Asteroid To Give Earth A Record Setting Close Shave On February 15

Credit: NASA
Talk about a close shave. On Feb. 15th an asteroid about half the size of a football field will fly past Earth only 17,200 miles above our planet's surface. There's no danger of a collision, but the space rock, designated 2012 DA14, has NASA's attention. Since regular sky surveys began in the 1990s, astronomers have never seen an object so big come so close to our planet. "This is a record-setting close approach," says Don Yeomans of NASA's Near Earth Object Program at JPL. "Since regular sky surveys began in the 1990s, we've never seen an object this big get so close to Earth." Earth's neighborhood is littered with asteroids of all shapes and sizes, ranging from fragments smaller than beach balls to mountainous rocks many kilometers wide. Many of these objects hail from the asteroid belt, while others may be corpses of long-dead, burnt out comets. NASA's Near-Earth Object Program helps find and keep track of them, especially the ones that come close to our planet. 2012 DA14 is a fairly typical near-Earth asteroid. It measures some 50 meters wide, neither very large nor very small, and is probably made of stone, as opposed to metal or ice. Yeomans estimates that an asteroid like 2012 DA14 flies past Earth, on average, every 40 years, yet actually strikes our planet only every 1200 years or so. The impact of a 50-meter asteroid is not cataclysmic--unless you happen to be underneath it. Yeomans points out that a similar-sized object formed the mile wide Meteor Crater in Arizona when it struck about 50,000 years ago. "That asteroid was made of iron," he says, "which made it an especially potent impactor." Also, in 1908, something about the size of 2012 DA14 exploded in the atmosphere above Siberia, leveling hundreds of
square miles of forest. Researchers are still studying the "Tunguska Event" for clues to the impacting object. "2012 DA14 will definitely not hit Earth," emphasizes Yeomans. "The orbit of the asteroid is known well enough to rule out an impact." In this oblique view, the path of near-Earth asteroid 2012 DA14 is seen passing close to Earth on Feb. 15, 2013. Even so, it will come interestingly close. NASA radars will be monitoring the space rock as it approaches Earth closer than many man-made satellites. Yeomans says the asteroid will thread the gap between low-Earth orbit, where the ISS and many Earth observation satellites are located, and the higher belt of geosynchronous satellites, which provide weather data and telecommunications. "The odds of an impact with a satellite are extremely remote," he says. Almost nothing orbits where DA14 will pass the Earth. NASA's Goldstone radar in the Mojave Desert is scheduled to ping 2012 DA14 almost every day from Feb. 16th through 20th. The echoes will not only pinpoint the orbit of the asteroid, allowing researchers to better predict future encounters, but also reveal physical characteristics such as size, spin, and reflectivity. A key outcome of the observing campaign will be a 3D radar map showing the space rock from all sides. During the hours around closest approach, the asteroid will brighten until it resembles a star of 8thmagnitude. Theoretically, that’s an easy target for backyard telescopes. The problem, points out Yeomans, is speed. “The asteroid will be racing across the sky, moving almost a full degree (or twice the width of a full Moon) every minute. That’s going to be hard to track.” Only the most experienced amateur astronomers are likely to succeed. Those who do might experience a tiny chill when they look at their images. That really was a close shave. For more information about 2012 DA14 and other asteroids of interest, visit NASA’s Near-Earth Object Program web site: http://neo.jpl.nasa.gov, Author: Dr. Tony Phillips |Production editor: Dr. Tony Phillips | Credit: Science@NASAAsteroid To Give , Source: Nano Patents And Innovations
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Vampire stars suck life from their neighbours

Light Echoes Red Supergiant Star V838 Monocerotis oct02
Star V838 Monocerotis's (V838 Mon) light echo, which is about six light years in diameter, is seen from the Hubble space telescope in this in this February 2004 handout photo released by NASA. It became the brightest star in the Milky Way Galaxy in January 2002 when its outer surface greatly expanded suddenly. 
An international team of astronomers has spotted a strange phenomena called as vampire stars, where a smaller companion star sucks matter off the surface of its larger neighbour using the very large telescope in Chile. They looked at what are known as O-type stars, which have very high temperature, mass and brightness. These stars have short and violent lives and play a key role in the evolution of galaxies. “These stars are absolute behemoths. They have 15 or more times the mass of our Sun and can be up to a million times brighter. These stars are so hot that they shine with a brilliant blue-white light and have surface temperatures over 30,000C,” the Daily Mail quoted Hugues Sana, from the University of Amsterdam, Netherlands, who is the lead author of the study, as saying. The astronomers studied a sample of 71 O-type single stars and stars in pairs (binaries) in six nearby young star clusters in the Milky Way. Most of the observations in their study were obtained using ESO telescopes, including the VLT. By analysing the light coming from these targets in greater detail than before, the team discovered that 75 per cent of all O-type stars exist inside binary systems, a higher proportion than previously thought, and the first precise determination of this number. Mergers between stars, which the team estimates will be the ultimate fate of around 20-30 per cent of O-type stars, are violent events. But even the comparatively gentle scenario of vampire stars, which accounts for a further 40-50 per cent of cases, has profound effects on how these stars evolve. Until now, astronomers mostly considered that closely-orbiting massive binary stars were the exception, something that was only needed to explain exotic phenomena such as X-ray binaries, double pulsars and black hole binaries. The new study shows that to properly interpret the Universe, this simplification cannot be made: these heavyweight double stars are not just common, their lives are fundamentally different from those of single stars. For instance, in the case of vampire stars, the smaller, lower-mass star is rejuvenated as it sucks the fresh hydrogen from its companion. Its mass will increase substantially and it will outlive its companion, surviving much longer than a single star of the same mass would. The victim star, meanwhile, is stripped of its envelope before it has a chance to become a luminous red super giant. Instead, its hot, blue core is exposed. As a result, the stellar population of a distant galaxy may appear to be much younger than it really is: both the rejuvenated vampire stars, and the diminished victim stars become hotter, and bluer in colour, mimicking the appearance of younger stars. Knowing the true proportion of interacting high-mass binary stars is therefore crucial to correctly characterise these faraway galaxies. The only information astronomers have on distant galaxies is from the light that reaches our telescopes. Without making assumptions about what is responsible for this light we cannot draw conclusions about the galaxy, such as how massive or how young it is. According to Sana, this study shows that the frequent assumption that most stars are single can lead to the wrong conclusions. Source: Hindustan TimesImage: flickr.com
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