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Future of Astronomy Astronomy 315 Professor Lee Carkner Lecture 25
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Yerkes Observatory 1897
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The Future of Astronomy What would we like to understand better? Formation of initial galaxies Properties and numbers of extrasolar planets Formation and evolution of black holes
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Problems and Solutions We want to study fainter objects We want better detail We want to study a broad range of astrophysical phenomena Use multiwavelength telescopes
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Key Initiatives While much science is done with small and common instruments, there are several large and expensive new projects that we hope will lead to big breakthroughs Three of these are: A Giant Segmented Mirror Telescope
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Webb Space Telescope See earliest galaxies View protoplanetary disks View planets To be launched in June 2014 Cost: 4.5 billion dollars
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Webb Format Want to be both high performance and “cheap” Telescope needs to be cool and so is deployed away from Earth with a large sun shield To get large mirror to fit in small launch vehicle, mirror folds up
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International X-ray Observatory Joint venture of NASA, ESA, and JAXA Would have collecting area ~10 times larger than current X-ray telescopes Would be able to get high resolution X-ray spectra of: Black hole accretion disks Hot interstellar X-ray gas Launch: 2020?
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Telescope Properties The light gathering power of a telescope depends on its area Area = r 2 The resolution of a telescope depends on its diameter (d) and the wavelength ( ) of light observed R = (1.22 ) / d Determines how close two objects can be and still be resolved (smaller R is better)
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Future Ground Based Telescopes Larger size means spectroscopy and imaging of fainter objects Extremely Large Telescopes
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Current Plans California universities are building the Thirty Meter Telescope (TMT) The ESO has plans for the European Extremely Large Telescope (E-ELT) of 42 meters Each will cost about 1 billion dollars
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Extremely Large Telescopes Success of large telescopes depends on adaptive optics ELT’s would complement space telescopes For follow up observations that require greater sensitivity
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Hobby Eberly Telescope 1997
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Telescope Trends 21 st century astronomy versus 20 th century astronomy: Information technology integral
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Next Time Meet in planetarium No homework or downloads
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