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The finding relates to research on medium-size stars, scientists said. The results will "shed light on a long-standing mystery about stars like our own sun," according to a statement by the European Southern Observatory, which operates the Very Large Telescope. The results come from data collected by the UVES spectrograph on the telescope.
The scientists will share their discovery and discuss its implications
The optical surface of the Sun (the photosphere) is known to have a temperature of approximately 6,000 K. Above it lies the solar corona, rising to a temperature of 1,000,000–2,000,000 K.[70] The high temperature of the corona shows that it is heated by something other than direct heat conduction from the photosphere.
The results will "shed light on a long-standing mystery about stars like our own sun," according to a statement by the European Southern Observatory, which operates the Very Large Telescope.
An international team led by astronomers from the University of São Paulo in Brazil has used the UVES spectrograph on ESO’s Very Large Telescope to shed light on a long-standing mystery about stars like our own Sun.
The Institute of Astronomy, Geophysics, and Atmospheric Sciences (IAG) at the University of São Paulo (USP) in Brazil, in collaboration with the European Southern Observatory, will hold a press conference to announce the results and assess their implications, offering journalists the opportunity to discuss with and interview the scientists.
The conference will be held on 28 August 2013, at 10:30 local time (BRT) and will take place in Portuguese with a summary in English.
The Very Large Telescope array (VLT) is the flagship facility for European ground-based astronomy at the beginning of the third Millennium. It is the world's most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter and four movable 1.8m diameter Auxiliary Telescopes. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Originally posted by wildespace
reply to post by eriktheawful
UVES is a spectrograph, so I assume that the study is more about chemical composition.
Originally posted by whatnext21
...I haven't a clue what this could divulge but the words 'Major' and 'implications' have grabbed my attention.
Originally posted by IkNOwSTuff
Im gonna guess it will be exciting if your an astronomer, otherwise it will be "huh!!!!! How is that important?"
I hope Im wrong
Originally posted by kaleshwarchand777
Anyone found any announcement in regards to this??
Originally posted by IkNOwSTuff
Yep, just as predicted not at all exciting outside of astronomy circles.
These nerds need to get a grip and stop getting the general public excited about what basically amounts to nothing.
Why they felt this needed any sort of build up or pre announcement is beyond me