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.
BHI: Black Hole Imager: an X-ray mission which will
directly resolve the event horizons of black holes.
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.
EREXS: Epoch of Reionization Energetic X-ray Survey,
a mission concept to study the birth and growth of the first black
holes, as well as to perform a multiwavelength time domain
astrophysics survey of a wide range of objects.
EXIST:
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.
Gen-X:
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.
NICER: Neutron star Interior Composition exploreR, a
proposed
instrument on the ISS consisting of an array of 56 X-ray telescopes
to study the time variability of the emission from X-ray pulsars,
thereby deriving information on their radii and masses which
will tightly constrain the neutron stars' equation of state. NICER
was selected in the Explorer 2011 AO as a 'mission of opportunity'
for evaluation as a potential future space mission and was
selected for Phase B in April 2013.
Pharos:
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.
SMART-X: Square Meter, Arcsecond Resolution X-ray Telescope,
a mission concept for a 2.3 m2 effective area, 0.5 arcsecs
angular resolution X-ray telescope, with a 5 arcmins FOV, 1 arcsec
pixel size microcalorimeter, 22 arcmins FOV imager, and
high-throughput gratings.
WFXIS: Wide-Field X-ray Imaging Spectrometer, a proposed
mission to provide wide-field X-ray imaging spectroscopy with
both high energy resolution (~ 5 eV) and high angular resolution
(~ 10 arcsecs).
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
ATHENA+, an X-ray observatory to be proposed as a large
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. ATHENA+ is a new
version of the previously proposed ATHENA: The Advanced Telescope for High Energy Astrophysics
[ESA], which itself superceded the joint ESA/JAXA/NASA concept, IXO: International X-ray
Observatory)
Dark Matter Satellite will search for dark matter in the
universe and study cosmic ray acceleration [China]
EDGE: Explorer of Diffuse emission and Gamma ray burst
Explosions, a mission with a high (< 3 eV) spectral resolution
wide field spectrometer (WFS), together with a wide (1.4-degree
diameter) field imager (WFI), a very wide (1/4 of the sky) field
monitor (WFM) and a gamma-ray burst detector (GRBD) [Europe]
GRAVITAS: General Relativistic Astrophysics Via Timing and
Spectroscopy, a large (1.5 m2) effective area, moderate
(125 eV) spectral resolution, high (100 µs) temporal
resolution broad (0.1 - 10 keV) band X-ray mission targetted at
studies of the Fe K line region at 6.4 keV in compact objects
[Europe]
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]