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
Enormous telescopes of the Future TMT = Ten Meter Telescope (US) OWL = Overwhelmingly Large telescope, 100m
The rest of the spectrum Space-based observatories needed Radio requires special telescopes
IRAS = InfraRed Astronomical Satellite – early NASA
IUE = International Ultraviolet Explorer—another…
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
NASA’s Great Observatories
HST = Hubble Space Telescope
Compton Gamma Ray Observatory (GRO) Mission now over
Chandra X-Ray Satellite
SIRTF = Space Infra-Red Telescope Facility launched a year ago Renamed the Spitzer Space Telescope
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)
Karl Jansky’s Rotating Antenna (Bell Labs, 1931) Saw a sidereal period (~23 h 56 m ) signal
Typical Radio Astronomy Telescope Why so large? ….
Resolution of telescopes Angular resolution depends on telescope diameter (D) and signal wavelength (λ): Rayleigh criterion: Θ min ~ λ / D
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…)
Schematic Today: a computer
Green Bank, WV
aricebo
Interferometry
VLA = Very Large Array (NM)
VLBA = Very Long Baseline Array
PARI = Pisgah Astronomical Research Institute