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Newborn. Astronomers have spied magnetic activity surrounding a massive young star in the Orion Nebula (inset), a hot spot of such activity in the Milky Way. Credit: Bill Saxton, NRAO/AUI/NSF; (inset) NASA/ESA/M. Robberto (STScI/ESA) Birth of a (Magnetic) HeavyweightBy Phil Berardelli The death of massive stars is reasonably well known--most blow their innards across galaxies in titanic explosions called supernovae--but their birth is another story. Solar giants are relatively rare, and they form inside giant clouds of gas and dust that block the view of optical telescopes. Lucky for astronomers, they managed to look at just the right patch of sky with a powerful new observing tool. That patch is located about 1300 light-years away, within the Great Nebula of the constellation Orion. Inside a vast cloud of dust and gas that is known as one of the Milky Way galaxy's premier star-hatcheries, the team found a zone emitting strong radio waves with the chemical signature of silicon monoxide gas, a strong indicator that the starmaking process is at work. The researchers then trained the Very Long Baseline Array of radio telescopes--a line of dishes that stretches about 8000 kilometers, from Mauna Kea, Hawaii, to St. Croix in the U.S. Virgin Islands--on the source of the gas, an object they called Source I (pronounced "source eye"). The scopes picked out thousands of these silicon monoxide clouds, which they liken to lasers because they emit radio waves as bright pinpoints. Astronomers call them masers. The researchers wanted to see if they could track the masers over time. So they took 21 monthly shots of the surrounding cloud and its masers between March 2001 and December 2002 and compiled a time-lapse movie.
This item requires the Flash plug-in (version 8 or higher). JavaScript must also be enabled in your browser. Please download the latest version of the free Flash plug-in. Credit: L. Matthews/MIT Slice of life. This time-lapse sequence shows a baby star both pulling in and ejecting its raw material. Many astronomers had thought that magnetic fields would be too weak in young stars--particularly young massive stars--to influence their development. But lately some observational evidence has been collected, and Source I represents the first time that astronomers have caught a glimpse of the process at work. Astronomer Daniel Apai of the Space Telescope Science Institute in Baltimore, Maryland, likens the tracks of the masers to "rising steam that reveals the boiling water as it swirls around a drain." The amount of detail and complexity in the images "will allow us to test in detail our models of the birth of the hottest and most massive stars," he says.
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