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The sun is nearly the roundest object ever measured. If scaled to the size of a beach ball, it would be so round that the difference between the widest and narrow diameters would be much less than the width of a human hair.
It rotates every 28 days, and because the sun doesn’t have a solid surface, it should be slightly flattened. This tiny flattening has been studied with many instruments for almost 50 years to learn about the sun’s rotation, especially the rotation below its surface, which can’t be seen directly.
University of Hawaiʻi at Mānoa Institute for Astronomy’s Jeff Kuhn and Isabelle Scholl, Stanford University’s Rock Bush and Universidade Estadual de Ponta Grossa’s Marcelo Emilio used the Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory satellite to obtain what they believe is the definitive, and baffling, answer. Their research was published in Science Express.
Because there is no atmosphere in space to distort the solar image, the researchers were able to use HMI’s exquisite image sensitivity to measure the solar shape with unprecedented accuracy. The results indicate that if the sun were shrunk to a ball one meter in diameter, its equatorial diameter would be only 17 millionths of a meter larger than the diameter through its North-South pole, which is its rotation axis.
They also found that the solar flattening is remarkably constant over time and too small to agree with that predicted from its surface rotation. This suggests that other subsurface forces, like solar magnetism or turbulence, may be a more powerful influence than expected.
“For years we’ve believed our fluctuating measurements were telling us that the sun varies, but these new results say something different,” said Kuhn, the team leader and first author. “While just about everything else in the sun changes along with its 11-year sunspot cycle, the shape doesn’t.”
A University of Hawaiʻi at Mānoa Institute for Astronomy news release