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Published byAbraham Glenn Modified over 9 years ago
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Russian 6-m Nasmyth focus platforms Problems: 17-ton mirror has thermal time constant of a few days; location based on politics. Note alt-az mount
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Enormous telescopes of the Future TMT = Ten Meter Telescope (US) OWL = Overwhelmingly Large telescope, 100m
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The rest of the spectrum Space-based observatories needed Radio requires special telescopes
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IRAS = InfraRed Astronomical Satellite – early NASA
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IUE = International Ultraviolet Explorer—another…
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Russian 6-m Nasmyth focus platforms Problems: 17-ton mirror has thermal time constant of a few days; location based on politics. Note alt-az mount
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NASA’s Great Observatories
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HST = Hubble Space Telescope
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Compton Gamma Ray Observatory (GRO) Mission now over
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Chandra X-Ray Satellite
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SIRTF = Space Infra-Red Telescope Facility launched a year ago Renamed the Spitzer Space Telescope
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James Webb Next Generation Space Telescope > 20-ft diameter Named after 2 nd NASA administrator; built by TRW L 2 Lagrange point for Earth-Sun system (thus 10 6 times closer to us than sun – mass ratio…), or 940,000 miles from us. (Sun-stationary)
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Karl Jansky’s Rotating Antenna (Bell Labs, 1931) Saw a sidereal period (~23 h 56 m ) signal
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Typical Radio Astronomy Telescope Why so large? ….
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Resolution of telescopes Angular resolution depends on telescope diameter (D) and signal wavelength (λ): Rayleigh criterion: Θ min ~ λ / D
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Some numbers … For optical wavelengths, Θ in arc-seconds, and D in inches it works out to Θ min ~ 4.5 / D Example: for your 8-inch telescopes, Θ min ~ 4.5 / 8 = 0.56 arc-sec (note signs…)
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Schematic Today: a computer
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Green Bank, WV
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aricebo
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Interferometry
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VLA = Very Large Array (NM)
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VLBA = Very Long Baseline Array
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PARI = Pisgah Astronomical Research Institute
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