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Optical-to-Ultraviolet Spectrum of Markarian 231

Optical-to-Ultraviolet Spectrum of Markarian 231
This simplified spectral plot shows the radiation emitted from the center of a nearby galaxy that hosts a quasar. Visible and infrared light coming from a disk surrounding a central black hole in the middle of the galaxy is measured. Surprisingly, ultraviolet light from the disk, as measured by the Hubble Space Telescope, shows a drop in radiation from the disk. This is evidence for a large gap in the center of the disk that is likely carved out by a second black hole orbiting the primary black hole.

About the Data

  • Data Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
    The Hubble image was created using HST data from proposal 10592: A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University). The galaxy pair was imaged with the ACS/WFC instrument with filters F435W (B) and F814W (I) on May 10, 2002. The science team comprises: C.-S. Yan and Y. Lu (National Astronomical Observatories, Chinese Academy of Sciences, Beijing), X. Dai (University of Oklahoma), and Q. Yu (Peking University).
  • Release Date
    August 27, 2015
  • Science Release
    Hubble Finds That the Nearest Quasar Is Powered by a Double Black Hole
  • Credits
    NASA, ESA, and P. Jeffries (STScI)

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Details

Last Updated
Feb 17, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov