Massive Dark Objects Detected in Galaxies
Galaxy | Const | Type | Distance | Luminosity | Mass | Comment |
---|---|---|---|---|---|---|
Milky Way | [Sgr] | Sbc | 0.028 | 1.9 | 2 | Sgr A, Galactic Center |
M31 | And | Sb | 2.9 | 5.2 | 30 | Andromeda Galaxy |
M32 | And | E2 | 2.9 | 0.25 | 3 | Satellite of M31 |
NGC 3115 | Sex | SO | 27 | 14.2 | 2 | |
M 106 | CVn | Sbc | 24 | 1.3 | 40 | Maser Detection |
NGC 4261 | Vir | E2 | 90 | 33 | 400 | |
M87 | Vir | E0 | 60 | 56 | 3000 | |
M104 | Vir | Sa | 50 | 47 | 1000 | Sombrero Galaxy |
NGC 3377 | Leo | E5 | 38 | 5.2 | 100 | |
M105 | Leo | E1 | 38 | 13 | 50 | |
NGC 4486B | Vir | E0 | 60 | 0.82 | 500 | Satellite of M87 |
M77 | Cet | Sb | 60 | Caltech IR detection | ||
M84 | Vir | S0 | 60 | 56 | 300 | HST STIS (May 1997) |
Key:
- Galaxy
- Identification/Catalog number of galaxy
- Const
- Constellation
- Type
- Hubble type
- Distance
- Distance in million light years (of massive dark object)
- Luminosity
- Galaxy luminosity in billion solar luminosities; bulge only for spirals
- Mass
- Dark Object Mass in million solar masses
- Comments
- Common name of galaxy or other comment
This table summarizes data for some of the well-established massive dark
objects in the nuclei of galaxies. The masses of these objects are usually
estimated from the orbital velocity of stars or gas orbiting the objects at
distances of some tens or hundreds of light years, which shows that enormous
masses are concentrated in small volumes. Many of these central objects
exhibit other signs of violent gravitational action: Accretion disks,
emission of strong radio and/or high-energy radiation, or jets of highly
accelerated material.
What may be the nature of these mysterious objects ?
Many astronomers take it for granted that these objects are supermassive
black holes, but none of them is really resolved. To get truely compelling
evidence, or better, to reveal the true nature of the massive dark objects,
a resolution would be required of the order of the Schwarzschild radius
(the “horizon” radius of a black hole acording to Einstein’s General
Relativity theory). The Schwarzschild radius is simply correlated to the
mass of an object, as it is defined as that radius where the escape velocity
from the mass equals light velocity; this means that it is propoertional to
the mass. The formal relation can be given as
R_S = 2.94 km * M [solar masses]
Even for the most massive central object (in M87), this yields a value of
R_S = 9 billion km, little more than the mean distance of Pluto to the sun
and only about 1/1000 of a light year, while the Hubble Space Telescope
could only resolve this object to a few tens of light years. So currently,
any evidence is indirect at best. It is particularly exaggerated to take
our current knowledge of these objects as a further evidence for the
validity of Einstein’s General Relativity, as was occasionally claimed.
The table above is partly based on
Last Modification: 14 Feb 1998, 17:30 MET