Suggested Searches

1 min read

Warped Disk Around a Bright Black Hole

Warped Disk Around a Bright Black Hole

This diagram shows the geometry of a warped disk of dust surrounding a suspected black hole in the active galaxy NGC 6251. The diagram is based on NASA Hubble Space Telescope images of the disk which reveal that only one side reflects light emitted from a suspected black hole, hence the disk is warped.

Such a warp could be due to gravitational perturbations in the galaxy's nucleus that keep the disk from being perfectly flat, or from precession of the rotation axis of the black hole relative to the rotation axis of the galaxy.

Perpendicular to the disk is a jet of high-energy particles blasted into space along the black hole's spin axis.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    16h 32m 31.63s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    82° 32' 16.29"
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    NGC 6251
  • Release Date
    September 10, 1997
  • Science Release
    Hubble Finds a Bare Black Hole Pouring Out Light
  • Credit
    James Gitlin (STScI)

Downloads

  • 800 × 582
    jpg (19.58 KB)
  • 200 × 200
    jpg (5.02 KB)

Share

Details

Last Updated
Mar 28, 2025
Contact
Media

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