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Paris, France (SPX) Oct 24, 2008 Sounding the Sun through a technique similar to seismology has opened a new era for understanding the Sun's interior. The CNES/ESA COROT satellite has now applied this technique to three stars, directly probing the interiors of stars beyond the Sun for the first time. When global oscillations of the Sun were discovered, scientists realised they opened a window to the Sun's interior. Like the propagation of seismic waves on Earth providing information about our planet's interior, sound waves travel throughout the Sun carrying information about what is happening below the surface. These oscillations can also be observed on other stars. They can be detected through the variation in the light emitted by the star as the surface wobbles - the technique used by COROT. This reveals the internal structure of the star, and the way energy is transported from the core to the surface. "Other techniques to estimate stellar oscillations have been used from the ground, but they are limited in what they can do," said Malcolm Fridlund, ESA Project Scientist for COROT at ESA's European Space Research and Technology Centre (ESTEC), in the Netherlands, and co-author of the results. "Adverse weather conditions, plus the fact that you cannot observe stars during daytime, oblige ground astronomers to interrupt their observations," he continued. "Now, the key to detecting such small stellar oscillations from big distances is not only the sensitivity of an instrument, but also the opportunity of observing the star without interruption: any interruption produces noise in the data that can cover a signal completely. Therefore, to be certain, we must approach the question with the right instruments and from space." The three stars probed by COROT - known as HD499933, HD181420 and HD181906 - are similar to the Sun. They are not exactly in our stellar neighbourhood, but rather far away, so their brightness doesn't blind COROT's instruments. "The fact that COROT succeeded in probing the interior of Sun-like stars with direct measurements for the first time is a huge leap in understanding stars in general", added Fridlund. "In addition, this will help us to understand, by comparison, our own Sun even better." Community Email This Article Comment On This Article Share This Article With Planet Earth
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Huntsville AL (SPX) Oct 03, 2008Scientists using NASA's RHESSI spacecraft have measured the roundness of the sun with unprecedented precision, and they find that it is not a perfect sphere. During years of high solar activity the sun develops a thin "cantaloupe skin" that significantly increases its apparent oblateness. |
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