Concepts for Future High-Energy Astrophysics Missions
This page lists high energy astrophysics mission concepts that are candidates
to be in the programs of national or international space agencies. More
information on mission studies under NASA's Physics of the Cosmos (PCos)
program office is available at the Physics of the Cosmos web site. In 2011 NASA HQ initiated an X-ray
mission concepts study through the NASA Physics of the Cosmos Program.
The final report of this study listed a number of notional missions,
including a notional calorimeter mission (N-CAL), a notional X-ray grating
spectrometer, AXSIO (see below), a notional wide-field imager (N-WFI), and
various combinations of these capabilities on a single platform.
US (often with international partners)
Advanced Energetic Pair Telescope, a concept for a pair production
telescope for medium-energy gamma-ray polarimetry designed to
achieve angular resolution within a factor of two of the pair production
kinematics limit (~0.6 degrees at 70 MeV), continuum sensitivity comparable
with the Fermi-LAT front detector, and minimum detectable polarization
less than 10% for a 10 mCrab source in 106 seconds.
Arcus, a concept for an X-ray grating spectrometer mission to
be deployed on the International Space Station, with a spectral resiolution of
2800 and an effective area of ~800 sq. cm at the critical O VII wavelength
near 21 A, with an overall bandpass from 8-52 A, enabling a wide range of
EPE: Extreme Physics Explorer: a concept for a
timing/spectroscopy mission that would use micro-channel plate optics
(MCPO) to provide 4 m2 effective area focused to ~1
arc-min onto an X-ray calorimeter.
Energetic X-ray Imaging Survey Telescope, a hard X-ray (5-600 keV)
imaging all-sky deep survey mission that will use a coded-mask
high-energy telescope (HET) with imaging CZT detectors to image
sources such as AGN, black hole transients, etc., in a 70 by 90
degree field of view with 2 arcminute resolution; an accompanying
optical/IR telescope (OIT) will enable multiwavelength studies and
prompt follow-up of gamma-ray bursts.
The Generation X-Ray Mission, a large effective area (50 square
meters at 1 keV,
or 500 x Chandra) X-ray telescope to study the new frontier of
astrophysics: the birth and evolution of the first stars, galaxies,
and black holes in the early Universe.
HEX-P: High-Energy X-ray Probe, a concept for a probe-class
next-generation high-energy X-ray mission with broadband (0.1-200
keV) response and ~40 times the sensitivity of previous missions
above 10 keV.
IXPE: Imaging X-ray Polarimetry Explorer:
a concept for a highly sensitive x-ray polarimeter with imaging
capability sensitive enough to measure X-ray (linear) polarization
for a broad range of cosmic sources, primarily those involving neutron
stars, stellar black holes, and supermassive black holes (AGN).
a concept for a low-cost, wide-field X-ray transient mission on the
International Space Station, with 30 x higher sensitivity compared to
BAT, ASM, MAXI, and designed for transient study of black holes,
neutron Stars, GRBs, etc.
a concept for a rapid response mission to study the warm-hot
intergalactic medium using
GRBs as its probes, as well as to study the host galaxies of GRBs
and the phyics of GRBs.
WFXT: Wide-Field X-ray Telescope, a proposed mission with
an effective area 10 times Chandra's which will perform
surveys of the sky in the soft X-ray band (0.4-6 keV).
Xenia: a Probe of Cosmic Chemical Evolution, a concept
for a medium-size cosmology mission (with international collaborators)
which will use gamma-ray
bursts to probe the cosmic 'web', dark energy, dark matter, and
clusters of galaxies.
Multinational and International
Transient Astrophysics Explorer is a
mission concept to detect and locate X-ray transients (XRT's), likely
including gravitational wave sources, TDE's, gamma-ray bursts, etc.,
using a wide-FOV coded mask instrument (Owl) to detect XRT's and a sensitive
wide-field focussing soft X-ray instrument (Lobster) to obtain arcminute
or better positions [Europe]
Athena, an X-ray observatory proposed as a concept for a
large effective area
mission for the ESA science program, incorporating a single telescope
with a fixed focal length (12 m) and two interchangeable instruments
in the focal plane, a wide-field imager (WFI) and an X-ray integral
field unit (X-IFU), i.e., an X-ray calorimeter. On Nov 28th, 2013, ESA
selected the science theme "The Hot and Energetic Universe" for
its next large satellite mission (L2), and on Jun 27th, 2014, it
selected Athena as the mission for this theme, with a target launch
date of 2028 [ESA]
DAMPE: Dark Matter Particle
Explorer, a mission which will search for dark matter in the universe
and also study cosmic ray acceleration and propagation, by detecting
high-energy (5 GeV - 10 TeV) gamma rays and electrons, as well as cosmic rays
with energies in the range from 100 GeV to 100 TeV [China]
LOFT: Large Observatory For X-ray Timing, a newly
proposed space mission intended to answer fundamental questions about the
motion of matter orbiting close to the event horizon of a black hole, and the
state of matter in neutron stars, using a highly capable 10 sq. meter
broad-band (1 - 80 keV) X-ray telescope with 10 μs timing resolution.
PheniX, a very-broad-band (1-200 keV) high spectral-resolution
(<~ 0.5 keV) focussing X-ray telescope able to do Compton polarimetry
for E > 50 keV, and a coded-mask all-sky monitor [Multi-national]
XIPE: the X-ray Imaging Polarimetry Explorer, a mission
to do cosmic polarimetry in the 2-10 keV band, as well as solar
flare polarimetry in the 15-35 keV band and solar coronal spectroscopy
in the 1.2-15 keV band [Multi-national]