Mostrando entradas con la etiqueta The sky. Mostrar todas las entradas
Mostrando entradas con la etiqueta The sky. Mostrar todas las entradas

jueves, 5 de diciembre de 2013

NASA : X-ray Binary Circinus X-1


X-ray Binary Circinus X-1
The youngest member of an important class of objects has been found using data from NASA's Chandra X-ray Observatory and the Australia Compact Telescope Array. A composite image shows the X-rays in blue and radio emission in purple, which have been overlaid on an optical field of view from the Digitized Sky Survey. This discovery, described in the press release, allows scientists to study a critical phase after a supernova and the birth of a neutron star.
Systems known as "X-ray binaries" are some of the brightest X-ray sources in the sky. They consist of either an ultra-dense star packed with neutrons --- a.k.a., a "neutron star" --- or a black hole that is paired with a normal star like the sun. As these two objects orbit one another, the neutron star or black hole pulls material from the companion star onto it.
A new study shows that the X-ray binary called Circinus X-1 is less than 4,600 years old, making it the youngest ever seen. Astronomers have detected hundreds of X-ray binaries throughout the Milky Way and other nearby galaxies. However, these older X-ray binaries only reveal information about what happens later in the evolution of these systems.
Astronomers were able to determine the age of Circinus X-1 by examining material around the orbiting pair. While the source itself has been known for decades, the neutron star is usually so bright that the glare from its X-ray light overwhelms any faint emission surrounding it. The new Chandra data were obtained while the neutron star was in a very faint state, which meant it was dim enough for astronomers to detect the faint afterglow created by the supernova explosion plowing through the surrounding interstellar gas. This, combined with characteristics of the radio emission, allowed the researchers to pinpoint the age of the supernova remnant. In turn, this information reveals the age of the neutron star since they were formed at the same time.
These results have been published in the December 4th issue of The Astrophysical Journal. In addition to those mentioned above, the other authors on this paper are Peter Jonker of the SRON Netherlands Institute for Space Research, Niel Brandt of Penn State University, Daniel Emilio Calvelo-Santos of the University of Southampton, Tasso Tzioumis of the Australia Telescope National Facility, Michael Nowak and Norbert Schultz of the Kavli Institute/MIT, Rudy Wijnands and Michiel van der Klis of the University of Amsterdam.
Image credit: X-ray: NASA/CXC/Univ. of Wisconsin-Madison/S. Heinz et al; Optical: DSS; Radio: CSIRO/ATNF/ATCA
 
NASA
Guillermo Gonzalo Sánchez Achutegui

domingo, 8 de septiembre de 2013

NASA - INFOGRAPHIC] Precision Pointing: It's a Matter of Scale


[INFOGRAPHIC] Precision Pointing: It's a Matter of Scale
Image credit: NASA Ames/Wendy Stenzel
For four years, the Kepler spacescraft continuously and simulatenously observed and collected data on more than 150,000 stars. Its mission-- to determine if Earth-size planets orbiting in the habitable zone of stars like our sun are common or rare.
The stability of Kepler's pointing is measured in degrees, arcminutes, arcseconds and milli-arcseconds. To put that into perspective, the image compares the measurements using a movie theatre screen, a small bag of popcorn, a kernel of corn and a grain of salt.
During the four years of science operations, the pointing precision of the spacecraft was controlled to within a few milli-arcseconds. That is the equivalent of keeping your gaze steady on a grain of salt from a quarter mile away.
The next time you're asked to pass the salt think of the Kepler space telescope, and share its story.

NASA
Guillermo Gonzalo Sánchez Achutegui
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ayabaca@hotmail.com
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lunes, 26 de agosto de 2013

nsf.gov - Is it a bird, a plane, a UFO? It's a...red sprite

Strange lights in the sky studied by atmospheric scientists
A sky with red sprites
Red sprites, these strange lights in the sky are called; they form above thunderstorms.
Credit and Larger Version
August 26, 2013
Is it a bird, is it a plane, is it a UFO? Strange lights in the sky are being closely watched by atmospheric scientists.
Dubbed red sprites by researchers, these dancing fairies-of-the-clouds are sometimes glimpsed as blood-red bursts of light in the shape of jellyfish.
At other times, they appear as trumpet-shaped blue emissions, called blue jets. Like the most elusive of nymphs, however, red sprites and blue jets come out on only one occasion: during severe thunderstorms.
Although sporadically reported for years by airline pilots, only in the past decade or two has there been enough evidence to convince atmospheric scientists to investigate the phenomenon.
 
What's that in the skies?
Now baffled researchers asking "What in the world is this?" may have found answers.
Above a thunderstorm's black clouds, sprites appear as bursts of red light flashing far into Earth's atmosphere, according to scientist Hans Nielsen of the University of Alaska at Fairbanks.
The brief flashes look like glowing jellyfish, with red bells and purple tentacles. In a single night, a large thunderstorm system can emit up to one hundred sprites.
Into the wild blue--or red--yonder
Nielsen, Jason Ahrns, also of the University of Alaska at Fairbanks, Matthew McHarg of the U.S. Air Force Academy and researchers from Fort Lewis College teamed up this summer to study sprites.
They used the National Science Foundation (NSF)/National Center for Atmospheric Research Gulfstream-V aircraft, a high-flying plane capable of reaching altitudes of 50,000 feet, to conduct their research. Their project is funded by NSF.
Sprites are similar to lightning, say Nielsen and McHarg, in that they are electrical discharges from the atmosphere.
But while sprites mimic lightning "in some ways," says McHarg, "they're different in others. Lightning happens below and within clouds, at altitudes of two to five miles. Sprites occur far above the clouds, at about 50 miles up--10 times higher than lightning."
They're also huge, he says, reaching 30 miles high.
"Red sprites don't last very long, though, about one-one thousandth of a second. That's 300 times quicker than the time it takes us to blink!"
Blue jets, which weren't directly part of the scientists' study, stick around longer than red sprites, originate at the tops of storm clouds, and shoot up to an altitude less than half that of red sprites. Blue jets are narrower than red sprites, and fan out like trumpet-shaped flowers in blue or purple hues.
"This field of research is fast evolving, and is important for understanding the global electric circuit," says Anne-Marie Schmoltner, program director in NSF's Division of Atmospheric and Geospace Sciences, which supports the research. "The red sprite airborne field campaign this summer provided observations at unprecedented time resolutions."
 
What makes thunderstorms' celestial lights
Atmospheric researchers have developed theories to try to explain these celestial lights.
Red sprites may happen at the time of positively charged cloud-to-ground lightning strikes, which make up about ten percent of all lightning and are many times more powerful than more common, negatively charged lightning.
The flashes may be akin to giant electric sparks.
After a powerful ground strike, the electric field above a thunderstorm may become strengthened to the point that it causes an "electrical breakdown," an overload that weakens the atmosphere's resistance to electric current flow. The result is an immense red spark, or sprite, in the atmosphere.
Although still something of a mystery, red sprites have helped solve other long-standing questions.
Scientists have found that red sprites create some of the low-frequency radio bursts picked up for years by instruments around the world, but whose source was unknown.
Large bursts of gamma rays, emanating from Earth rather than space, originate during thunderstorms, although their exact relationship to red sprites remains unclear.
Researchers now wonder whether red sprites (and blue jets) might affect the atmosphere in important ways.
For example, sprites and jets might alter the chemical composition of the upper atmosphere. Though brief, they could set off lasting charges.
Sprites' deep red color is caused by the light emitted from nitrogen molecules in the atmosphere, says McHarg. Red sprites may turn out to be important to atmospheric chemistry and global climate by changing concentrations of nitric oxides high in the atmosphere.
The researchers are using a technique called high-speed spectroscopy to study sprites' different colors to determine the amount of energy the sprites carry, and to find out more about their chemical composition.
 
How to see a sprite
Can thunderstorm-watchers on the ground glimpse red sprites and blue jets with the naked eye? Yes, if they know where to look.
Viewers must be able to see a distant thunderstorm with no clouds in the way, in an area without city lights. Then they must look above the storm, not at the lightning within the clouds.
It's likely, say the scientists, that if watchers wait long enough, they'll see a red sprite. Blue jets are more elusive. The best viewing would probably come from a plane flying very high, and located miles and miles away from a thunderstorm.
With its rubber tires, a car may be the safest vehicle from which to hunt for ephemeral sprites of the thunderclouds.
-- Cheryl Dybas, NSF (703) 292-7734 cdybas@nsf.gov
Investigators Hans Nielsen
Related Institutions/Organizations University of Alaska Fairbanks Campus
Total Grants $225,880
Related WebsitesNSF News: Lightning's Mirror Image ... Only Much Bigger:
 http://www.nsf.gov/news/news_summ.jsp?cntn_id=115440
sky with red sprites
One-one thousandth of a second: How long red sprites last, faster than our blinking time.
Credit and Larger Version
Sky with red sprites resembling glowing jellyfish
Red sprites can resemble glowing jellyfish, with structures like bells and tentacles.
Credit and Larger Version
Above a thunderstorm's black clouds, red sprites mimic lightning.
Above a thunderstorm's black clouds, red sprites (upper right corner) mimic lightning.
Credit and Larger Version
Scientists next to the NSF/NCAR Gulfstream-V aircraft.
The scientists conducted their research aboard the NSF/NCAR Gulfstream-V aircraft.
Credit and Larger Version
Blue jets ona  dark sky
Other NSF-funded research has tracked blue jets, close relatives of red sprites.
Credit and Larger Vers
 
The National Science Foundation (NSF).-

lunes, 5 de noviembre de 2012

ESA - Space Science - Opening the curtains at Concordia


Aurora over the south pole
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 The aurora australis, or southern lights, snakes across the permanently dark winter skies of the south pole above the Concordia research station. The misty red band of light known as the Milky Way rises high into the sky. 
Stars appear slightly smeared due to the rotation of Earth during the exposure of the image.
The image was taken on 18 July 2012 and first published on ESA’s Concordia blog
Credits: ESA/IPEV/ENEAA/A. Kumar & E. Bondoux

Set against a star-studded backdrop and a splash of the Milky Way, the green glow of an auroral curtain pervades the permanently dark winter skies of the South Pole.

The only sign of life here is the Concordia research station that ESA uses to prepare for future long-duration missions beyond Earth. The site also caters to scientific research from geology and glaciology to climate change, astronomy and planetary magnetic fields.
Even though the Sun barely peeks above the horizon for months on end, its effects are still played out with the fleeting visit of the aurora australis, or southern lights (at the North Pole they are known as aurora borealis, or the northern lights).
These colourful displays are produced when electrically charged particles travelling from the Sun in the solar wind are channelled along Earth’s magnetic field lines and strike atoms high in the atmosphere.
The colours correspond to collisions with different gases in the atmosphere at different altitudes. Collisions with oxygen atoms typically generate green aurora, while nitrogen lights up the sky in red.
This auroral curtain is snaking towards the misty band of light known as the Milky Way, which rises high into the sky.
Since our Solar System resides inside the Milky Way Galaxy, this bright streak is the edge-on view towards the highly populated centre.
The patchy nature of the swath traces sites of rich star formation interspersed with dark ‘holes’ of obscuring clouds of dust.
This image was taken on 18 July by scientists stationed at the Concordia research base during southern hemisphere winter.
Situated 3200 m above sea level, and with an average temperature of –51°C during the permanently dark winter months, Concordia provides the ideal conditions to study the effects of prolonged isolation in an extremely hostile environment.
Lessons learnt here will help to prepare future astronauts for possible future interplanetary exploration to Mars or beyond.  
ESA
Guillermo Gonzalo Sánchez Achutegui
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miércoles, 13 de junio de 2012

Astronomy: The Veil Nebula



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NASA
 Guillermo Gonzalo Sánchez Achutegui
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jueves, 7 de junio de 2012

Astronomy: NASA'S Spitzer Finds First Objects Burned Furiously

Hi My Friends: A VUELO DE UN QUINDE EL BLOG., he faint, lumpy glow given off by the very first objects in the universe may have been detected with the best precision yet, using NASA's Spitzer Space Telescope. These faint objects might be wildly massive stars or voracious black holes. They are too far away to be seen individually, but Spitzer has captured new, convincing evidence of what appears to be the collective pattern of their infrared light.
 These two panels show the same slice of sky in the constellation Boötes, dubbed the "Extended Groth Strip." The area covered is about 1 by 0.12 degrees. Image credit: NASA/JPL-Caltech/GSFC › Full image and caption

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PASADENA, Calif. -- The faint, lumpy glow given off by the very first objects in the universe may have been detected with the best precision yet, using NASA's Spitzer Space Telescope. These faint objects might be wildly massive stars or voracious black holes. They are too far away to be seen individually, but Spitzer has captured new, convincing evidence of what appears to be the collective pattern of their infrared light.
The observations help confirm the first objects were numerous in quantity and furiously burned cosmic fuel.
"These objects would have been tremendously bright," said Alexander "Sasha" Kashlinsky of NASA's Goddard Space Flight Center in Greenbelt, Md., lead author of a new paper appearing in The Astrophysical Journal. "We can't yet directly rule out mysterious sources for this light that could be coming from our nearby universe, but it is now becoming increasingly likely that we are catching a glimpse of an ancient epoch. Spitzer is laying down a roadmap for NASA's upcoming James Webb Telescope, which will tell us exactly what and where these first objects were."
Spitzer first caught hints of this remote pattern of light, known as the cosmic infrared background, in 2005, and again with more precision in 2007. Now, Spitzer is in the extended phase of its mission, during which it performs more in-depth studies on specific patches of the sky. Kashlinsky and his colleagues used Spitzer to look at two patches of sky for more than 400 hours each.
The team then carefully subtracted all the known stars and galaxies in the images. Rather than being left with a black, empty patch of sky, they found faint patterns of light with several telltale characteristics of the cosmic infrared background. The lumps in the pattern observed are consistent with the way the very distant objects are thought to be clustered together.
Kashlinsky likens the observations to looking for Fourth of July fireworks in New York City from Los Angeles. First, you would have to remove all the foreground lights between the two cities, as well as the blazing lights of New York City itself. You ultimately would be left with a fuzzy map of how the fireworks are distributed, but they would still be too distant to make out individually.
"We can gather clues from the light of the universe's first fireworks," said Kashlinsky. "This is teaching us that the sources, or the "sparks," are intensely burning their nuclear fuel."
The universe formed roughly 13.7 billion years ago in a fiery, explosive Big Bang. With time, it cooled and, by around 500 million years later, the first stars, galaxies and black holes began to take shape. Astronomers say some of that "first light" might have traveled billions of years to reach the Spitzer Space Telescope. The light would have originated at visible or even ultraviolet wavelengths and then, because of the expansion of the universe, stretched out to the longer, infrared wavelengths observed by Spitzer.
The new study improves on previous observations by measuring this cosmic infrared background out to scales equivalent to two full moons -- significantly larger than what was detected before. Imagine trying to find a pattern in the noise in an old-fashioned television set by looking at just a small piece of the screen. It would be hard to know for certain if a suspected pattern was real. By observing a larger section of the screen, you would be able to resolve both small- and large-scale patterns, further confirming your initial suspicion.
Likewise, astronomers using Spitzer have increased the amount of sky examined to obtain more definitive evidence of the cosmic infrared background. The researchers plan to explore more patches of sky in the future to gather more clues hidden in the light of this ancient era.
"This is one of the reasons we are building the James Webb Space Telescope," said Glenn Wahlgren, Spitzer program scientist at NASA Headquarters in Washington. "Spitzer is giving us tantalizing clues, but James Webb will tell us what really lies at the era where stars first ignited."
Other authors are Richard Arendt of Goddard and the University of Maryland in Baltimore County; Matt Ashby and Giovanni Fazio of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass.; and John Mather and Harvey Moseley of Goddard. Fazio led the initial observations of these sky fields.
NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for the agency's Science Mission Directorate in Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA.
For more information about Spitzer, visit: http://www.nasa.gov/spitzer
 NASA
Guillermo Gonzao Sánchez Achutegui
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