Black Hole-Powered Jet of Electrons and Sub-Atomic Particles Streams From Center of Galaxy M87

Stsci_2000-20a_1024

stsci_2000-20a July 6th, 2000

Credit: NASA and The Hubble Heritage Team (STScI/AURA)

Streaming out from the center of the galaxy M87 like a cosmic searchlight is one of nature's most amazing phenomena, a black-hole-powered jet of electrons and other sub-atomic particles traveling at nearly the speed of light. In this NASA Hubble Space Telescope image, the blue of the jet contrasts with the yellow glow from the combined light of billions of unseen stars and the yellow, point-like globular clusters that make up this galaxy. At first glance, M87 (also known as NGC 4486) appears to be an ordinary giant elliptical galaxy; one of many ellipticals in the nearby Virgo cluster of galaxies. However, as early as 1918, astronomer H.D. Curtis noted a "curious straight ray" protruding from M87. In the 1950s when the field of radio was blossoming, one of the brightest radio sources in the sky, Virgo A, was discovered to be associated with M87 and its jet. After decades of study, prompted by these discoveries, the source of this incredible amount of energy powering the jet has become clear. Lying at the center of M87 is a supermassive black hole, which has swallowed up a mass equivalent to 2 billion times the mass of our Sun. The jet originates in the disk of superheated gas swirling around this black hole and is propelled and concentrated by the intense, twisted magnetic fields trapped within this plasma. The light that we see (and the radio emission) is produced by electrons twisting along magnetic field lines in the jet, a process known as synchrotron radiation, which gives the jet its bluish tint. M87 is one of the nearest and is the most well-studied extragalactic jet, but many others exist. Wherever a massive black hole is feeding on a particularly rich diet of disrupted stars, gas, and dust, the conditions are right for the formation of a jet. Interestingly, a similar phenomenon occurs around young stars, though at much smaller scales and energies. At a distance of 50 million light-years, M87 is too distant for Hubble to discern individual stars. The doz

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2000/news-2000-20

Curator: STScI, Baltimore, MD, USA

Image Use Policy: http://hubblesite.org/copyright/

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Image Details Image Details

Image Type
Observation
Object Name
M87 NGC 4486
Subject - Local Universe
Galaxy > Type > Elliptical
Galaxy > Activity > AGN
Nebula > Type > Jet

Distance Details Distance

Universescale2
50,000,000 light years
Stsci_2000-20a_128
 

Position Details Position Details

Position (ICRS)
RA = 12h 30m 48.6s
DEC = 12° 23’ 31.0”
Orientation
North is 65.3° CW
Field of View
0.5 x 0.5 arcminutes
Constellation
Virgo

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Magenta Hubble (WFPC2) Ultraviolet (U) 300.0 nm
Blue Hubble (WFPC2) Optical (B) 450.0 nm
Green Hubble (WFPC2) Optical (V) 606.0 nm
Red Hubble (WFPC2) Infrared (I) 814.0 nm
Spectrum_base
Magenta
Blue
Green
Red
Stsci_2000-20a_1280
×
ID
2000-20a
Subject Category
C.5.1.4   C.5.3.2   C.4.1.5  
Subject Name
M87, NGC 4486
Credits
NASA and The Hubble Heritage Team (STScI/AURA)
Release Date
2000-07-06T00:00:00
Lightyears
50,000,000
Redshift
50,000,000
Reference Url
https://hubblesite.org/contents/news-releases/2000/news-2000-20
Type
Observation
Image Quality
Good
Distance Notes
Distance in Lightyears
Facility
Hubble, Hubble, Hubble, Hubble
Instrument
WFPC2, WFPC2, WFPC2, WFPC2
Color Assignment
Magenta, Blue, Green, Red
Band
Ultraviolet, Optical, Optical, Infrared
Bandpass
U, B, V, I
Central Wavelength
300, 450, 606, 814
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
187.70244020361, 12.39194282361
Reference Dimension
1222.00, 1276.00
Reference Pixel
528.12812641439, 654.57041667814
Scale
-0.00000696589, 0.00000696589
Rotation
-65.27749865173
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
World Coordinate System resolved using PinpointWCS 0.9.2 revision 218+ by the Chandra X-ray Center FITS X FITS Y EPO X EPO Y 282.38 508.60 333.75 234.66 409.53 436.84 567.16 406.68 255.08 649.79 58.33 301.08 388.47 542.15 361.16 454.95 Center Pixel Coordinates: 611.00 187.70209303651 638.00 12.39242928506
Creator (Curator)
STScI
URL
http://hubblesite.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
Address
3700 San Martin Drive
City
Baltimore
State/Province
MD
Postal Code
21218
Country
USA
Rights
http://hubblesite.org/copyright/
Publisher
STScI
Publisher ID
stsci
Resource ID
STSCI-H-p0020a-f-1222x1276.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p0020a-f-1222x1276.tif
Related Resources
http://hubblesite.org/newscenter/archive/releases/2000/20
Metadata Date
2022-07-06T00:00:00
Metadata Version
1.2
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Detailed color mapping information coming soon...

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Universescalefull
50,000,000 light years

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