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Artist’s View of Black Hole and Companion Star GRO J1655-40

Artist's View of Black Hole and Companion Star GRO J1655-40
GRO J1655-40 is the second so-called 'microquasar' discovered in our Galaxy. Microquasars are black holes of about the same mass as a star. They behave as scaled-down versions of much more massive black holes that are at the cores of extremely active galaxies, called quasars. Astronomers have known about the existence of stellar-mass black holes since the early 1970s. Their masses can range from 3.5 to approximately 15 times the mass of our Sun. Using Hubble data, astronomers were able to describe the black-hole system. The companion star had apparently survived the original supernova explosion that created the black hole. It is an aging star that completes an orbit around the black hole every 2.6 days. It is being slowly devoured by the black hole. Blowtorch-like jets (shown in blue) are streaming away from the black-hole system at 90 percent of the speed of light.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    16h 54m 0.13s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -39° 50' 44.9"
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    GRO J1655-40
  • Release Date
    November 18, 2002
  • Science Release
    Fast-Flying Black Hole Yields Clues to Supernova Origin
  • Credit
    Illustration Credit: ESA, NASA, and Felix Mirabel (French Atomic Energy Commission and Institute for Astronomy and Space Physics/Conicet of Argentina)

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Details

Last Updated
Mar 28, 2025
Contact
Media

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