PIA18467: Big, Spinning Black Hole Blurs Light
 Mission:  NuSTAR
 Instrument:  NuSTAR
 Product Size:  3300 x 2550 pixels (w x h)
 Produced By:  IPAC-Caltech
 Full-Res TIFF:  PIA18467.tif (25.26 MB)
 Full-Res JPEG:  PIA18467.jpg (349.5 kB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

This plot of data captured by NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR, shows X-ray light streaming from regions near a supermassive black hole known as Markarian 335. The light is coming from two areas: a superheated disk of material feeding the black hole, called the accretion disk; and a cloud of particles traveling near the speed of light, called the corona. The exact shape and nature of coronas are not clear, but researchers know that X-ray light from the corona is reflected off the accretion disk.

That reflected light, and the corona's direct light, are mapped in this plot over a range of X-ray energies. (This is the highest range of X-rays, which NuSTAR was specially designed to see.) The yellow line is a model that shows what the data are predicted to look like if X-ray light has been stretched, or blurred. The blue line shows what the plot would look like without the blurring effects. The white dots show the actual NuSTAR data, indicating the light is extremely blurred.

What's blurring the light? It's a combination of factors. First, there is a Doppler shift happening due to the spinning disk. As one side of the disk moves toward us and the other side away, the light is squeezed or stretched. A second effect has to do with the enormous speeds of the spinning black hole, which approach the speed of light. A final effect is from the enormous gravity of the black hole, which pulls on the light, making it harder to escape its grasp. The light loses energy in this process. All of these factors contribute to the smeared look of the data as seen in the plot.

These data were taken after a dramatic dip in brightness had first been observed by NASA's Swift satellite. NuSTAR's high-energy X-ray data pointed to the cause for the observed change: Markarian 335's corona had shifted closer to the black hole itself -- and this closer proximity meant that the black hole's gravity could yank harder on the corona's light, stretching it to lower energies than observed before. The astronomers say that the corona moved over a period of days, and is still in the close configuration. They don't know if and when it would move back to where it was previously, or why the corona moved. NuSTAR and other high-energy telescopes are busy trying to crack these mysteries.

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/Institute for Astronomy, Cambridge

Image Addition Date: