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Encyclopedia > Virgo A Galaxy
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The jet emitted by M87 in this image is thought to be caused by a supermassive black hole at the galaxy's center.
Observation data
Type E1
Right ascension (RA, α) 12 h 30.8 m (J2000,00)
Declination (Dec, δ) +12° 24' (J2000,00)
Distance from Earth 60 millions LY
(18.4 Mpc)
Apparent magnitude (V)  +8.6m
Apparent dimension(s) (V)  7.0'
Physical characteristics
Mass (Sun=1) > 1.0 × 1012
Diameter 120,000 light years
Absolute magnitude -22m
Peculiarities

-Radio emission
-jet from galaxy core
-huge (13,000)
globular cluster system

Other denominations

NGC 4486
Virgo A radio source
Arp 152

Elliptical Galaxy M87 (also known as the Virgo A Galaxy, Virgo A, Messier Object 87, Messier 87, M87, or NGC 4486) is a giant elliptical galaxy dominating the Virgo cluster. It is one of the biggest known galaxies. Its relative closeness makes it a preferred target for studying the high-energy activities currently going on in its nucleus, suspected of holding a supermassive black hole. Astronomers believe that the black hole in this galaxy is approximately of 3×109 solar masses.


Related topics

External link

  • Messier 87 (http://www.seds.org/messier/m/m087.html), SEDS Messier pages

  Results from FactBites:
 
Galaxy - Wikipedia, the free encyclopedia (2686 words)
Most galaxies are several thousand to several hundred thousand light years in diameter and are usually separated from one another by distances on the order of millions of light years.
Galaxies that emit high-energy radiation in the form of x-rays are classified as Seyfert galaxies, quasars and blazars.
Active galaxies that emit radio frequencies from relativistic jets erupting from the core are classified as Radio galaxies.
  More results at FactBites »


 
 

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