Mostrando entradas con la etiqueta "Wise". Mostrar todas las entradas
Mostrando entradas con la etiqueta "Wise". Mostrar todas las entradas

jueves, 18 de febrero de 2010

NASA.............PRIMERAS IMÁGENES DEL OBSERVATORIO "WISE" DE LA GALAXIA ANDRÓMEDA

Hola amigos: A VUELO DE UN QUINDE EL BLOG; la agencia espacial norteamericana NASA , todos los días nos enriquece con sus nuevos descubrimientos espaciales por medio de sus telescopios y observatorios espaciales, nuevamente el Observatorio WISE o Wide-field Infrared Survey Explorer nos muestra en la imagen de nuestra galaxia vecina ANDRÓMEDA.
La imnesa galaxia Andrómeda , nuestra vecina, también conocida como Messier 31 o simplemente M31, es captada por completo en esta nueva imagen del Explorador de Revisión Amplio de campaña Infrarrojo de la NASA, o WISE. El mosaico cubre un equivalente de área con más de 100 lunas llenas, o cinco grados a través del cielo. WISE ha usado todos los cuatro de sus detectores infrarrojos para capturar este cuadro(imagen) (3.4-y la luz de 4.6 micras es coloreado azul; la luz de 12 micras es verde; y la luz de 22 micras es roja). Toques de luz azules maduran estrellas, mientras el polvo de espectáculo amarillo y rojo acalorado por estrellas recién nacidas, masivas.

Versión de la NASA
In English:

Our Neighbor Andromeda:

The immense Andromeda galaxy, also known as Messier 31 or simply M31, is captured in full in this new image from NASA's Wide-field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4- and 4.6-micron light is colored blue; 12-micron light is green; and 22-micron light is red). Blue highlights mature stars, while yellow and red show dust heated by newborn, massive stars.

Andromeda is the closest large galaxy to our Milky Way galaxy, and is located 2.5 million light-years from our sun. It is close enough for telescopes to spy the details of its ringed arms of new stars and hazy blue backbone of older stars. Also seen in the mosaic are two satellite galaxies, known as M32, located just a bit above Andromeda to the left of center, and the fuzzy blue M110, located below the center of the great spiral arms. These satellites are the largest of several that are gravitationally bound to Andromeda.

The Andromeda galaxy is larger than our Milky Way and contains more stars, but the Milky Way is thought to perhaps have more mass due to its larger proportion of a mysterious substance called dark matter. Both galaxies belong to our so-called Local Group, a collection of more than 50 galaxies, most of which are tiny dwarf systems. In its quest to map the whole sky, WISE will capture the entire Local Group.

Image credit: NASA/JPL-Caltech/UCLA
› Larger image

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

NASA.................PRIMERAS IMÁGENES EN INFRAROJO DEL OBSERVATORIO "WISE", COMETA SIDING SPRING o C/2007 Q3

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido de la NASA una espectacular vista del Cometa conocido como:C/2007 Q3, captada por el Observatorio Wise o Wide-field Infrared Survey Explorer . Este cometa fue descubierto por astrónomos de Australia en 2007 .

Aquí apreciamos en la imagen captada por el WISE o Wide-field Infrared Survey Explorer, del Cometa conocido como :C/2007 Q3, es una bellísima imagen de fotografía espacial en infrarrojo
El Cometa " Siding Spring aparece a través del cielo como un superhéroe en esta nueva imagen infrarroja del WISE Explorador de Revisión Amplio de campaña Infrarrojo de la NASA.

Versión de la NASA
In English:

Visitor from Deep Space
02.17.10


› Larger image
Comet Siding Spring appears to streak across the sky like a superhero in this new infrared image from NASA's Wide-field Infrared Survey Explorer, or WISE. The comet, also known as C/2007 Q3, was discovered in 2007 by observers in Australia. The snowball-like mass of ice and dust spent billions of years orbiting in the deep freeze of the Oort Cloud, a spherical cloud of comets surrounding our solar system. At some point, it got knocked out of this orbit and onto a course that brings it closer to the sun. On October 7, 2009, it passed as close as 1.2 astronomical units from Earth and 2.25 astronomical units from the sun (an astronomical unit is the distance between the sun and Earth).

Now, the comet is leaving the warmer, more hospitable neighborhood of the solar system and heading back out to chillier parts.In this view, longer wavelengths of infrared light are red and shorter wavelengths are blue. The comet appears red because it is more than ten times colder than the surrounding stars, for example, the bright blue star in the foreground.

Colder objects give off more of their light at longer wavelengths. An ice cube, for example, pours out a larger fraction of its light at longer infrared wavelengths than a cup of hot tea emits.A comet like this one can be thought of as a time capsule leftover from the formation of our solar system 4.5 billion years ago. After spending most of its long, lonely life in the darkest, coldest parts of our solar system, it warms up as it approaches the sun.

The sunlight causes it to shed ices and dust in a long tail that trails behind it. Comet Siding Spring, having experienced this "spring" awakening, is glowing in infrared light that WISE can see. Once it moves too far from the sun's warmth and light, it will disappear from view for the foreseeable future.Astronomers will use these measurements to learn about the comet's size, composition, reflectivity, and the size and makeup of the dust particles in its coma (the hazy cloud surrounding its nucleus) and its tail.

WISE data on this and other comets will help unlock clues that lay within these icy time capsules, teaching us about our solar system's evolution.In this image, 3.4-micron light is colored blue; 4.6-micron light is green; 12-micron light is orange; and 22-micron light is red. It was taken on Jan. 10, 2010.
Image credit: NASA/JPL-Caltech/UCLA
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Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com

domingo, 10 de enero de 2010

NASA.......................PRIMERAS IMÁGENES DEL OBSERVATORIO "WISE"

Aquí apreciamos en la imagen a la NEBULOSA "CARINA", parte de esta constelación fue captada por el Observatorio de Rayos Infrarrojos "WISE", se encuentra a 7,500 años luz del sol. Fuente: Wikipedia.

Hola amigos: A VUELO DE UN QUINDE EL BLOG:, hemos recibido de la NASA, las primeras imágenes captadas por el Observatorio de Rayos Infrarrojos WISE".

Esta foto infrarroja de una región en la constelación "Carina " cerca de la Vía Láctea fue tomada un poco después de estar en el espacio por el Observatorio "Wise"del Explorador de Revisión Amplio de campaña Infrarrojo de la NASA "la primera luz" muestra miles de estrellas y cubre un área tres veces el tamaño de la luna. SABIO tomará más de un millón de cuadros similares que cubren el cielo entero.


La imagen fue captada como la nave espacial que enfocó fijamente en una dirección fija, para ayudar calibrar su sistema que señala. La revisión de la misión será hecha mientras el satélite continuamente explora el cielo, y un espejo de exploración interno neutraliza el movimiento crear imágenes de imagen fija. El equipo trabaja ahora para emparejar los movimientos de la nave espacial y el espejo de exploración con precisión.


Esta ocho segunda exposición muestra la luz infrarroja de tres de las cuatro cintas de longitud de onda del WISE: Azul, verde y rojo corresponden a 3.4, 4.6, y 12 micras, respectivamente.


Versión de la NASA

In English:


NASA's WISE Eye Spies First Glimpse of the Starry Sky:


This infrared snapshot of a region in the constellation Carina near the Milky Way was taken shortly after NASA's Wide-field Infrared Survey Explorer (WISE) ejected its cover. Image credit: NASA/JPL-Caltech/UCLA › Full image and caption Infrared all-sky surveying telescope sends back first images from space.


PASADENA, Calif. -- NASA's Wide-field Infrared Survey Explorer, or WISE, has captured its first look at the starry sky that it will soon begin surveying in infrared light.


Launched on Dec. 14, WISE will scan the entire sky for millions of hidden objects, including asteroids, "failed" stars and powerful galaxies. WISE data will serve as navigation charts for other missions, such as NASA's Hubble and Spitzer Space Telescopes, pointing them to the most interesting targets the mission finds.


A new WISE infrared image was taken shortly after the space telescope's cover was removed, exposing the instrument's detectors to starlight for the first time. The picture shows about 3,000 stars in the Carina constellation and can be viewed online at http://www.nasa.gov/mission_pages/WISE/multimedia/wise20100106.html .


The image covers a patch of sky about three times larger than the full moon, and was presented today at the 215th meeting of the American Astronomical Society in Washington. The patch was selected because it does not contain any unusually bright objects, which could damage instrument detectors if observed for too long. The picture was taken while the spacecraft was staring at a fixed patch of sky and is being used to calibrate the spacecraft's pointing system.


When the WISE survey begins, the spacecraft will scan the sky continuously as it circles the globe, while an internal scan mirror counteracts its motion. This allows WISE to take "freeze-frame" snapshots every 11 seconds, resulting in millions of images of the entire sky.


"Right now, we are busy matching the rate of the scan mirror to the rate of the spacecraft, so we will capture sharp pictures as our telescope sweeps across the sky," said William Irace, the mission's project manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif.


To sense the infrared glow of stars and galaxies, the WISE spacecraft cannot give off any detectable infrared light of its own. This is accomplished by chilling the telescope and detectors to ultra-cold temperatures. The coldest of WISE's detectors will operate at less than 8 Kelvin, or minus 445 degrees Fahrenheit.


The first sky survey will be complete in six months, followed by a second scan of one-half of the sky lasting three months. The mission ends when the frozen hydrogen that keeps the instrument cold evaporates away, an event expected to occur in October 2010.


Preliminary survey images are expected to be released six months later, in April 2011, with the final atlas and catalog coming 11 months later, in March 2012. Selected images will be released to the public beginning in February 2010.


JPL manages WISE for NASA's Science Mission Directorate in Washington. The mission was competitively selected under NASA's Explorers Program, managed by NASA's Goddard Space Flight Center in Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory in Logan, Utah, and the spacecraft was built by Ball Aerospace & Technologies Corp. in Boulder, Colo. Science operations and data processing take place at the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena.


More information is online at http://www.nasa.gov/wise

and http://wise.astro.ucla.edu/.

J.D. Harrington 202-358-5241Headquarters, Washington


Whitney Clavin 818-354-4673Jet Propulsion Laboratory, Pasadena, Calif.


2010-005


Guillermo Gonzalo Sánchez Achutegui




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