Astrophysics in the 21st Century - PowerPoint PPT Presentation

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Astrophysics in the 21st Century

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SWIFT (multi-l) investigating g-ray bursts. GAIA, FAME (Hipparcos) ... No atmosphere / weather / moonlight. Better, faster and cheaper. Scientific breakthroughs ... – PowerPoint PPT presentation

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Title: Astrophysics in the 21st Century


1
Astrophysics in the 21st Century
2
Current directions in Space Science
General purpose, high-specification
  • Chandra
  • Astro-E
  • XMM (multi-l)
  • Integral
  • NGST
  • FIRST
  • XEUS
  • Constellation-X
  • LISA

XMM
3
Current directions in Space Astronomy
Themed observatories
  • SWIFT (multi-l) investigating g-ray
    bursts
  • GAIA, FAME (Hipparcos) mapping the Galaxy
  • Planck (COBE) measuring the CMB

4
Directions in the future
  • Increasing trend for themed missions
  • NASAs Great Observatories and ESAs
    Cornerstone Missions
  • Multi-l observatories
  • Better, faster and cheaper
  • Throughput
  • Spectral and spatial resolution
  • Timing
  • Broadband simultaneity
  • Photometric conditions
  • No atmosphere / weather / moonlight

5
Scientific breakthroughs
Spectral throughput spatial
  • Cosmology
  • Relativity
  • Astroparticle physics
  • XEUS launch 2010
  • 1-10eV resolution over 0.1-30keV
  • 100x deeper than XMM
  • 2 HEW _at_1keV

6
Scientific breakthroughs
Spectral throughput spatial
Simulation of XEUS spectrum of OVIII line at
0.65keV in AR Lac. 100 sec exposure
7
Scientific breakthroughs
Spatial throughput spectral
Image of the supernova remnant Cassiopeia A taken
with the Chandra spacecraft. 1 resolution. Shows
filaments of iron, silicon and sulphur and
absorption by dusty gas.
Also evolution of clusters, galaxies quasars
8
Scientific breakthroughs
Timing throughput spectral
Mapping structures in binary systems and the
geometry of the complex gas distributions in AGN
9
Astronomers wishlist
  • Multi-l data now essential for many classes of
    object
  • High throughput 100x XMM from XEUS in 10 years
  • Spectral resolution eg a few eV over 0.1-50
    keV
  • Spatial resolution 1/10 arcsec in EUV/X-rays
  • Timing resolution - millisecs for bright
    sources
  • priority for all missions
  • Essential for high-res timing and spectroscopy
  • Conveyor-belt approach (eg Constellation-X)
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