Make your own free website on Tripod.com

Galaxies and Actual Clusters

 

The actual galaxies are classified as ellipticals (like M87), spirals (like the Milky Way or the Andromeda galaxy), lenticulars (endowed with a disk but missing spiral arms) and irregulars (like M82 in Ursa Majoris), being the spirals split in ordinary and barred spirals. Each spiral is still classified according to the proportional size that the central bulge assumes in the galactic bulk (bigger bulges imply smaller paces of stellar formation, closer to those seen in the ellipticals) and each elliptical according to the more or less pronounced flatness (disproportion between the bigger and the smaller axis). The galaxies may still be classified according to their size, like the dwarfs (with diameters measuring a few hundred light years), the giants (with halos that may reach millions light years and overlay the neighbouring galaxies' halos) or intermediate sized galaxies like the Milky Way.

 

E0-E7 (to the left): ellipticals, S0 (in the intersection): lenticulars, Sa-Sc (at the top): ordinary spirals, SBa-SBc (at the bottom): barred spirals (MoonRunner Design UK)

 

M87 in the centre or the Virgo cluster: giant elliptical galaxy (AAO)

 

 

Sombrero: lenticular galaxy (AAO)

 

 

M83: spiral galaxy (AAO)

 

 

NGC1365: barred spiral galaxy (AAO)

 

 

Evolutionary Divergences between Spirals and Ellipticals

 

The Collapse Velocity

One model advocates that what determined the split between spiral and elliptical galaxies was the velocity at which the proto-galactic clouds collapsed, which was in turn controlled by the speed of the conversion of the gas into stars.

In spiral galaxies, the rotation provides to the matter of the disk a centrifugal force that prevents it (like those located outside the rotation plane) from directly falling into the core, contrarily to what happens to the materials located outside the rotation plane. This way, this kind of galaxies gradually assumes a discoid shape.

Bu, if the galactic gas is quickly transformed into stars, the collapse of the outer layers of the galaxy is braked much earlier, no matter the distance at which they are from the rotation plane.

 

Alternative Models

An alternative theory defends that some elliptical galaxies might have been formed as a consequence of collisions between spirals, which can eventually be supported in some observations that suggest the existence of a higher proportion of spiral galaxies in the primitive Universe than in the actual one. The observation of a higher proportion of ellipticals in the dense cores of the galactic clusters also supports this idea. The collisions between galaxies are also a mechanism invoked to explain the formation of irregular galaxies.

Recently it has been also advocated that the arising of a spiral or an elliptical galaxy may depend on the speed at which the supermassive black holes are formed in its interior.

 

 

Distribution of the Galaxies

 

The galaxies tend to concentrate in clusters that in turn tend to concentrate in galactic superclusters.

 

The Local Group

The Milky Way belongs to the so-called Local Group, which also includes the spiral galaxies of Andromeda (the only big galaxy that, in the expanding Universe, gets closer to the Milky Way) and Triangulum, along with other galaxies with smaller dimensions, like the Magellanic Clouds.

 

The Large Magellanic Cloud, a member of the Local Group: an irregular galaxy (AAO)

 

Classification and Stratification of the Clusters

Among the clusters two types can be distinguished:

    1. The regular clusters, with a central core and a well-defined spherical structure. Its dimensions may vary between 3 and 30 million light years.
    2. The irregular clusters, like the Virgo cluster, missing a well-defined centre and with similar dimensions, though more rarefied.

As it was already mentioned, the elliptical galaxies tend to concentrate and to be more massive in the clusters' cores, in opposition to the spirals, which prevail in the outskirts.

 

The Virgo cluster (Cambridge Cosmology)

 

Superclusters

The superclusters are huge structures containing several clusters and may reach dimensions of about 300 million light years, like the one in Coma Berenices. The supercluster to which the Milky Way belongs is called the supercluster of Virgo and is more modest, with an extension of about 50 million light years. About 90% of all the galaxies are detected inside this kind of structures.

 

The Coma Berenices cluster, which is the core of the supercluster named after it (Cambridge Cosmology)

 

Filaments and Big Voids

At an even larger scale we find galaxies distributed along long sheets or filaments, bordered by big voids that hold average dimensions of about 75 million light years, but some of them, like the Bootes void, may reach more than 400 million light years. It's estimated that the big voids occupy about 90% of the space.

 

Structure of the Universe in a large scale, where are visible the long filaments and the big voids (CfA)

 

The Size of the Universe

At last, if the inflation theory of Alan Guth is true, it is estimated that the whole Universe may be about 1050 times bigger than the visible Universe (which is a sphere extending as far as about 13,7 billion light years from us). If, however, it is confirmed that the Universe is open, then it shall assume an infinite size.

 

 

Return to the previous page

_