Friday, January 20, 2012

Taking a picture of a Black Hole

Achieving the unbelievable: taking a picture of a black hole 

- Thu, Jan 19, 2012
Post filled in: Astrophysics, Physics, Space
Courtesy: www.zmescience.com 
Black Holes are the least understood entities, so far, in the Universe. However, if there’s one thing scientists know for sure about them, it’s that they’re the most extreme environment in cosmos. Black Holes have such a powerful, relentless gravity pull that it swallows absolutely everything in its vicinity, even light gets absorbed with zero reflection. This makes it practically invisible, which is why they’re very difficult to study. Scientists  are now set to embark on one of the most ambitious astrophysical ventures in history – taking a picture of a black hole. No, by no means is this a mad science stunt. The greatest minds of the scientific community have pledged their aid for the project and firmly believe this is possible, in an unprecedented worldwide combined effort, which only a few years ago would’ve been considered ludicrous.
“Nobody has ever taken a picture of a black hole,” said Dimitrios Psaltis, an associate professor of astrophysics at the University of Arizona’s Steward Observatory, who along with Daniel Marrone, an assistant professor of astronomy at Steward Observatory, organized a conference in Tucson, Ariz. where the endeavor was announced “We are going to do just that.”
“Even five years ago, such a proposal would not have seemed credible,” added Sheperd Doeleman, assistant director of the Haystack Observatory at Massachusetts Institute of Technology (MIT), who is the principal investigator of the Event Horizon Telescope, as the project is dubbed. “Now we have the technological means to take a stab at it.”
Computer simulation of superheated plasma swirling around the black hole at the center of our galaxy. (Image by Scott Noble/RIT)
Computer simulation of superheated plasma swirling around the black hole at the center of our galaxy. (Image by Scott Noble/RIT)
Einstein’s Theory of Relativity laid the foundation for the postulation of black holes, proving gravity does indeed influence light’s motion. Based on Einstein’s theory, fellow German physicist Karl Schwarzschild found a solution which described the gravitational field of a point mass and a spherical mass. Since then, scientists have observed, measured and conducted experiments for decades with significant breakthroughs, however it was never possible for them to directly observe or image a black hole. But if black holes don’t emit light, how is it possible to image them? Professor Doeleman explains this extremely ingenious project in a masterful way.
“As dust and gas swirls around the black hole before it is drawn inside, a kind of cosmic traffic jam ensues,” Doeleman explained. “Swirling around the black hole like water circling the drain in a bathtub, the matter compresses and the resulting friction turns it into plasma heated to a billion degrees or more, causing it to ‘glow’ – and radiate energy that we can detect here on Earth.”

Capturing the Milky Way’s supermassive black hole halo

Very clever, right? Once light passes the point of no return, or Event Horizon, it is lost forever, however its outline can be studied – this is called the black hole’s shadow.
Scientists have well founded reasons to believe that at the center of the Milky Way, like in most galaxies, if not all actually, lies a supermassive black hole (one to four million times the mass of the sun). Estimated at 26,000 light years away, to have a chance at seeing it scientists say you’d need a very big telescope – a telescope the size of the entire Earth to be more exact.
Of course, there’s a solution around this – connecting the biggest and most powerful radio telescopes in the world together. As such, 50 radio telescopes scattered around the globe have joined the effort, including the Submillimeter Telescope (SMT) on Mt. Graham in Arizona, telescopes on Mauna Kea in Hawaii and the Combined Array for Research in Millimeter-wave Astronomy (CARMA) in California. The astronomers hope once the biggest telescope in the world, the Atacama Large Millimeter Array (ALMA) in Chile, is finished it will provide the necessary power to provide the project, the Event Horizon Telescope as it was dubbed, with a great chance of success.
“In essence, we are making a virtual telescope with a mirror that is as big as the Earth,” Doeleman said. “Each radio telescope we use can be thought of as a small silvered portion of a large mirror. With enough such silvered spots, one can start to make an image.”
“The Event Horizon Telescope is not a first-light project, where we flip a switch and go from no data to a lot of data,” he added. “Every year, we increase its capabilities by adding more telescopes, gradually sharpening the image we see of the black hole.”
General Relativity predicts that the bright outline defining the black hole’s shadow must be a perfect circle. If this shape will be found to be deviated in any manner, than it would prove that the Theory of Relativity is wrong. On the contrary, if it is indeed a circle, little doubt would be left to cast.
Bringing together radio telescopes around the globe requires an extraordinary global team effort, and I can only salute this initiative. What a milestone for science would it be if the researchers will manage to capture a black hole’s shadow.
“This is not only the usual international conference where people come from all over the world because they are interested in sharing their research,” Psaltis said. “For the Event Horizon Telescope, we need the entire world to come together to build this instrument because it is as big as the planet. People are coming from all over the world because they have to work on it.”
source

Thursday, June 23, 2011

SOLAR FLARE !!!

http://sdo.gsfc.nasa.gov/gallery/gallery/assets/preview/M2_CME.jpg

Please click and see the solar flare
read more here....
Read more here.....

A Solar Flare That Will Blow Your Socks Off


By now many of you who follow the Sun have probably heard about the “solar flare that will blow your socks off,” which occurred in early morning of Sunday June 7. Here at the Chandra X-ray Center we watched it too -- with some pride as our colleagues downstairs with the Solar Dynamics Observatory were responsible for some of the movies that were being circulated around the Internet. On the one hand, an M2 is a medium-sized event and not usually a big deal. On the other hand, I also thought of a slogan written on my whiteboard a few years ago, “West limb worry.”

Saturday, October 9, 2010

Really Heart Breaking !!! Aftermath of a Supernova

  • 327 is the aftermath of a star that exploded as a supernova.
  • In the composite, X-rays are blue, radio data are red and yellow, and infrared data show the stars in the field.
  • A rapidly spinning neutron star left behind is producing the wind of relativistic particles seen in X-rays.

G327.1-1.1 is the aftermath of a massive star that exploded as a supernova in the Milky Way galaxy. A highly magnetic, rapidly spinning neutron star called a pulsar was left behind after the explosion and is producing a wind of relativistic particles, seen in X-rays by Chandra and XMM-Newton (blue) as well as in the radio data (red and yellow). This structure is called a pulsar wind nebula. The likely location of the spinning neutron star is shown in the labeled version. The large red circle shows radio emission from the blast wave, and the composite image also contains infrared data from the 2MASS survey (red, green, and blue) that show the stars in the field.

Read  More about this by clicking below:

G327.1-1.1: Pushing the Envelope


Friday, April 23, 2010

TODAY'S NEWS THRO' PICTURES..

http://www.boston.com/bigpicture/

இன்றைய செய்தி படங்களின் வழியே தெரிந்துகொள்ள கிளிக்குங்கள்.

COURTESY: 







Saturday, June 20, 2009

Running Out of This World..News from NASA

06.15.2009
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June 15, 2009: International Space Station astronauts are getting a new toy in August – a treadmill. Famously named after comedian Stephen Colbert1, the new running machine will help astronauts stay fit, fighting off the bone loss and muscle decay2 that otherwise comes with space travel.
Just one problem: How do you run where there's no gravity to hold your feet to the ground?
"Bungee cords! You have to strap yourself to the treadmill," explains astronaut Sunita "Suni" Williams. And she's not joking.
In 2007, she ran the Boston Marathon on the station station's TVIS treadmill wrapped in bungee cords for the entire 26.2 mile race.
"It's not as bad as it sounds," she laughs.
Right: Suni Williams bungeed to the TVIS treadmill onboard the ISS. [more] [larger image]
TVIS stands for "Treadmill with Vibration Isolation System." It's the space station's original treadmill, designed to allow astronauts to run without vibrating delicate microgravity science experiments in adjacent labs. COLBERT, short for "Combined Operational Load Bearing External Resistance Treadmill", has a different kind of vibration-suppression system plus some other improvements3 for runners:
"I tried a COLBERT mockup at Johnson Space Center," says Williams. "It's broader than TVIS, so you don't have to watch out where your feet go. It allows a wider, more natural gait."
Williams spent a lot of time running during her six months on board the ISS, and she recalls what it's like:
Sign up for EXPRESS SCIENCE NEWS delivery "Just getting ready to run is a workout when you're weightless. Before all my training runs up there, I had to hook the toes of one foot under a handrail to keep from floating around while I struggled to put my sock and shoe on my other foot."
"I did this so often, it made calluses on top of my feet. Meanwhile, the calluses on the bottoms of my feet from running on Earth went away. It's totally upside down and backwards!" she laughs.
The treadmill's bungee harness "can be a bit uncomfortable," she continues. "During the marathon my foot sometimes went numb and tingly from the straps' pressure on my hip. Also, I had to use moleskin where the harness rubbed my neck raw."
And inside the close, still quarters of the space station, there are no gentle breezes to cool you down.
"Sweat globs onto you. It doesn't evaporate. I was soaking wet. During the marathon my hair was so sopping it flopped right in my face. We have little fans blowing on us but they don't do much good."
And Williams missed more than the soft winds of Earth.
"On Earth, the crowd cheers you on and you enjoy the camaraderie and support of the other runners. In space it's a little bit lonely. I was by myself most of race. My crewmates did cheer me through the last half hour to the finish. That was great!"
"Also, one of the Soyuz astronauts floated sweet, juicy pieces of oranges to me – so refreshing!"
Right: The official patch for "COLBERT," the Combined Operational Load Bearing External Resistance Treadmill, due to launch onboard shuttle Discovery as early as August 2009. [more] [larger image]
After the grueling run, Williams longed for a hot shower. "A sponge bath just isn't the same!" she says. Neither did she have a washer and dryer for cleaning her sweat-soaked running clothes. "I hung my drenched clothes near a fan and tied my sneakers to a handrail to air them out."
Williams is the only person to have run the Boston Marathon on Earth and in space—and she noted some interesting differences:
"I recovered faster after the space marathon. When you're floating, your muscles get to rest, so you can totally relax when you finish running – it's like being in a pool."
"Also, the space marathon didn't give me the same endorphin4 effect – that wonderful mood lift runners enjoy after running – as the Earth marathon did. I'm not sure why," she says. "We are loaded with only about 60% of our Earth weight on TVIS and its harness system, so maybe I just didn't work hard enough!"
Williams says she'd consider running another marathon on COLBERT. "If another astronaut challenges my time, maybe I’ll do it. I have a competitive nature."
When it comes to running, you could say "it's out of this world."
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Author: Dauna Coulter Editor: Dr. Tony Phillips Credit: Science@NASA
end notes
(1) Stephen Colbert hosts Comedy Central's "The Colbert Report." NASA chose the new treadmill’s name after he entered the Node 3 naming contest, asked his fans to post the name "Colbert," and won. NASA decided to honor him instead by naming the treadmill after him.
(2) Exercise is crucial to the astronauts' wellbeing. Without gravity, crewmembers lose bone and muscle mass and their cardiovascular system weakens. By exercising on COLBERT and other exercise devices, they can counteract these effects and keep their bodies in condition.
Williams says, "We need another treadmill up there. On the station, just like at the gym, sometimes you have to wait in line. The one of us in line will ask the one on the treadmill, 'When you gonna get off? I only have 30 minutes and I need to get on there.' COLBERT will allow more astronauts to get workouts more conveniently and frequently and longer."
(3) To create COLBERT, NASA started with a medical-grade treadmill -- the same kind used in most professional sports organization to train their athletes. Modifications included nickel plating the parts, changing the sheathing of the wires, and taking the rubber off the runner surface and anodizing it to give it texture for footing. The designers also developed a vibration isolation system for the new mill to prevent upsetting delicate science experiments. In addition, the engineers reinforced the rack that will hold the new treadmill, so sans mill it weighs about 2200 pounds -- much more than the rack on station now. Heavier mass makes it absorb loads better instead of passing them on to the space station itself. They also added special springs called ‘isolators’ that absorb impact. The combination of the springs and extra mass dampens out all the vibration from running. All of this is done without using any power.
Williams says: "Up on station, COLBERT won't sit on a gyro like TEVIS does. It took me a week to get used to running on TEVIS, which kind of floats on a gyro in a pit so you don't impart loads to the station. It makes it hard to get your balance. You feel kind of like a top, with the ground moving underneath you, until you get a rhythm going and get stabilized. COLBERT won’t be on a gyro so won’t require time to get used to. You can just hop on and run. It’s stiffer and feels more stable. It will also have programs to choose from: hill workouts, intervals etc. Not just manual. That will had variety and make for some more intense workouts, which will help improve our fitness and bone density more."
(4) For more information about running and endorphins, see http://www.nytimes.com/2008/03/27/health/nutrition/27best.html
NASA's Future: US Space Exploration Policy

Monday, May 11, 2009

A planetary Nebula Kohotek 4-55 , 4600 light years away


This Hubble image of planetary nebula Kohoutek 4-55 was taken by the Wide Field and Planetary Camera 2 on May 4, 2009. The colors represent the makeup of the various emission clouds in the nebula: red represents nitrogen, green represents hydrogen, and blue represents oxygen. K 4-55 is nearly 4,600 light-years away in the constellation Cygnus. Credit: NASA/ESA/JPL

Courtesy: NASA