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Past ...future? NASA's Great Observatories 'an astronomica

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Title: Past ...future? NASA's Great Observatories 'an astronomica


1
HUBBLE
Past future?
2
Spitzer
Chandra
NASAs Great Observatories an astronomical
Mount Rushmore
Compton
Hubble
3
Gains in orbit
  • No atmospheric blurring
  • Wider accessible wavelength range
  • Instrumental stability
  • No clouds/daylight (timing)

4
Some HST Science highlights
  • Structures of distant galaxies

5
Some HST Science highlights
  • Structures of distant galaxies
  • Hubble constant from Cepheid variable stars

6
Some HST Science highlights
  • Structures of distant galaxies
  • Hubble constant from Cepheid variable stars
  • Black holes in (almost all) galactic nuclei

7
Some HST Science highlights
  • Structures of distant galaxies
  • Hubble constant from Cepheid variable stars
  • Black holes in (almost all) galactic nuclei
  • Protoplanetary material near young stars

8
Some HST Science highlights
  • Structures of distant galaxies
  • Hubble constant from Cepheid variable stars
  • Black holes in (almost all) galactic nuclei
  • Protoplanetary material near young stars
  • Gravitational lenses

9
Some HST Science highlights
  • Structures of distant galaxies
  • Hubble constant from Cepheid variable stars
  • Black holes in (almost all) galactic nuclei
  • Protoplanetary material near young stars
  • Gravitational lenses
  • Intergalactic gas and its history
  • Stuff scattered all the way through the textbooks

10
Instrument history
  • 1990 FGS HSP FOS GHRS FOC
    WF/PC
  • 1993 FGS CoSTAR FOS GHRS FOC WFPC2
  • FGS CoSTAR NICMOS STIS FOC WFPC2
  • 2002 FGS CoSTAR NICMOS STIS ACS WFPC2
  • 200? COS, WFC3

11
Hubble status, Sept. 2004
  • Space Telescope Imaging Spectrograph dead
  • (only high-res/small-region spectrometer)
  • 3 of 6 gyros (RSUs) functional (3 needed for full
    tracking, some observations with 2)
  • Battery capacity decreasing (will be useless
    circa 2010)
  • Estimated 50 failure time on above 2007
  • Instrument/transmitter power cycling now reduced
    by rescheduling/eliminating parallel imaging

12
Options
  • Shuttle SM4 (OKeefe ruled out, CAIB concerns)
  • Robotic mission (new tech, some changeouts very
    risky)
  • Replace the whole thing (HOP proposal to refly
    COS/WFC3)

13
Shuttle?
  • Safe haven would mean standby orbiter
  • Limited remaining flights earmarked to ISS
  • Need for independent orbital inspection
  • Victim of the Vision?
  • Orbital mechanics 28.5-degree inclination,
    getting heaviest payloads highest from Cape
    Canaveral, restricts options now

14
Servicing non-options
  • Prohibitive energy requirements to co-orbit with
    ISS in reach of astronauts
  • 28-degree orbit out of reach from Baikonur (ITAR
    restrictions aside)
  • Ion thrusters would take the estimated telescope
    lifetime for orbit change
  • 2015 estimated deorbit without boosting

15
Robotics/teleoperation?
  • Canadian ISS arm not required yet spare
  • Some tasks straightforward, actually robotic plus
    teleoperations mission
  • Double big/small arm
  • Robot docking/deorbit committed already
  • Tests make this look possible
  • 2-piece spacecraft, Delta/Atlas launch
  • 2007 a challenge budget is ballooning
  • Political aspects re pinning blame

16
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17
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18
Solar array connectors
19
Replace capabilities?
  • Technology since 1980 lots cheaper. Thin
    flexible mirrors, lightweight structures,
    stabilize mirrors rather than structure
  • Unique access to optical/UV range
  • Plan on table to fly 2.4m mirror with existing
    HST instruments (Hubble Origins Probe or HOP)
    could be as low as 250M.
  • Need to decide who gets the instruments!

20
Next up JWST
21
James Webb Space Telescope
  • Launch 2011, on Ariane V, to L2 region
  • 6.5m deployable primary
  • 0.6-20 microns (far red to mid-IR)
  • Key problems formation of galaxies, first stars,
    maybe planets
  • Spacecraft weight/mirror area ratio roughly that
    of Hubble mirror alone!

22
And at other wavelengths
Chandra and its complement XMM-Newton
23
Across the spectrum -
now FarIR MidIR nearIR opt UV farUV X-ray
gamma
FUSE
INTEGRAL
Spitzer
GALEX
WMAP
Hubble
Chandra
24
Multispectral Greatest Hits
  • Intergalactic gas
  • Starburst galaxies
  • High-redshift galaxies
  • Evaporating planets
  • Protoplanetary disks
  • Growth of black holes
  • Complexity of stardeath
  • Gamma-ray bursts
  • Supernova chemistry
  • Quasar jets
  • Stripped galaxies
  • Pregalactic lumps
  • Galaxy history
  • Relativistic jets

25
A panchromatic view -spiral galaxy M81
ROSAT GALEX Kitt Peak Spitzer VLA
26
Across the spectrum -
soon FarIR MidIR nearIR opt UV farUV X-ray
gamma
FUSE?
JWST
INTEGRAL
Spitzer
Swift
GALEX?
Planck
Hubble?
Chandra and XMM
SIM TPF?
Herschel
27
A new Universe to explore
  • The full electromagnetic spectrum
  • Open international competition for observations
  • Public data archives (without mailing tapes!)
  • The beginnings of the Virtual Observatory
  • But astronomers think about facilities
    differently from NASA and ESA
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