geometric center is a relatively recent phenomenon. For the first few hundred years of the remnant, the explosion’s shock was so powerful that the density of gas it was running into did not affect its motion. The density discrepancy from the left side to the right has increased as the shock moved outwards, causing the offset in position between the explosion center and the geometric center to grow with time. So, if future X-ray astronomers, say 1,000 years from now, do the same observation, they should find a much larger offset.

A paper describing these results has been accepted for publication in The Astrophysical Journal Letters and is available online. The authors are Brian Williams (NASA's Goddard Space Flight Center and Universities Space Research Association), Laura Chomiuk (Michigan State University), John Hewitt (University of North Florida), John Blondin (North Carolina State University), Kazimierz Borkowski (NCSU), Parviz Ghavamian (Towson University), Robert Petre (GSFC), and Stephen Reynolds (NCSU).

NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.


Image credits: X-ray: NASA/CXC/GSFC/B. Williams et al; Optical: DSS; Radio: NSF/NRAO/VLA
For more Chandra images, multimedia and related materials, visit:
Last Updated: May 13, 2016
Editor: Lee Mohon
NASA
Guillermo Gonzalo Sánchez Achutegui
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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 : Hubble Spies the Barred Spiral Galaxy NGC 4394 .- Telescopio Espacial Hubble, espía a la Galaxia NGC 4394

http://www.nasa.gov/image-feature/goddard/2016/hubble-spies-the-barred-spiral-galaxy-ngc-4394

NGC 4394 is the archetypal barred spiral galaxy with spiral arms emerging from the ends of a bar that cuts through the galaxy
Discovered in 1784 by the German–British astronomer William Herschel, NGC 4394 is a barred spiral galaxy situated about 55 million light-years from Earth. The galaxy lies in the constellation of Coma Berenices (Berenice's Hair) and is considered to be a member of the Virgo Cluster.

NGC 4394 is the archetypal barred spiral galaxy, with bright spiral arms emerging from the ends of a bar that cuts through the galaxy’s central bulge. These arms are peppered with young blue stars, dark filaments of cosmic dust, and bright, fuzzy regions of active star formation. At the center of NGC 4394 lies a region of ionized gas known as a low-ionization nuclear emission-line region (LINER). LINERs are active regions that display a characteristic set of emission lines in their spectra— mostly from weakly ionized atoms of oxygen, nitrogen and sulphur.

Although LINER galaxies are relatively common, it’s still unclear where the energy comes from to ionize the gas. In most cases it is thought to be the influence of a black hole at the center of the galaxy, but it could also be the result of a high level of star formation. In the case of NGC 4394, it is likely that gravitational interaction with a nearby neighbor has caused gas to flow into the galaxy’s central region, providing a new reservoir of material to fuel the black hole or to make new stars.
Text credit: European Space Agency
Image credit: ESA/Hubble & NASA, Acknowledgement: Judy Schmidt
Last Updated: May 6, 2016
Editor: Ashley Morrow
NASA
Guillermo Gonzalo Sánchez Achutegui
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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
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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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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