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

lunes, 8 de agosto de 2016

NASA : ¿Qué Hay Dentro de Ceres? Nuevos Hallazgos con Datos de la Gravedad

https://www.lanasa.net/
 
08.08.16.- En decenas de miles de fotos enviadas por la nave espacial Dawn de la NASA, el interior de Ceres no es visible. Pero los científicos tienen datos poderosos para estudiar la estructura interna de Ceres: el propio movimiento de Dawn.
 
Como la gravedad domina la órbita de Dawn, los científicos pueden medir variaciones de la gravedad de Ceres estudiando los cambios sutiles en el movimiento de la nave espacial. Utilizando datos de Dawn, los científicos han cartografiado las variaciones de la gravedad de Ceres por primera vez, en un estudio publicado en la revista Nature, que proporciona pistas sobre la estructura interna del planeta enano.
 
"Los datos nuevos sugieren que Ceres posee un interior débil, y que el agua y otros materiales ligeros se separaron parcialmente de la roca durante una fase de calentamiento al principio de su historia", dijo Ryan Park, autor del estudio en el Laboratorio de Propulsión a Chorro de la NASA en Pasadena, California.

Este concepto artístico muestra un diagrama de cómo el interior de Ceres podría estar estructurado, según los datos sobre el campo gravitatorio del planeta enano tomados por la misión Dawn de NASA. Image Credit: NASA/JPL-Caltech
 
El campo de gravedad de Ceres se mide mediante el control de las señales de radio enviadas por Dawn, y luego recibidas en la Tierra, por la Red del Espacio Profundo de la NASA.
 
Ceres tiene una propiedad especial llamada "equilibrio hidrostático", que ha sido confirmada en este estudio.  Esto significa que el interior de Ceres es lo suficientemente débil para que su forma esté gobernada por el modo en que gira. Los científicos alcanzaron esta conclusión comparando el campo gravitatorio de Ceres con su forma. El equilibrio hidrostático de Ceres es una de las razones por la que los astrónomos lo clasificaron como planeta enano en 2006.
 
Los datos indican que Ceres está "diferenciado", lo que significa que tiene varias capas de composiciones diferentes a distintas profundidades, encontrándose la capa más densa en el centro. Los científicos también han averiguado, tal como esperaban, que Ceres es mucho menos denso que la Tierra, la Luna y el asteroide gigante Vesta (el objetivo anterior de Dawn) y otros cuerpos rocosos de nuestro Sistema Solar. Además, se ha sospechado durante mucho tiempo que Ceres contiene materiales de baja densidad como hielo de agua, que el estudio muestra separado del material rocoso y que asciende a la capa más externa junto con otros materiales ligeros.
 
"Hemos descubierto que las divisiones entre las diferentes capas son menos pronunciadas dentro de Ceres que en la Luna y otros planetas en nuestro sistema solar", dijo Park. "La Tierra, con su núcleo metálico, su manto semifluido y corteza exterior, tiene una estructura más claramente definida que Ceres".
 
Los científicos también descubrieron que las áreas de gran elevación en Ceres desplazan la masa en el interior. Esto es análogo a cómo los barcos flotan en el agua: la cantidad de agua desplazada depende en la masa de la embarcación. Del mismo modo, los científicos concluyen que el manto débil de Ceres puede ser empujado a un lado por la masa de montañas y otras características topográficas en la capa más exterior como si las áreas de alta elevación ‘flotasen’ sobre el material. Este fenómeno ha sido observado en otros planetas, incluyendo la Tierra, pero este estudio es el primero en confirmarlo en Ceres.
NASA en español
Guillermo Gonzalo Sánchez Achutegui
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domingo, 20 de septiembre de 2015

NASA :Dawn Takes a Closer Look at Occator .- Satélite Dawn de la NASA, toma una mirada más cercana a Occator

Hola amigos: A VUELO DE UN QUINDE EL BLOG., Esta vista, hecha usando imágenes tomadas por la nave espacial Dawn de la NASA, muestra el cráter Occator en Ceres, el hogar de una colección de puntos brillantes intrigantes.
Los puntos brillantes son mucho más brillante que el resto de la superficie de Ceres, y tienden a aparecer sobreexpuesta en la mayoría de las imágenes. Este punto de vista es un compuesto de dos imágenes de Occator: uno usando una corta exposición que capta el detalle en los puntos brillantes, y uno donde se capta la superficie de fondo en la exposición normal.

More information.....
 http://www.nasa.gov/image-feature/jpl/dawn-takes-a-closer-look-at-occator

Dawn Takes a Closer Look at Occator
This image, made using images taken by NASA's Dawn spacecraft, shows Occator crater on Ceres, home to a collection of intriguing bright spots. 
The bright spots are much brighter than the rest of Ceres' surface, and tend to appear overexposed in most images. This view is a composite of two images of Occator: one using a short exposure that captures the detail in the bright spots, and one where the background surface is captured at normal exposure.
The images were obtained by Dawn during the mission's High Altitude Mapping Orbit (HAMO) phase, from which the spacecraft imaged the surface at a resolution of about 450 feet (140 meters) per pixel.
Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
Last Updated: Sep. 9, 2015
Editor: Martin Perez
Tags:  Ceres, Dawn, Image of the Day
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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domingo, 5 de julio de 2015

NASA : Dawn Survey Orbit Image 11.- Examinar un Amanecer en Orbita con la Imagen 11.....................

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido una rarísima imagen de: Un grupo de puntos brillantes misteriosas en el planeta enano Ceres  de la Agencia Espacial NASA, captada por  NASA's Dawn spacecraft al pequeño planeta Ceres, desde una altitud de 2.700 millas (4400 kilómetros). La imagen, con una resolución de 1.400 pies (410 metros) por píxel, fue tomada el 9 de junio de 2015.

Dwarf planet Ceres
A cluster of mysterious bright spots on dwarf planet Ceres can be seen in this image, taken by NASA's Dawn spacecraft from an altitude of 2,700 miles (4,400 kilometers). The image, with a resolution of 1,400 feet (410 meters) per pixel, was taken on June 9, 2015.
For more information about the Dawn mission, visit:
http://dawn.jpl.nasa.gov.
Image Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
Last Updated: July 5, 2015
Editor: Tony Greicius
Tags:  Ceres, Dawn, Dwarf Planets, Image of the Day, Solar System
NASA
Guillermo Gonzalo Sánchez Achutegui
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ayabaca@hotmail.com
ayabaca@yahoo.com
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domingo, 19 de abril de 2015

NASA : The Solar System and Beyond is Awash in Water .- El Sistema Solar y más allá está inundado de agua

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

Artist's concept of our universe
NASA is exploring our solar system and beyond to understand the workings of the universe, searching for water and life among the stars
Credits: NASA
As NASA missions explore our solar system and search for new worlds, they are finding water in surprising places. Water is but one piece of our search for habitable planets and life beyond Earth, yet it links many seemingly unrelated worlds in surprising ways.
"NASA science activities have provided a wave of amazing findings related to water in recent years that inspire us to continue investigating our origins and the fascinating possibilities for other worlds, and life, in the universe," said Ellen Stofan, chief scientist for the agency. "In our lifetime, we may very well finally answer whether we are alone in the solar system and beyond."
 
La Tierra no es el único mundo océano en nuestro sistema solar. Los océanos podrían existir en diversas formas en las lunas y planetas enanos, ofrecer pistas a la búsqueda para descubrir la vida más allá de nuestro planeta. Esta ilustración representa a los candidatos más conocidos en nuestra búsqueda de vida en el sistema solar.
 
This illustration depicts the best-known candidates in our search for life in the solar system
Earth isn't the only ocean world in our solar system. Oceans could exist in diverse forms on moons and dwarf planets, offering clues in the quest to discover life beyond our home planet. This illustration depicts the best known candidates in our search for life in the solar system.
 
 
 
 
Credits: NASA/JPL-Caltech
 
 
 
The chemical elements in water, hydrogen and oxygen, are some of the most abundant elements in the universe. Astronomers see the signature of water in giant molecular clouds between the stars, in disks of material that represent newborn planetary systems, and in the atmospheres of giant planets orbiting other stars.
There are several worlds thought to possess liquid water beneath their surfaces, and many more that have water in the form of ice or vapor. Water is found in primitive bodies like comets and asteroids, and dwarf planets like Ceres. The atmospheres and interiors of the four giant planets -- Jupiter, Saturn, Uranus and Neptune -- are thought to contain enormous quantities of the wet stuff, and their moons and rings have substantial water ice.
Perhaps the most surprising water worlds are the five icy moons of Jupiter and Saturn that show strong evidence of oceans beneath their surfaces: Ganymede, Europa and Callisto at Jupiter, and Enceladus and Titan at Saturn.
Scientists using NASA's Hubble Space Telescope recently provided powerful evidence that Ganymede has a saltwater, sub-surface ocean, likely sandwiched between two layers of ice.
Europa and Enceladus are thought to have an ocean of liquid water beneath their surface in contact with mineral-rich rock, and may have the three ingredients needed for life as we know it: liquid water, essential chemical elements for biological processes, and sources of energy that could be used by living things. NASA's Cassini mission has revealed Enceladus as an active world of icy geysers. Recent research suggests it may have hydrothermal activity on its ocean floor, an environment potentially suitable for living organisms.
NASA spacecraft have also found signs of water in permanently shadowed craters on Mercury and our moon, which hold a record of icy impacts across the ages like cryogenic keepsakes.
While our solar system may seem drenched in some places, others seem to have lost large amounts of water.
On Mars, NASA spacecraft have found clear evidence that the Red Planet had water on its surface for long periods in the distant past. NASA's Curiosity Mars Rover discovered an ancient streambed that existed amidst conditions favorable for life as we know it.
More recently, NASA scientists using ground-based telescopes were able to estimate the amount of water Mars has lost over the eons. They concluded the planet once had enough liquid water to form an ocean occupying almost half of Mars' northern hemisphere, in some regions reaching depths greater than a mile (1.6 kilometers). But where did the water go?
It's clear some of it is in the Martian polar ice caps and below the surface. We also think much of Mars' early atmosphere was stripped away by the wind of charged particles that streams from the sun, causing the planet to dry out. NASA's MAVEN mission is hard at work following this lead from its orbit around Mars.
The story of how Mars dried out is intimately connected to how the Red Planet's atmosphere interacts with the solar wind. Data from the agency's solar missions -- including STEREO, Solar Dynamics Observatory and the planned Solar Probe Plus -- are vital to helping us better understand what happened.
Understanding the distribution of water in our solar system tells us a great deal about how the planets, moons, comets and other bodies formed 4.5 billion years ago from the disk of gas and dust that surrounded our sun. The space closer to the sun was hotter and drier than the space farther from the sun, which was cold enough for water to condense. The dividing line, called the "frost line," sat around Jupiter's present-day orbit. Even today, this is the approximate distance from the sun at which the ice on most comets begins to melt and become "active." Their brilliant spray releases water ice, vapor, dust and other chemicals, which are thought to form the bedrock of most worlds of the frigid outer solar system.
Scientists think it was too hot in the solar system's early days for water to condense into liquid or ice on the inner planets, so it had to be delivered -- possibly by comets and water-bearing asteroids. NASA's Dawn mission is currently studying Ceres, which is the largest body in the asteroid belt between Mars and Jupiter. Researchers think Ceres might have a water-rich composition similar to some of the bodies that brought water to the three rocky, inner planets, including Earth.
The amount of water in the giant planet Jupiter holds a critical missing piece to the puzzle of our solar system's formation. Jupiter was likely the first planet to form, and it contains most of the material that wasn't incorporated into the sun. The leading theories about its formation rest on the amount of water the planet soaked up. To help solve this mystery, NASA's Juno mission will measure this important quantity beginning in mid-2016.
Looking further afield, observing other planetary systems as they form is like getting a glimpse of our own solar system's baby pictures, and water is a big part of that story. For example, NASA's Spitzer Space Telescope has observed signs of a hail of water-rich comets raining down on a young solar system, much like the bombardment planets in our solar system endured in their youth.
With the study of exoplanets -- planets that orbit other stars -- we are closer than ever to finding out if other water-rich worlds like ours exist. In fact, our basic concept of what makes planets suitable for life is closely tied to water: Every star has a habitable zone, or a range of distances around it in which temperatures are neither too hot nor too cold for liquid water to exist. NASA's planet-hunting Kepler mission was designed with this in mind. Kepler looks for planets in the habitable zone around many types of stars.
Recently verifying its thousandth exoplanet, Kepler data confirm that the most common planet sizes are worlds just slightly larger than Earth. Astronomers think many of those worlds could be entirely covered by deep oceans. Kepler's successor, K2, continues to watch for dips in starlight to uncover new worlds.
The agency's upcoming TESS mission will search nearby, bright stars in the solar neighborhood for Earth- and super-Earth-sized exoplanets. Some of the planets TESS discovers may have water, and NASA's next great space observatory, the James Webb Space Telescope, will examine the atmospheres of those special worlds in great detail.
It's easy to forget that the story of Earth's water, from gentle rains to raging rivers, is intimately connected to the larger story of our solar system and beyond. But our water came from somewhere -- every world in our solar system got its water from the same shared source. So it's worth considering that the next glass of water you drink could easily have been part of a comet, or an ocean moon, or a long-vanished sea on the surface of Mars. And note that the night sky may be full of exoplanets formed by similar processes to our home world, where gentle waves wash against the shores of alien seas.
For more information about NASA's exploration of the solar system and beyond, visit:
Preston Dyches
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-7013
preston.dyches@jpl.nasa.gov
 
Felicia Chou
NASA Headquarters, Washington
202-358-0257
Felicia.chou@nasa.gov
2015-119
NASA
Guillermo Gonzalo Sánchez Achutegui
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martes, 17 de febrero de 2015

NASA : Dawn Approaches: Two Faces of Ceres .- Enfoques la sonda Dawn: dos caras de Ceres

Hola amigos: A VUELO DE UN QUINDE EL BLOG., la Agencia Espacial NASA, nos informa que la nave : NASA's Dawn spacecraft, ha captado la imagen del planeta enano o asteroide Ceres, que se encuentra en la órbita de Marte y Júpiter, que ha sido enfocado por ambas caras, está ubicado el llamado : Cinturón de Asteroides, siendo Ceres el más grande de los todos los asteroides del Sistema Solar.
Comparación de Ceres entre La Tierra y la Luna (Wikipedia.
Imagen esquemática del cinturón de asteroides. Se muestra el cinturón principal, entre las órbitas de Marte y Júpiter, y el grupo de los troyanos, en la órbita de Júpiter
El cinturón de asteroides es una región del Sistema Solar comprendida aproximadamente entre las órbitas de Marte y Júpiter. Alberga multitud de objetos irregulares, denominados asteroides, y al planeta enano Ceres. Esta región también se denomina cinturón principal con la finalidad de distinguirla de otras agrupaciones de cuerpos menores del Sistema Solar, como el cinturón de Kuiper o la nube de Oort.
Wikipedia.
 
Dawn Approaches: Two Faces of Ceres
These two views of Ceres were acquired by NASA's Dawn spacecraft on Feb. 12, 2015, from a distance of about 52,000 miles (83,000 kilometers) as the dwarf planet rotated. The images have been magnified from their original size.
The Dawn spacecraft is due to arrive at Ceres on March 6, 2015.
 
Dawn's mission to Vesta and Ceres is managed by the Jet Propulsion Laboratory for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. UCLA is responsible for overall Dawn mission science. Orbital ATK, Inc., of Dulles, Virginia, designed and built the spacecraft. JPL is managed for NASA by the California Institute of Technology in Pasadena. The framing cameras were provided by the Max Planck Institute for Solar System Research, Göttingen, Germany, with significant contributions by the German Aerospace Center (DLR) Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig. The visible and infrared mapping spectrometer was provided by the Italian Space Agency and the Italian National Institute for Astrophysics, built by Selex ES, and is managed and operated by the Italian Institute for Space Astrophysics and Planetology, Rome. The gamma ray and neutron detector was built by Los Alamos National Laboratory, New Mexico, and is operated by the Planetary Science Institute, Tucson, Arizona.
Image Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
 
Dawn Delivers New Image of Ceres
Dawn spacecraft observed Ceres for an hour on Jan. 13, 2015
The Dawn spacecraft observed Ceres for an hour on Jan. 13, 2015, from a distance of 238,000 miles (383,000 kilometers). A little more than half of its surface was observed at a resolution of 27 pixels. This animated GIF shows bright and dark features.
Image Credit: 
NASA/JPL-Caltech/UCLA/MPS/DLR/IDA/PSI
 
Ceres
This processed image, taken Jan. 13, 2015, shows the dwarf planet Ceres as seen from the Dawn spacecraft. The image hints at craters on the surface of Ceres. Dawn's framing camera took this image at 238,000 miles (383,000 kilometers) from Ceres.
Image Credit: 
NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
 
Ceres
This is a raw image, taken Jan. 13, 2015, showing the dwarf planet Ceres as seen from the Dawn spacecraft on its approach. Dawn's framing camera took this image at 238,000 miles (383,000 kilometers) from Ceres.
Image Credit: 
NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
 
Ceres
This is a zoomed-in raw image, taken Jan. 13, 2015, showing the dwarf planet Ceres as seen from the Dawn spacecraft on its approach. Surface features have started to become apparent in the image. Dawn's framing camera took this image at 238,000 miles (383,000 kilometers) from Ceres.
Image Credit: 
NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
 
As NASA's Dawn spacecraft closes in on Ceres, new images show the dwarf planet at 27 pixels across, about three times better than the calibration images taken in early December. These are the first in a series of images that will be taken for navigation purposes during the approach to Ceres.
 
Over the next several weeks, Dawn will deliver increasingly better and better images of the dwarf planet, leading up to the spacecraft's capture into orbit around Ceres on March 6. The images will continue to improve as the spacecraft spirals closer to the surface during its 16-month study of the dwarf planet.
“We know so little about dwarf planet Ceres. Now, Dawn is ready to change that," said Marc Rayman, Dawn's chief engineer and mission director, based at NASA's Jet Propulsion Laboratory in Pasadena, California.
The best images of Ceres so far were taken by NASA's Hubble Space Telescope in 2003 and 2004. This most recent images from Dawn, taken January 13, 2015, at about 80 percent of Hubble resolution, are not quite as sharp. But Dawn's images will surpass Hubble's resolution at the next imaging opportunity, which will be at the end of January.
 
“Already, the [latest] images hint at first surface structures such as craters," said Andreas Nathues, lead investigator for the framing camera team at the Max Planck Institute for Solar System Research, Gottingen, Germany.
Ceres is the largest body in the main asteroid belt, which lies between Mars and Jupiter. It has an average diameter of 590 miles (950 kilometers), and is thought to contain a large amount of ice. Some scientists think it's possible that the surface conceals an ocean.
 
Dawn's arrival at Ceres will mark the first time a spacecraft has ever visited a dwarf planet.
"The team is very excited to examine the surface of Ceres in never-before-seen detail," said Chris Russell, principal investigator for the Dawn mission, based at the University of California, Los Angeles. "We look forward to the surprises this mysterious world may bring." 
The spacecraft has already delivered more than 30,000 images and many insights about Vesta, the second most massive body in the asteroid belt. Dawn orbited Vesta, which has an average diameter of 326 miles (525 kilometers), from 2011 to 2012. Thanks to its ion propulsion system, Dawn is the first spacecraft ever targeted to orbit two deep-space destinations.
JPL manages the Dawn mission for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. The University of California, Los Angeles (UCLA) is responsible for overall Dawn mission science. Orbital Sciences Corp. in Dulles, Virginia, designed and built the spacecraft. The Dawn framing cameras were developed and built under the leadership of the Max Planck Institute for Solar System Research, Gottingen, Germany, with significant contributions by German Aerospace Center (DLR), Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig. The Framing Camera project is funded by the Max Planck Society, DLR, and NASA/JPL. The Italian Space Agency and the Italian National Astrophysical Institute are international partners on the mission team.
More information about Dawn is online at
NASA
Guillermo Gonzalo Sánchez Achutegui
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jueves, 1 de enero de 2015

NASA: Ceres, Target of NASA's Dawn Mission

Hola amigos: A VUELO DE UN QUINDE EL BLOG., Hemos recibido de la Agencia Espacial NASA, la información sobre el objetivo de la Misión: NASA's Dawn misión, en enfocar al asteroide Ceres, que está ubicado en el llamado Cinturón de Asteroides, una franja del Sistema Solar entre Marte y Júpiter.
Ceres, Target of NASA's Dawn Mission
 
Discovered on Jan. 1, 1801 by Giuseppe Piazzi of Italy, Ceres is the largest object in the asteroid belt - the strip of solar system real estate between Mars and Jupiter. On March 6, 2015, NASA's Dawn spacecraft will arrive at Ceres, marking the first time that a spacecraft has ever orbited two solar system targets. Dawn previously explored the protoplanet Vesta for 14 months, from 2011 to 2012, capturing detailed images and data about that body. Dawn has entered its approach phase toward Ceres, and the next couple of months promise continually improving views prior to arrival. By the end of January, the spacecraft's images and other data will be the best ever taken of the dwarf planet.
This image of Ceres was taken by the Advanced Camera for Surveys on NASA's Hubble Space Telescope between December 2003 and January 2004. Hubble images of Vesta and Ceres helped astronomers plan for the Dawn spacecraft’s tour. Astronomers enhanced the sharpness in the image to bring out features on Ceres' surface, including brighter and darker regions that could be asteroid impact features. The observations were made in visible and ultraviolet light.
The colors represent the differences between relatively red and blue regions. These differences may simply be due to variation on the surface among different types of material. Ceres' round shape suggests that its interior is layered like those of terrestrial planets such as Earth. Ceres may have a rocky inner core, an icy mantle, and a thin, dusty outer crust inferred from its density and rotation rate of 9 hours. Ceres is approximately 590 miles (950 kilometers) across.
Image Credit: NASA/ESA/J. Parker (SWRI), P. Thomas (Cornell U.), L. McFadden (U-Md., College Park), and M. Mutchler and Z. Levay (STScI)
NASA
Guillermo Gonzalo Sánchez Achutegui
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