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M87

M87
This radio image of the galaxy M87, taken with the Very Large Array (VLA) radio telescope in February 1989, shows giant bubble-like structures where radio emission is thought to be powered by the jets of subatomic particles coming from the the galaxy's central black hole. The false color corresponds to the intensity of the radio energy being emitted by the jet. M87 is located 50 million light-years away in the constellation Virgo.
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    M87
  • Release Date
    October 27, 1999
  • Science Release
    Very Long Baseline Array Reveals Formation Region of Giant Cosmic Jet Near a Black Hole
    Read the release
  • Credit
    Credit: National Radio Astronomy Observatory/National Science Foundation

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Related Images & Videos

Close-Up Look at a Jet Near a Black Hole

Close-Up Look at a Jet Near a Black Hole

[top left] - This radio image of the galaxy M87, taken with the Very Large Array (VLA) radio telescope in February 1989, shows giant bubble-like structures where radio emission is thought to be powered by the jets of subatomic particles coming from the the galaxy's central black...

Black Hole in Galaxy M87 Emits Jet of High-Speed Electrons

Black Hole in Galaxy M87 Emits Jet of High-Speed Electrons

A visible light image of the giant elliptical galaxy M87, taken with NASA Hubble Space Telescope's Wide Field Planetary Camera 2 in February 1998, reveals a brilliant jet of high-speed electrons emitted from the nucleus (diagonal line across image). The jet is produced by a...

M87

M87

A Very Long Baseline Array (VLBA) radio image of the region close to the black hole, where an extragalactic jet is formed into a narrow beam by magnetic fields. The false color corresponds to the intensity of the radio energy being emitted by the jet. The red region is about...

At the Source of an Extragalactic Jet

At the Source of an Extragalactic Jet

Artist's concept of the formation region of M87's jet. An accretion disk (red-yellow) surrounds the black hole, and its magnetic field lines twist tightly to channel the outpouring subatomic particles into a narrow jet. The jet opens widely near the black hole, then is shaped...

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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

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