PIA17567: Different Flavors of Black Holes
 Mission:  NuSTAR
 Instrument:  NuSTAR
 Product Size:  3300 x 2800 pixels (w x h)
 Produced By:  JPL
JPL News Release 2014-010
 Full-Res TIFF:  PIA17567.tif (27.73 MB)
 Full-Res JPEG:  PIA17567.jpg (545.3 kB)

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Original Caption Released with Image:

A range of supermassive black holes lights up this new image from NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR. All of the dots are active black holes tucked inside the hearts of galaxies, with colors representing different energies of X-ray light.

The red, yellow and green colors represent black holes seen previously by NASA's Chandra X-ray Observatory (with red denoting the lowest-energy X-ray light). The color blue shows black holes recently detected by NuSTAR, which was uniquely designed to detect the highest-energy X-ray light. The black holes in this picture are between about 3 to 10 billion light-years away.

Why do some black holes produce more high-energy X-ray light than others? Astronomers say this is because the black holes are more actively feeding off surrounding clouds of dust and gas, and also because the material surrounding them is so dense that only high-energy X-ray photons can penetrate the thick screen.

NuSTAR is the first telescope capable of imaging obscured black holes at this distance using high-energy X-rays; previous telescopes operating in a similar energy range would not have been able to discern the separate host galaxies. One of the goals of the NuSTAR mission is to pinpoint the different types of distant black holes that are contributing to a diffuse X-ray glow in our sky, what is called the X-ray background. This will reveal new details about the evolution of both black holes and the galaxies that house them.

The image shows an area, called the COSMOS field, that has been studied in great detail by many telescopes (COSMOS stands for Cosmic Evolution Survey). Red and green represent X-ray light seen by Chandra with energies of 0.5 to 2 kiloelectron volts (keV), and 2 to 7 keV, respectively. Blue is 8 to 24 keV, which can only be seen by NuSTAR.

NuSTAR is a Small Explorer mission led by the California Institute of Technology in Pasadena and managed by NASA's Jet Propulsion Laboratory, also in Pasadena, for NASA's Science Mission Directorate in Washington. The spacecraft was built by Orbital Sciences Corporation, Dulles, Va. Its instrument was built by a consortium including Caltech; JPL; the University of California, Berkeley; Columbia University, N.Y.; NASA's Goddard Space Flight Center, Greenbelt, Md.; the Danish Technical University in Denmark; Lawrence Livermore National Laboratory, Livermore, Calif.; ATK Aerospace Systems, Goleta, Calif., and with support from the Italian Space Agency (ASI) Science Data Center, Rome, Italy.

NuSTAR's mission operations center is at UC Berkeley, with ASI providing its equatorial ground station located at Malindi, Kenya. The mission's outreach program is based at Sonoma State University, Rohnert Park, Calif. NASA's Explorer Program is managed by Goddard. JPL is managed by Caltech for NASA.

For more information, visit http://www.nasa.gov/nustar and http://www.nustar.caltech.edu/.

Image Credit:
NASA/JPL-Caltech/Yale University

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