X-ray AstROnomy - McGill University Astrophysics and Cosmology
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Transcript X-ray AstROnomy - McGill University Astrophysics and Cosmology
Vicky Kaspi
McGill University
Lorne Trottier Chair in Astrophysics and Cosmology
X-RAY ASTRONOMY:
UPCOMING MISSIONS
Overview
Introduction to X-ray astronomy
NuSTAR
Astro-H
NICER
Other missions
Astronomy with X-rays
The most energetic, violent
Optical sky: calm, unchanging
objects in the Universe
produce X-rays
Black holes, neutron stars
Active galaxies, galaxy clusters
The X-ray sky highly volatile:
objects explode,
appear/disappear daily
Extremes of:
Gravity
Density
Temperature
Magnetic field
Magnetic Explosions on a Neutron Star:
Less calm, highly variable
X-ray Astronomy: Space-based
X-ray Telescopes: Space-Based
Must be in space
as X-rays cannot
penetrate atmosphere
X-rays hard to focus!
Need special telescope
geometries, materials
Chandra X-ray Telescope
Focusing X-rays
Currently Flying X-ray Telescopes
XMM-Newton
Chandra
MAXI
NuSTAR
Suzaku
Swift
X-ray Sources
Stellar mass black holes and neutron star
accreting from companion stars
Isolated neutron stars like pulsars & magnetars
Supernova remnants
Active galactic nuclei
Galaxy clusters
Next: High Energy Groove
NASA Outreach movie: made & performed by astronomers,
factually accurate, artist & real data combined, clearly illustrates
changing X-ray sky, note McGill’s contribution!
High Energy Groove
Currently Flying X-ray Telescopes
XMM-Newton
Chandra
MAXI
NuSTAR
Suzaku
Swift
Launched June 2012
NASA’s NuSTAR: The Future is Now!
Launched June 14, 2012
First focusing “hard” X-
ray telescope
“hard” = high-energy
5-80 keV
~100X more sensitive
Yesterday
than previous hard X-ray
telescopes
10-m focal length: long!
How to launch??
Today
NuSTAR: Newest X-ray Telescope
NuSTAR in Space
NuSTAR Pegasus Launch
For more on NuSTAR & its science goals
see poster by Dr. Hongjun An
NuSTAR First Light: Cyg X-1
Astro-H: Launch 2015
Next major X-ray
mission
Joint JAXA/NASA with
international
involvement including
Canadian Space Agency
Complex mission with
4 different instruments
Astro-H: Broad energy response
Multiple instruments:
Soft X-ray Spectrometer
0.3-12 keV, 1.7’ angular resolution, 7 eV@ 6 keV
Hard X-ray Imagers
5-80 keV, 1.7’ angular resolution, 1.5 keV @ 60 keV
Soft X-ray Imager
0.4-12 keV, 1.7’ angular resolution
Soft Gamma-Ray Detector
40-600 keV, non-imaging
All instruments co-aligned:
observers get data from all detectors.
Astro-H
Takahashi et al. 2010
Astro-H Canadian Involvement
Top recommendation
of CSA-sponsored report
Ottawa-based NEPTEC
building laser metrology
system
CSA cost $6M
Canadians leading
multiple SWGs
Canadians have access to
PV data and propose
for Japanese time
Astro-H Science Goals
Large Scale Structure in the Universe, Dark
Matter & Dark Energy
Galaxy Cluster dynamics, evolution
Supermassive black hole evolution
Extreme Conditions in the Universe
Motion of matter near black holes
Shock acceleration, jets
Neutron star spectra, binaries
NEW! NASA’s NICER
Neutron Star Internal
Composition Explorer
Approved for
construction Apr 5!
To be installed on
International Space
Station
Expected launch
December 2016
Deputy PI Z.
Arzoumanian,
McGill Physics Alum!
International Space Station
FRAM = Flight Releasable Attachment Mechanism
ELC = ExPRESS Logistics Carrier (power, telemetry)
Gendreau et al. 2012
NICER Science Goals
Low energy (0.2-12 keV) X-ray mission tailored for
understanding neutron star structure, composition
Factor of ~2 more sensitive than current most
sensitive XMM-Newton
Gendreau et al. 2012
NICER: Combined Capability
Unique capability
combination:
Sensitivity
Time resolution
Energy resolution
Will allow detailed
observations of
emission from
neutron stars’ surfaces
constraints on
unknown properties of
ultradense matter
Gendreau et al. 2012
Upcoming & Envisioned
X-ray Missions
Upcoming:
ASTROSAT
ASTROSAT – Indian mission with significant CSA
eRosita
involvement; 5 instruments; launch 2014?
e-ROSITA – German instrument to launch on Russian
Spectrum Roentgen Gamma mission in 2014; will do all
sky survey in soft X-ray band
HMXT – 1st Chinese astronomy satellite, non-imaging
20-200 keV; launch 2014-2016
ATHENA
Envisioned:
ATHENA – ESA Advanced Telescope for High-Energy
Astrophysics; formerly Constellation-X, Xeus, IXO
high throughput (3 m2) X-ray spectroscopy + WFI
LOFT – ESA Large Observatory for X-ray Timing
LAD 12 m2 for timing; WFM large FOV
LOFT
Summary
Near-term X-ray astronomy healthy
Multiple major missions flying, several interesting
upcoming missions planned
Long-term situation unclear:
2 major ESA concepts being promoted
Good news: CSA already cooperates with ESA
Bad news: CSA presently in state of flux
No major NASA X-ray mission under development
US budgetary constraints problematic
NASA “Physics of the Cosmos” Program charged with
identifying next X-ray advance…
Stay tuned!